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123 <title>Lorentzian Quantum Gravity and the Graviton Spectral Function</title>
124 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.081501</link>
125 <description>Author(s): Jannik Fehre, Daniel F. Litim, Jan M. Pawlowski, and Manuel Reichert<br/><p>We present the first direct and nonperturbative computation of the graviton spectral function in quantum gravity. This is achieved with the help of a novel Lorentzian renormalization group approach, combined with a spectral representation of correlation functions. We find a positive graviton spectra…</p><br/>[Phys. Rev. Lett. 130, 081501] Published Fri Feb 24, 2023</description>
126 <content:encoded><![CDATA[<p>Author(s): Jannik Fehre, Daniel F. Litim, Jan M. Pawlowski, and Manuel Reichert</p><p>We present the first direct and nonperturbative computation of the graviton spectral function in quantum gravity. This is achieved with the help of a novel Lorentzian renormalization group approach, combined with a spectral representation of correlation functions. We find a positive graviton spectra…</p><br/><p>[Phys. Rev. Lett. 130, 081501] Published Fri Feb 24, 2023</p>]]></content:encoded>
127 <dc:title>Lorentzian Quantum Gravity and the Graviton Spectral Function</dc:title>
128 <dc:creator>Jannik Fehre, Daniel F. Litim, Jan M. Pawlowski, and Manuel Reichert</dc:creator>
129 <dc:date>2023-02-24T10:00:00+00:00</dc:date>
130 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
131 <dc:source>Phys. Rev. Lett. 130, 081501 (2023)</dc:source>
132 <dc:type>article</dc:type>
133 <dc:identifier>doi:10.1103/PhysRevLett.130.081501</dc:identifier>
134 <prism:doi>10.1103/PhysRevLett.130.081501</prism:doi>
135 <prism:publicationName>Physical Review Letters</prism:publicationName>
136 <prism:volume>130</prism:volume>
137 <prism:number>8</prism:number>
138 <prism:publicationDate>2023-02-24T10:00:00+00:00</prism:publicationDate>
139 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.081501</prism:url>
140 <prism:startingPage>081501</prism:startingPage>
141 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
142 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
143 </item>
144 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.081401">
145 <title>Nonlinear Effects in Black Hole Ringdown</title>
146 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.081401</link>
147 <description>Author(s): Mark Ho-Yeuk Cheung, Vishal Baibhav, Emanuele Berti, Vitor Cardoso, Gregorio Carullo, Roberto Cotesta, Walter Del Pozzo, Francisco Duque, Thomas Helfer, Estuti Shukla, and Kaze W. K. Wong<br/><p>Simulations show that nonlinear spacetime dynamics manifest in the postmerger gravitational-wave signal of binary black hole coalescence.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.081401.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 130, 081401] Published Wed Feb 22, 2023</description>
148 <content:encoded><![CDATA[<p>Author(s): Mark Ho-Yeuk Cheung, Vishal Baibhav, Emanuele Berti, Vitor Cardoso, Gregorio Carullo, Roberto Cotesta, Walter Del Pozzo, Francisco Duque, Thomas Helfer, Estuti Shukla, and Kaze W. K. Wong</p><p>Simulations show that nonlinear spacetime dynamics manifest in the postmerger gravitational-wave signal of binary black hole coalescence.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.081401.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 130, 081401] Published Wed Feb 22, 2023</p>]]></content:encoded>
149 <dc:title>Nonlinear Effects in Black Hole Ringdown</dc:title>
150 <dc:creator>Mark Ho-Yeuk Cheung, Vishal Baibhav, Emanuele Berti, Vitor Cardoso, Gregorio Carullo, Roberto Cotesta, Walter Del Pozzo, Francisco Duque, Thomas Helfer, Estuti Shukla, and Kaze W. K. Wong</dc:creator>
151 <dc:date>2023-02-22T10:00:00+00:00</dc:date>
152 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
153 <dc:source>Phys. Rev. Lett. 130, 081401 (2023)</dc:source>
154 <dc:type>article</dc:type>
155 <dc:identifier>doi:10.1103/PhysRevLett.130.081401</dc:identifier>
156 <prism:doi>10.1103/PhysRevLett.130.081401</prism:doi>
157 <prism:publicationName>Physical Review Letters</prism:publicationName>
158 <prism:volume>130</prism:volume>
159 <prism:number>8</prism:number>
160 <prism:publicationDate>2023-02-22T10:00:00+00:00</prism:publicationDate>
161 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.081401</prism:url>
162 <prism:startingPage>081401</prism:startingPage>
163 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
164 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
165 </item>
166 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.081402">
167 <title>Nonlinearities in Black Hole Ringdowns</title>
168 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.081402</link>
169 <description>Author(s): Keefe Mitman, Macarena Lagos, Leo C. Stein, Sizheng Ma, Lam Hui, Yanbei Chen, Nils Deppe, François Hébert, Lawrence E. Kidder, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, and Nils L. Vu<br/><p>Simulations show that nonlinear spacetime dynamics manifest in the postmerger gravitational-wave signal of binary black hole coalescence.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.081402.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 130, 081402] Published Wed Feb 22, 2023</description>
170 <content:encoded><![CDATA[<p>Author(s): Keefe Mitman, Macarena Lagos, Leo C. Stein, Sizheng Ma, Lam Hui, Yanbei Chen, Nils Deppe, François Hébert, Lawrence E. Kidder, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, and Nils L. Vu</p><p>Simulations show that nonlinear spacetime dynamics manifest in the postmerger gravitational-wave signal of binary black hole coalescence.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.081402.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 130, 081402] Published Wed Feb 22, 2023</p>]]></content:encoded>
171 <dc:title>Nonlinearities in Black Hole Ringdowns</dc:title>
172 <dc:creator>Keefe Mitman, Macarena Lagos, Leo C. Stein, Sizheng Ma, Lam Hui, Yanbei Chen, Nils Deppe, François Hébert, Lawrence E. Kidder, Jordan Moxon, Mark A. Scheel, Saul A. Teukolsky, William Throwe, and Nils L. Vu</dc:creator>
173 <dc:date>2023-02-22T10:00:00+00:00</dc:date>
174 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
175 <dc:source>Phys. Rev. Lett. 130, 081402 (2023)</dc:source>
176 <dc:type>article</dc:type>
177 <dc:identifier>doi:10.1103/PhysRevLett.130.081402</dc:identifier>
178 <prism:doi>10.1103/PhysRevLett.130.081402</prism:doi>
179 <prism:publicationName>Physical Review Letters</prism:publicationName>
180 <prism:volume>130</prism:volume>
181 <prism:number>8</prism:number>
182 <prism:publicationDate>2023-02-22T10:00:00+00:00</prism:publicationDate>
183 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.081402</prism:url>
184 <prism:startingPage>081402</prism:startingPage>
185 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
186 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
187 </item>
188 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.081403">
189 <title>Silicon Oxy-Nitride for the Low Refractive Index Layers in the Mirror Coatings of the Cryogenic Laser Interferometer Gravitational Waves Detector</title>
190 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.081403</link>
191 <description>Author(s): Shiuh Chao, Wen-Jie Tsai, Dong-Lin Tsai, I-Peng Chang, Qian-Yi Hong, Wei-Chih Chang, and Yu-Hsun Kao<br/><p>The low refractive index layers in the mirror coatings of the room-temperature laser interferometer gravitational waves detectors are silica deposited by the ion beam sputter method. However, the silica film suffers from the cryogenic mechanical loss peak, hindering its application for the next gene…</p><br/>[Phys. Rev. Lett. 130, 081403] Published Wed Feb 22, 2023</description>
192 <content:encoded><![CDATA[<p>Author(s): Shiuh Chao, Wen-Jie Tsai, Dong-Lin Tsai, I-Peng Chang, Qian-Yi Hong, Wei-Chih Chang, and Yu-Hsun Kao</p><p>The low refractive index layers in the mirror coatings of the room-temperature laser interferometer gravitational waves detectors are silica deposited by the ion beam sputter method. However, the silica film suffers from the cryogenic mechanical loss peak, hindering its application for the next gene…</p><br/><p>[Phys. Rev. Lett. 130, 081403] Published Wed Feb 22, 2023</p>]]></content:encoded>
193 <dc:title>Silicon Oxy-Nitride for the Low Refractive Index Layers in the Mirror Coatings of the Cryogenic Laser Interferometer Gravitational Waves Detector</dc:title>
194 <dc:creator>Shiuh Chao, Wen-Jie Tsai, Dong-Lin Tsai, I-Peng Chang, Qian-Yi Hong, Wei-Chih Chang, and Yu-Hsun Kao</dc:creator>
195 <dc:date>2023-02-22T10:00:00+00:00</dc:date>
196 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
197 <dc:source>Phys. Rev. Lett. 130, 081403 (2023)</dc:source>
198 <dc:type>article</dc:type>
199 <dc:identifier>doi:10.1103/PhysRevLett.130.081403</dc:identifier>
200 <prism:doi>10.1103/PhysRevLett.130.081403</prism:doi>
201 <prism:publicationName>Physical Review Letters</prism:publicationName>
202 <prism:volume>130</prism:volume>
203 <prism:number>8</prism:number>
204 <prism:publicationDate>2023-02-22T10:00:00+00:00</prism:publicationDate>
205 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.081403</prism:url>
206 <prism:startingPage>081403</prism:startingPage>
207 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
208 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
209 </item>
210 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.071002">
211 <title>Axion Dark Matter Search around $4.55\text{ }\text{ }\mathrm{μ}\mathrm{eV}$ with Dine-Fischler-Srednicki-Zhitnitskii Sensitivity</title>
212 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.071002</link>
213 <description>Author(s): Andrew K. Yi <em>et al.</em><br/><p>We report an axion dark matter search at Dine-Fischler-Srednicki-Zhitnitskii sensitivity with the CAPP-12TB haloscope, assuming axions contribute 100% of the local dark matter density. The search excluded the axion-photon coupling ${g}_{aγγ}$ down to about $6.2×{10}^{−16}\text{ }\text{ }{\mathrm{GeV…</p><br/>[Phys. Rev. Lett. 130, 071002] Published Thu Feb 16, 2023</description>
214 <content:encoded><![CDATA[<p>Author(s): Andrew K. Yi <em>et al.</em></p><p>We report an axion dark matter search at Dine-Fischler-Srednicki-Zhitnitskii sensitivity with the CAPP-12TB haloscope, assuming axions contribute 100% of the local dark matter density. The search excluded the axion-photon coupling <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>g</mi><mrow><mi>a</mi><mi>γ</mi><mi>γ</mi></mrow></msub></math> down to about <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mn>6.2</mn><mo>×</mo><msup><mn>10</mn><mrow><mo>−</mo><mn>16</mn></mrow></msup><mtext> </mtext><mtext> </mtext><mrow><msup><mrow><mi>GeV</mi></mrow><mrow><mo>−</mo><mn>1</mn></mrow></msup></mrow></math> over the axion mass range between…</p><br/><p>[Phys. Rev. Lett. 130, 071002] Published Thu Feb 16, 2023</p>]]></content:encoded>
215 <dc:title>Axion Dark Matter Search around $4.55\text{ }\text{ }\mathrm{μ}\mathrm{eV}$ with Dine-Fischler-Srednicki-Zhitnitskii Sensitivity</dc:title>
216 <dc:creator>Andrew K. Yi <em>et al.</em></dc:creator>
217 <dc:date>2023-02-16T10:00:00+00:00</dc:date>
218 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
219 <dc:source>Phys. Rev. Lett. 130, 071002 (2023)</dc:source>
220 <dc:type>article</dc:type>
221 <dc:identifier>doi:10.1103/PhysRevLett.130.071002</dc:identifier>
222 <prism:doi>10.1103/PhysRevLett.130.071002</prism:doi>
223 <prism:publicationName>Physical Review Letters</prism:publicationName>
224 <prism:volume>130</prism:volume>
225 <prism:number>7</prism:number>
226 <prism:publicationDate>2023-02-16T10:00:00+00:00</prism:publicationDate>
227 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.071002</prism:url>
228 <prism:startingPage>071002</prism:startingPage>
229 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
230 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
231 </item>
232 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.071001">
233 <title>Magnetic Dynamo Caused by Axions in Neutron Stars</title>
234 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.071001</link>
235 <description>Author(s): Filippo Anzuini, José A. Pons, Antonio Gómez-Bañón, Paul D. Lasky, Federico Bianchini, and Andrew Melatos<br/><p>The coupling between axions and photons modifies Maxwell’s equations, introducing a dynamo term in the magnetic induction equation. In neutron stars, for critical values of the axion decay constant and axion mass, the magnetic dynamo mechanism increases the total magnetic energy of the star. We show…</p><br/>[Phys. Rev. Lett. 130, 071001] Published Wed Feb 15, 2023</description>
236 <content:encoded><![CDATA[<p>Author(s): Filippo Anzuini, José A. Pons, Antonio Gómez-Bañón, Paul D. Lasky, Federico Bianchini, and Andrew Melatos</p><p>The coupling between axions and photons modifies Maxwell’s equations, introducing a dynamo term in the magnetic induction equation. In neutron stars, for critical values of the axion decay constant and axion mass, the magnetic dynamo mechanism increases the total magnetic energy of the star. We show…</p><br/><p>[Phys. Rev. Lett. 130, 071001] Published Wed Feb 15, 2023</p>]]></content:encoded>
237 <dc:title>Magnetic Dynamo Caused by Axions in Neutron Stars</dc:title>
238 <dc:creator>Filippo Anzuini, José A. Pons, Antonio Gómez-Bañón, Paul D. Lasky, Federico Bianchini, and Andrew Melatos</dc:creator>
239 <dc:date>2023-02-15T10:00:00+00:00</dc:date>
240 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
241 <dc:source>Phys. Rev. Lett. 130, 071001 (2023)</dc:source>
242 <dc:type>article</dc:type>
243 <dc:identifier>doi:10.1103/PhysRevLett.130.071001</dc:identifier>
244 <prism:doi>10.1103/PhysRevLett.130.071001</prism:doi>
245 <prism:publicationName>Physical Review Letters</prism:publicationName>
246 <prism:volume>130</prism:volume>
247 <prism:number>7</prism:number>
248 <prism:publicationDate>2023-02-15T10:00:00+00:00</prism:publicationDate>
249 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.071001</prism:url>
250 <prism:startingPage>071001</prism:startingPage>
251 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
252 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
253 </item>
254 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.061002">
255 <title>Search for Gamma-Ray Spectral Lines from Dark Matter Annihilation up to 100 TeV toward the Galactic Center with MAGIC</title>
256 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.061002</link>
257 <description>Author(s): H. Abe <em>et al.</em> (MAGIC Collaboration)<br/><p>Linelike features in TeV $γ$ rays constitute a “smoking gun” for TeV-scale particle dark matter and new physics. Probing the Galactic Center region with ground-based Cherenkov telescopes enables the search for TeV spectral features in immediate association with a dense dark matter reservoir at a sen…</p><br/>[Phys. Rev. Lett. 130, 061002] Published Fri Feb 10, 2023</description>
258 <content:encoded><![CDATA[<p>Author(s): H. Abe <em>et al.</em> (MAGIC Collaboration)</p><p>Linelike features in TeV <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>γ</mi></math> rays constitute a “smoking gun” for TeV-scale particle dark matter and new physics. Probing the Galactic Center region with ground-based Cherenkov telescopes enables the search for TeV spectral features in immediate association with a dense dark matter reservoir at a sensi…</p><br/><p>[Phys. Rev. Lett. 130, 061002] Published Fri Feb 10, 2023</p>]]></content:encoded>
259 <dc:title>Search for Gamma-Ray Spectral Lines from Dark Matter Annihilation up to 100 TeV toward the Galactic Center with MAGIC</dc:title>
260 <dc:creator>H. Abe <em>et al.</em> (MAGIC Collaboration)</dc:creator>
261 <dc:date>2023-02-10T10:00:00+00:00</dc:date>
262 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
263 <dc:source>Phys. Rev. Lett. 130, 061002 (2023)</dc:source>
264 <dc:type>article</dc:type>
265 <dc:identifier>doi:10.1103/PhysRevLett.130.061002</dc:identifier>
266 <prism:doi>10.1103/PhysRevLett.130.061002</prism:doi>
267 <prism:publicationName>Physical Review Letters</prism:publicationName>
268 <prism:volume>130</prism:volume>
269 <prism:number>6</prism:number>
270 <prism:publicationDate>2023-02-10T10:00:00+00:00</prism:publicationDate>
271 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.061002</prism:url>
272 <prism:startingPage>061002</prism:startingPage>
273 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
274 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
275 </item>
276 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.061001">
277 <title>Limits to Gauge Coupling in the Dark Sector Set by the Nonobservation of Instanton-Induced Decay of Super-Heavy Dark Matter in the Pierre Auger Observatory Data</title>
278 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.061001</link>
279 <description>Author(s): P. Abreu <em>et al.</em> (Pierre Auger Collaboration)<br/><p>Instantons, which are nonperturbative solutions to Yang-Mills equations, provide a signal for the occurrence of quantum tunneling between distinct classes of vacua. They can give rise to decays of particles otherwise forbidden. Using data collected at the Pierre Auger Observatory, we search for sign…</p><br/>[Phys. Rev. Lett. 130, 061001] Published Tue Feb 07, 2023</description>
280 <content:encoded><![CDATA[<p>Author(s): P. Abreu <em>et al.</em> (Pierre Auger Collaboration)</p><p>Instantons, which are nonperturbative solutions to Yang-Mills equations, provide a signal for the occurrence of quantum tunneling between distinct classes of vacua. They can give rise to decays of particles otherwise forbidden. Using data collected at the Pierre Auger Observatory, we search for sign…</p><br/><p>[Phys. Rev. Lett. 130, 061001] Published Tue Feb 07, 2023</p>]]></content:encoded>
281 <dc:title>Limits to Gauge Coupling in the Dark Sector Set by the Nonobservation of Instanton-Induced Decay of Super-Heavy Dark Matter in the Pierre Auger Observatory Data</dc:title>
282 <dc:creator>P. Abreu <em>et al.</em> (Pierre Auger Collaboration)</dc:creator>
283 <dc:date>2023-02-07T10:00:00+00:00</dc:date>
284 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
285 <dc:source>Phys. Rev. Lett. 130, 061001 (2023)</dc:source>
286 <dc:type>article</dc:type>
287 <dc:identifier>doi:10.1103/PhysRevLett.130.061001</dc:identifier>
288 <prism:doi>10.1103/PhysRevLett.130.061001</prism:doi>
289 <prism:publicationName>Physical Review Letters</prism:publicationName>
290 <prism:volume>130</prism:volume>
291 <prism:number>6</prism:number>
292 <prism:publicationDate>2023-02-07T10:00:00+00:00</prism:publicationDate>
293 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.061001</prism:url>
294 <prism:startingPage>061001</prism:startingPage>
295 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
296 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
297 </item>
298 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.061401">
299 <title>Exotic Compact Objects and the Fate of the Light-Ring Instability</title>
300 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.061401</link>
301 <description>Author(s): Pedro V. P. Cunha, Carlos Herdeiro, Eugen Radu, and Nicolas Sanchis-Gual<br/><p>The results of new simulations negate the argument that some objects thought to be black holes are instead hypothetical exotic systems called bosonic stars.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.061401.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 130, 061401] Published Tue Feb 07, 2023</description>
302 <content:encoded><![CDATA[<p>Author(s): Pedro V. P. Cunha, Carlos Herdeiro, Eugen Radu, and Nicolas Sanchis-Gual</p><p>The results of new simulations negate the argument that some objects thought to be black holes are instead hypothetical exotic systems called bosonic stars.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.130.061401.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 130, 061401] Published Tue Feb 07, 2023</p>]]></content:encoded>
303 <dc:title>Exotic Compact Objects and the Fate of the Light-Ring Instability</dc:title>
304 <dc:creator>Pedro V. P. Cunha, Carlos Herdeiro, Eugen Radu, and Nicolas Sanchis-Gual</dc:creator>
305 <dc:date>2023-02-07T10:00:00+00:00</dc:date>
306 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
307 <dc:source>Phys. Rev. Lett. 130, 061401 (2023)</dc:source>
308 <dc:type>article</dc:type>
309 <dc:identifier>doi:10.1103/PhysRevLett.130.061401</dc:identifier>
310 <prism:doi>10.1103/PhysRevLett.130.061401</prism:doi>
311 <prism:publicationName>Physical Review Letters</prism:publicationName>
312 <prism:volume>130</prism:volume>
313 <prism:number>6</prism:number>
314 <prism:publicationDate>2023-02-07T10:00:00+00:00</prism:publicationDate>
315 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.061401</prism:url>
316 <prism:startingPage>061401</prism:startingPage>
317 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
318 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
319 </item>
320 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.051201">
321 <title>Particle Motion under the Conservative Piece of the Self-Force is Hamiltonian</title>
322 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.051201</link>
323 <description>Author(s): Francisco M. Blanco and Éanna É. Flanagan<br/><p>We consider the motion of a point particle in a stationary spacetime under the influence of a scalar, electromagnetic, or gravitational self-force. We show that the conservative piece of the first-order self-force gives rise to Hamiltonian dynamics, and we derive an explicit expression for the Hamil…</p><br/>[Phys. Rev. Lett. 130, 051201] Published Wed Feb 01, 2023</description>
324 <content:encoded><![CDATA[<p>Author(s): Francisco M. Blanco and Éanna É. Flanagan</p><p>We consider the motion of a point particle in a stationary spacetime under the influence of a scalar, electromagnetic, or gravitational self-force. We show that the conservative piece of the first-order self-force gives rise to Hamiltonian dynamics, and we derive an explicit expression for the Hamil…</p><br/><p>[Phys. Rev. Lett. 130, 051201] Published Wed Feb 01, 2023</p>]]></content:encoded>
325 <dc:title>Particle Motion under the Conservative Piece of the Self-Force is Hamiltonian</dc:title>
326 <dc:creator>Francisco M. Blanco and Éanna É. Flanagan</dc:creator>
327 <dc:date>2023-02-01T10:00:00+00:00</dc:date>
328 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
329 <dc:source>Phys. Rev. Lett. 130, 051201 (2023)</dc:source>
330 <dc:type>article</dc:type>
331 <dc:identifier>doi:10.1103/PhysRevLett.130.051201</dc:identifier>
332 <prism:doi>10.1103/PhysRevLett.130.051201</prism:doi>
333 <prism:publicationName>Physical Review Letters</prism:publicationName>
334 <prism:volume>130</prism:volume>
335 <prism:number>5</prism:number>
336 <prism:publicationDate>2023-02-01T10:00:00+00:00</prism:publicationDate>
337 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.051201</prism:url>
338 <prism:startingPage>051201</prism:startingPage>
339 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
340 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
341 </item>
342 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.051001">
343 <title>Constraining First-Order Phase Transitions with Curvature Perturbations</title>
344 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.051001</link>
345 <description>Author(s): Jing Liu, Ligong Bian, Rong-Gen Cai, Zong-Kuan Guo, and Shao-Jiang Wang<br/><p>The randomness of the quantum tunneling process induces superhorizon curvature perturbations during cosmological first-order phase transitions. We for the first time utilize curvature perturbations to constrain the phase transition parameters, and find that the observations of the cosmic microwave b…</p><br/>[Phys. Rev. Lett. 130, 051001] Published Tue Jan 31, 2023</description>
346 <content:encoded><![CDATA[<p>Author(s): Jing Liu, Ligong Bian, Rong-Gen Cai, Zong-Kuan Guo, and Shao-Jiang Wang</p><p>The randomness of the quantum tunneling process induces superhorizon curvature perturbations during cosmological first-order phase transitions. We for the first time utilize curvature perturbations to constrain the phase transition parameters, and find that the observations of the cosmic microwave b…</p><br/><p>[Phys. Rev. Lett. 130, 051001] Published Tue Jan 31, 2023</p>]]></content:encoded>
347 <dc:title>Constraining First-Order Phase Transitions with Curvature Perturbations</dc:title>
348 <dc:creator>Jing Liu, Ligong Bian, Rong-Gen Cai, Zong-Kuan Guo, and Shao-Jiang Wang</dc:creator>
349 <dc:date>2023-01-31T10:00:00+00:00</dc:date>
350 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
351 <dc:source>Phys. Rev. Lett. 130, 051001 (2023)</dc:source>
352 <dc:type>article</dc:type>
353 <dc:identifier>doi:10.1103/PhysRevLett.130.051001</dc:identifier>
354 <prism:doi>10.1103/PhysRevLett.130.051001</prism:doi>
355 <prism:publicationName>Physical Review Letters</prism:publicationName>
356 <prism:volume>130</prism:volume>
357 <prism:number>5</prism:number>
358 <prism:publicationDate>2023-01-31T10:00:00+00:00</prism:publicationDate>
359 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.051001</prism:url>
360 <prism:startingPage>051001</prism:startingPage>
361 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
362 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
363 </item>
364 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.041001">
365 <title>Doppler Boosted Dust Emission and Cosmic Infrared Background–Galaxy Cross-Correlations: A New Probe of Cosmology and Astrophysics</title>
366 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.041001</link>
367 <description>Author(s): Abhishek S. Maniyar, Simone Ferraro, and Emmanuel Schaan<br/><p>We identify a new cosmological signal, the Doppler-boosted cosmic infrared background (DB CIB), arising from the peculiar motion of the galaxies whose thermal dust emission source the cosmic infrared background (CIB). This new observable is an independent probe of the cosmic velocity field, highly a…</p><br/>[Phys. Rev. Lett. 130, 041001] Published Tue Jan 24, 2023</description>
368 <content:encoded><![CDATA[<p>Author(s): Abhishek S. Maniyar, Simone Ferraro, and Emmanuel Schaan</p><p>We identify a new cosmological signal, the Doppler-boosted cosmic infrared background (DB CIB), arising from the peculiar motion of the galaxies whose thermal dust emission source the cosmic infrared background (CIB). This new observable is an independent probe of the cosmic velocity field, highly a…</p><br/><p>[Phys. Rev. Lett. 130, 041001] Published Tue Jan 24, 2023</p>]]></content:encoded>
369 <dc:title>Doppler Boosted Dust Emission and Cosmic Infrared Background–Galaxy Cross-Correlations: A New Probe of Cosmology and Astrophysics</dc:title>
370 <dc:creator>Abhishek S. Maniyar, Simone Ferraro, and Emmanuel Schaan</dc:creator>
371 <dc:date>2023-01-24T10:00:00+00:00</dc:date>
372 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
373 <dc:source>Phys. Rev. Lett. 130, 041001 (2023)</dc:source>
374 <dc:type>article</dc:type>
375 <dc:identifier>doi:10.1103/PhysRevLett.130.041001</dc:identifier>
376 <prism:doi>10.1103/PhysRevLett.130.041001</prism:doi>
377 <prism:publicationName>Physical Review Letters</prism:publicationName>
378 <prism:volume>130</prism:volume>
379 <prism:number>4</prism:number>
380 <prism:publicationDate>2023-01-24T10:00:00+00:00</prism:publicationDate>
381 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.041001</prism:url>
382 <prism:startingPage>041001</prism:startingPage>
383 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
384 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
385 </item>
386 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.021401">
387 <title>Coordinate Singularities of Self-Interacting Vector Field Theories</title>
388 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.021401</link>
389 <description>Author(s): Andrew Coates and Fethi M. Ramazanoğlu<br/><p>Self-interacting vectors are seeing a burst of interest where various groups demonstrated that the field evolution ends in finite time. Two nonequivalent criteria have been offered to identify this breakdown: (i) the vector constraint equation cannot be satisfied beyond a point where the breakdown o…</p><br/>[Phys. Rev. Lett. 130, 021401] Published Thu Jan 12, 2023</description>
390 <content:encoded><![CDATA[<p>Author(s): Andrew Coates and Fethi M. Ramazanoğlu</p><p>Self-interacting vectors are seeing a burst of interest where various groups demonstrated that the field evolution ends in finite time. Two nonequivalent criteria have been offered to identify this breakdown: (i) the vector constraint equation cannot be satisfied beyond a point where the breakdown o…</p><br/><p>[Phys. Rev. Lett. 130, 021401] Published Thu Jan 12, 2023</p>]]></content:encoded>
391 <dc:title>Coordinate Singularities of Self-Interacting Vector Field Theories</dc:title>
392 <dc:creator>Andrew Coates and Fethi M. Ramazanoğlu</dc:creator>
393 <dc:date>2023-01-12T10:00:00+00:00</dc:date>
394 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
395 <dc:source>Phys. Rev. Lett. 130, 021401 (2023)</dc:source>
396 <dc:type>article</dc:type>
397 <dc:identifier>doi:10.1103/PhysRevLett.130.021401</dc:identifier>
398 <prism:doi>10.1103/PhysRevLett.130.021401</prism:doi>
399 <prism:publicationName>Physical Review Letters</prism:publicationName>
400 <prism:volume>130</prism:volume>
401 <prism:number>2</prism:number>
402 <prism:publicationDate>2023-01-12T10:00:00+00:00</prism:publicationDate>
403 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.021401</prism:url>
404 <prism:startingPage>021401</prism:startingPage>
405 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
406 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
407 </item>
408 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.021001">
409 <title>Novel Ringdown Amplitude-Phase Consistency Test</title>
410 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.021001</link>
411 <description>Author(s): Xisco Jiménez Forteza, Swetha Bhagwat, Sumit Kumar, and Paolo Pani<br/><p>The ringdown signal emitted during a binary black hole coalescence can be modeled as a linear superposition of the characteristic damped modes of the remnant black hole that get excited during the merger phase. While checking the consistency of the measured frequencies and damping times against the …</p><br/>[Phys. Rev. Lett. 130, 021001] Published Wed Jan 11, 2023</description>
412 <content:encoded><![CDATA[<p>Author(s): Xisco Jiménez Forteza, Swetha Bhagwat, Sumit Kumar, and Paolo Pani</p><p>The ringdown signal emitted during a binary black hole coalescence can be modeled as a linear superposition of the characteristic damped modes of the remnant black hole that get excited during the merger phase. While checking the consistency of the measured frequencies and damping times against the …</p><br/><p>[Phys. Rev. Lett. 130, 021001] Published Wed Jan 11, 2023</p>]]></content:encoded>
413 <dc:title>Novel Ringdown Amplitude-Phase Consistency Test</dc:title>
414 <dc:creator>Xisco Jiménez Forteza, Swetha Bhagwat, Sumit Kumar, and Paolo Pani</dc:creator>
415 <dc:date>2023-01-11T10:00:00+00:00</dc:date>
416 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
417 <dc:source>Phys. Rev. Lett. 130, 021001 (2023)</dc:source>
418 <dc:type>article</dc:type>
419 <dc:identifier>doi:10.1103/PhysRevLett.130.021001</dc:identifier>
420 <prism:doi>10.1103/PhysRevLett.130.021001</prism:doi>
421 <prism:publicationName>Physical Review Letters</prism:publicationName>
422 <prism:volume>130</prism:volume>
423 <prism:number>2</prism:number>
424 <prism:publicationDate>2023-01-11T10:00:00+00:00</prism:publicationDate>
425 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.021001</prism:url>
426 <prism:startingPage>021001</prism:startingPage>
427 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
428 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
429 </item>
430 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.011402">
431 <title>Dynamical Instability of Self-Gravitating Membranes</title>
432 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.011402</link>
433 <description>Author(s): Huan Yang, Béatrice Bonga, and Zhen Pan<br/><p>We show that a generic relativistic membrane with in-plane pressure and surface density having the same sign is unstable with respect to a series of warping mode instabilities with high wave numbers. We also examine the criteria of instability for commonly studied exotic compact objects with membran…</p><br/>[Phys. Rev. Lett. 130, 011402] Published Thu Jan 05, 2023</description>
434 <content:encoded><![CDATA[<p>Author(s): Huan Yang, Béatrice Bonga, and Zhen Pan</p><p>We show that a generic relativistic membrane with in-plane pressure and surface density having the same sign is unstable with respect to a series of warping mode instabilities with high wave numbers. We also examine the criteria of instability for commonly studied exotic compact objects with membran…</p><br/><p>[Phys. Rev. Lett. 130, 011402] Published Thu Jan 05, 2023</p>]]></content:encoded>
435 <dc:title>Dynamical Instability of Self-Gravitating Membranes</dc:title>
436 <dc:creator>Huan Yang, Béatrice Bonga, and Zhen Pan</dc:creator>
437 <dc:date>2023-01-05T10:00:00+00:00</dc:date>
438 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
439 <dc:source>Phys. Rev. Lett. 130, 011402 (2023)</dc:source>
440 <dc:type>article</dc:type>
441 <dc:identifier>doi:10.1103/PhysRevLett.130.011402</dc:identifier>
442 <prism:doi>10.1103/PhysRevLett.130.011402</prism:doi>
443 <prism:publicationName>Physical Review Letters</prism:publicationName>
444 <prism:volume>130</prism:volume>
445 <prism:number>1</prism:number>
446 <prism:publicationDate>2023-01-05T10:00:00+00:00</prism:publicationDate>
447 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.011402</prism:url>
448 <prism:startingPage>011402</prism:startingPage>
449 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
450 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
451 </item>
452 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.130.011401">
453 <title>Supertranslation-Invariant Formula for the Angular Momentum Flux in Gravitational Scattering</title>
454 <link>http://link.aps.org/doi/10.1103/PhysRevLett.130.011401</link>
455 <description>Author(s): Reza Javadinezhad and Massimo Porrati<br/><p>The angular momentum radiated in gravitational scattering can be changed by performing a supertranslation of the asymptotic metric, i.e., by adding radiation with infinite wavelength to the metric. This puzzling property can be avoided by adopting a supertranslation-invariant definition of the angul…</p><br/>[Phys. Rev. Lett. 130, 011401] Published Tue Jan 03, 2023</description>
456 <content:encoded><![CDATA[<p>Author(s): Reza Javadinezhad and Massimo Porrati</p><p>The angular momentum radiated in gravitational scattering can be changed by performing a supertranslation of the asymptotic metric, i.e., by adding radiation with infinite wavelength to the metric. This puzzling property can be avoided by adopting a supertranslation-invariant definition of the angul…</p><br/><p>[Phys. Rev. Lett. 130, 011401] Published Tue Jan 03, 2023</p>]]></content:encoded>
457 <dc:title>Supertranslation-Invariant Formula for the Angular Momentum Flux in Gravitational Scattering</dc:title>
458 <dc:creator>Reza Javadinezhad and Massimo Porrati</dc:creator>
459 <dc:date>2023-01-03T10:00:00+00:00</dc:date>
460 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
461 <dc:source>Phys. Rev. Lett. 130, 011401 (2023)</dc:source>
462 <dc:type>article</dc:type>
463 <dc:identifier>doi:10.1103/PhysRevLett.130.011401</dc:identifier>
464 <prism:doi>10.1103/PhysRevLett.130.011401</prism:doi>
465 <prism:publicationName>Physical Review Letters</prism:publicationName>
466 <prism:volume>130</prism:volume>
467 <prism:number>1</prism:number>
468 <prism:publicationDate>2023-01-03T10:00:00+00:00</prism:publicationDate>
469 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.130.011401</prism:url>
470 <prism:startingPage>011401</prism:startingPage>
471 <dc:subject>Cosmology, Astrophysics, and Gravitation</dc:subject>
472 <prism:section>Cosmology, Astrophysics, and Gravitation</prism:section>
473 </item>
474 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261104">
475 <title>Well-Posedness of the Four-Derivative Scalar-Tensor Theory of Gravity in Singularity Avoiding Coordinates</title>
476 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261104</link>
477 <description>Author(s): Llibert Aresté Saló, Katy Clough, and Pau Figueras<br/><p>We show that the most general scalar-tensor theory of gravity up to four derivatives in $3+1$ dimensions is well-posed in a modified version of the CCZ4 formulation of the Einstein equations in singularity-avoiding coordinates. We demonstrate the robustness of our new formulation in practice by stud…</p><br/>[Phys. Rev. Lett. 129, 261104] Published Fri Dec 23, 2022</description>
478 <content:encoded><![CDATA[<p>Author(s): Llibert Aresté Saló, Katy Clough, and Pau Figueras</p><p>We show that the most general scalar-tensor theory of gravity up to four derivatives in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>3</mn><mo>+</mo><mn>1</mn></mrow></math> dimensions is well-posed in a modified version of the CCZ4 formulation of the Einstein equations in singularity-avoiding coordinates. We demonstrate the robustness of our new formulation in practice by studyi…</p><br/><p>[Phys. Rev. Lett. 129, 261104] Published Fri Dec 23, 2022</p>]]></content:encoded>
479 <dc:title>Well-Posedness of the Four-Derivative Scalar-Tensor Theory of Gravity in Singularity Avoiding Coordinates</dc:title>
480 <dc:creator>Llibert Aresté Saló, Katy Clough, and Pau Figueras</dc:creator>
481 <dc:date>2022-12-23T10:00:00+00:00</dc:date>
482 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
483 <dc:source>Phys. Rev. Lett. 129, 261104 (2022)</dc:source>
484 <dc:type>article</dc:type>
485 <dc:identifier>doi:10.1103/PhysRevLett.129.261104</dc:identifier>
486 <prism:doi>10.1103/PhysRevLett.129.261104</prism:doi>
487 <prism:publicationName>Physical Review Letters</prism:publicationName>
488 <prism:volume>129</prism:volume>
489 <prism:number>26</prism:number>
490 <prism:publicationDate>2022-12-23T10:00:00+00:00</prism:publicationDate>
491 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261104</prism:url>
492 <prism:startingPage>261104</prism:startingPage>
493 <dc:subject>Gravitation and Astrophysics</dc:subject>
494 <prism:section>Gravitation and Astrophysics</prism:section>
495 </item>
496 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261303">
497 <title>Domain Walls Seeding the Electroweak Phase Transition</title>
498 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261303</link>
499 <description>Author(s): Simone Blasi and Alberto Mariotti<br/><p>Topological defects can act as local impurities that seed cosmological phase transitions. In this Letter, we study the case of domain walls and how they can affect the electroweak phase transition in the singlet-extended standard model with a ${Z}_{2}$-symmetric potential. When the transition occurs…</p><br/>[Phys. Rev. Lett. 129, 261303] Published Fri Dec 23, 2022</description>
500 <content:encoded><![CDATA[<p>Author(s): Simone Blasi and Alberto Mariotti</p><p>Topological defects can act as local impurities that seed cosmological phase transitions. In this Letter, we study the case of domain walls and how they can affect the electroweak phase transition in the singlet-extended standard model with a <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><msub><mi>Z</mi><mn>2</mn></msub></math>-symmetric potential. When the transition occurs in two…</p><br/><p>[Phys. Rev. Lett. 129, 261303] Published Fri Dec 23, 2022</p>]]></content:encoded>
501 <dc:title>Domain Walls Seeding the Electroweak Phase Transition</dc:title>
502 <dc:creator>Simone Blasi and Alberto Mariotti</dc:creator>
503 <dc:date>2022-12-23T10:00:00+00:00</dc:date>
504 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
505 <dc:source>Phys. Rev. Lett. 129, 261303 (2022)</dc:source>
506 <dc:type>article</dc:type>
507 <dc:identifier>doi:10.1103/PhysRevLett.129.261303</dc:identifier>
508 <prism:doi>10.1103/PhysRevLett.129.261303</prism:doi>
509 <prism:publicationName>Physical Review Letters</prism:publicationName>
510 <prism:volume>129</prism:volume>
511 <prism:number>26</prism:number>
512 <prism:publicationDate>2022-12-23T10:00:00+00:00</prism:publicationDate>
513 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261303</prism:url>
514 <prism:startingPage>261303</prism:startingPage>
515 <dc:subject>Gravitation and Astrophysics</dc:subject>
516 <prism:section>Gravitation and Astrophysics</prism:section>
517 </item>
518 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261301">
519 <title>Observing Nulling of Primordial Correlations via the 21-cm Signal</title>
520 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261301</link>
521 <description>Author(s): Shyam Balaji, H. V. Ragavendra, Shiv K. Sethi, Joseph Silk, and L. Sriramkumar<br/><p>The 21-cm line emitted by neutral hydrogen (HI) during the Dark Ages carries imprints of pristine primordial correlations. In models of inflation driven by a single, canonical scalar field, we show that a phase of ultra-slow-roll can lead to a <i>null</i> in <i>all</i> the primordial correlations at a specific wa…</p><br/>[Phys. Rev. Lett. 129, 261301] Published Thu Dec 22, 2022</description>
522 <content:encoded><![CDATA[<p>Author(s): Shyam Balaji, H. V. Ragavendra, Shiv K. Sethi, Joseph Silk, and L. Sriramkumar</p><p>The 21-cm line emitted by neutral hydrogen (HI) during the Dark Ages carries imprints of pristine primordial correlations. In models of inflation driven by a single, canonical scalar field, we show that a phase of ultra-slow-roll can lead to a <i>null</i> in <i>all</i> the primordial correlations at a specific wa…</p><br/><p>[Phys. Rev. Lett. 129, 261301] Published Thu Dec 22, 2022</p>]]></content:encoded>
523 <dc:title>Observing Nulling of Primordial Correlations via the 21-cm Signal</dc:title>
524 <dc:creator>Shyam Balaji, H. V. Ragavendra, Shiv K. Sethi, Joseph Silk, and L. Sriramkumar</dc:creator>
525 <dc:date>2022-12-22T10:00:00+00:00</dc:date>
526 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
527 <dc:source>Phys. Rev. Lett. 129, 261301 (2022)</dc:source>
528 <dc:type>article</dc:type>
529 <dc:identifier>doi:10.1103/PhysRevLett.129.261301</dc:identifier>
530 <prism:doi>10.1103/PhysRevLett.129.261301</prism:doi>
531 <prism:publicationName>Physical Review Letters</prism:publicationName>
532 <prism:volume>129</prism:volume>
533 <prism:number>26</prism:number>
534 <prism:publicationDate>2022-12-22T10:00:00+00:00</prism:publicationDate>
535 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261301</prism:url>
536 <prism:startingPage>261301</prism:startingPage>
537 <dc:subject>Gravitation and Astrophysics</dc:subject>
538 <prism:section>Gravitation and Astrophysics</prism:section>
539 </item>
540 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261302">
541 <title>Glueball Dark Matter Revisited</title>
542 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261302</link>
543 <description>Author(s): Pierluca Carenza, Roman Pasechnik, Gustavo Salinas, and Zhi-Wei Wang<br/><p>We revisit the possibility that dark matter is composed of stable scalar glueballs of a confining dark SU(3) gauge theory coupled only to gravity. The relic abundance of dark glueballs is studied for the first time in a thermal effective theory accounting for strong-coupling dynamics. An important i…</p><br/>[Phys. Rev. Lett. 129, 261302] Published Thu Dec 22, 2022</description>
544 <content:encoded><![CDATA[<p>Author(s): Pierluca Carenza, Roman Pasechnik, Gustavo Salinas, and Zhi-Wei Wang</p><p>We revisit the possibility that dark matter is composed of stable scalar glueballs of a confining dark SU(3) gauge theory coupled only to gravity. The relic abundance of dark glueballs is studied for the first time in a thermal effective theory accounting for strong-coupling dynamics. An important i…</p><br/><p>[Phys. Rev. Lett. 129, 261302] Published Thu Dec 22, 2022</p>]]></content:encoded>
545 <dc:title>Glueball Dark Matter Revisited</dc:title>
546 <dc:creator>Pierluca Carenza, Roman Pasechnik, Gustavo Salinas, and Zhi-Wei Wang</dc:creator>
547 <dc:date>2022-12-22T10:00:00+00:00</dc:date>
548 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
549 <dc:source>Phys. Rev. Lett. 129, 261302 (2022)</dc:source>
550 <dc:type>article</dc:type>
551 <dc:identifier>doi:10.1103/PhysRevLett.129.261302</dc:identifier>
552 <prism:doi>10.1103/PhysRevLett.129.261302</prism:doi>
553 <prism:publicationName>Physical Review Letters</prism:publicationName>
554 <prism:volume>129</prism:volume>
555 <prism:number>26</prism:number>
556 <prism:publicationDate>2022-12-22T10:00:00+00:00</prism:publicationDate>
557 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261302</prism:url>
558 <prism:startingPage>261302</prism:startingPage>
559 <dc:subject>Gravitation and Astrophysics</dc:subject>
560 <prism:section>Gravitation and Astrophysics</prism:section>
561 </item>
562 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261102">
563 <title>Quantum Fluxes at the Inner Horizon of a Spinning Black Hole</title>
564 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261102</link>
565 <description>Author(s): Noa Zilberman, Marc Casals, Amos Ori, and Adrian C. Ottewill<br/><p>Rotating or charged classical black holes in isolation possess a special surface in their interior, the <i>Cauchy horizon</i>, beyond which the evolution of spacetime (based on the equations of General Relativity) ceases to be deterministic. In this Letter, we study the effect of a quantum massless scalar …</p><br/>[Phys. Rev. Lett. 129, 261102] Published Wed Dec 21, 2022</description>
566 <content:encoded><![CDATA[<p>Author(s): Noa Zilberman, Marc Casals, Amos Ori, and Adrian C. Ottewill</p><p>Rotating or charged classical black holes in isolation possess a special surface in their interior, the <i>Cauchy horizon</i>, beyond which the evolution of spacetime (based on the equations of General Relativity) ceases to be deterministic. In this Letter, we study the effect of a quantum massless scalar …</p><br/><p>[Phys. Rev. Lett. 129, 261102] Published Wed Dec 21, 2022</p>]]></content:encoded>
567 <dc:title>Quantum Fluxes at the Inner Horizon of a Spinning Black Hole</dc:title>
568 <dc:creator>Noa Zilberman, Marc Casals, Amos Ori, and Adrian C. Ottewill</dc:creator>
569 <dc:date>2022-12-21T10:00:00+00:00</dc:date>
570 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
571 <dc:source>Phys. Rev. Lett. 129, 261102 (2022)</dc:source>
572 <dc:type>article</dc:type>
573 <dc:identifier>doi:10.1103/PhysRevLett.129.261102</dc:identifier>
574 <prism:doi>10.1103/PhysRevLett.129.261102</prism:doi>
575 <prism:publicationName>Physical Review Letters</prism:publicationName>
576 <prism:volume>129</prism:volume>
577 <prism:number>26</prism:number>
578 <prism:publicationDate>2022-12-21T10:00:00+00:00</prism:publicationDate>
579 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261102</prism:url>
580 <prism:startingPage>261102</prism:startingPage>
581 <dc:subject>Gravitation and Astrophysics</dc:subject>
582 <prism:section>Gravitation and Astrophysics</prism:section>
583 </item>
584 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261103">
585 <title>Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations</title>
586 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261103</link>
587 <description>Author(s): Zhen Cao <em>et al.</em> (LHAASO Collaboration)<br/><p>The first measurements from a newly built gamma-ray observatory have been analyzed for signs of the decay of heavy dark matter, putting a lower limit on the hypothetical particles’ lifetime.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.261103.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 129, 261103] Published Wed Dec 21, 2022</description>
588 <content:encoded><![CDATA[<p>Author(s): Zhen Cao <em>et al.</em> (LHAASO Collaboration)</p><p>The first measurements from a newly built gamma-ray observatory have been analyzed for signs of the decay of heavy dark matter, putting a lower limit on the hypothetical particles’ lifetime.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.261103.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 129, 261103] Published Wed Dec 21, 2022</p>]]></content:encoded>
589 <dc:title>Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations</dc:title>
590 <dc:creator>Zhen Cao <em>et al.</em> (LHAASO Collaboration)</dc:creator>
591 <dc:date>2022-12-21T10:00:00+00:00</dc:date>
592 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
593 <dc:source>Phys. Rev. Lett. 129, 261103 (2022)</dc:source>
594 <dc:type>article</dc:type>
595 <dc:identifier>doi:10.1103/PhysRevLett.129.261103</dc:identifier>
596 <prism:doi>10.1103/PhysRevLett.129.261103</prism:doi>
597 <prism:publicationName>Physical Review Letters</prism:publicationName>
598 <prism:volume>129</prism:volume>
599 <prism:number>26</prism:number>
600 <prism:publicationDate>2022-12-21T10:00:00+00:00</prism:publicationDate>
601 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261103</prism:url>
602 <prism:startingPage>261103</prism:startingPage>
603 <dc:subject>Gravitation and Astrophysics</dc:subject>
604 <prism:section>Gravitation and Astrophysics</prism:section>
605 </item>
606 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.261101">
607 <title>Time-Dependent and Quasisteady Features of Fast Neutrino-Flavor Conversion</title>
608 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.261101</link>
609 <description>Author(s): Hiroki Nagakura and Masamichi Zaizen<br/><p>Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs iin core-collapse supernovae and binary neutron star mergers, the lack of global simulations has been the greatest obstacle to study their astrophysical consequences. In this Letter, we present large-sc…</p><br/>[Phys. Rev. Lett. 129, 261101] Published Mon Dec 19, 2022</description>
610 <content:encoded><![CDATA[<p>Author(s): Hiroki Nagakura and Masamichi Zaizen</p><p>Despite the theoretical indication that fast neutrino-flavor conversion (FFC) ubiquitously occurs iin core-collapse supernovae and binary neutron star mergers, the lack of global simulations has been the greatest obstacle to study their astrophysical consequences. In this Letter, we present large-sc…</p><br/><p>[Phys. Rev. Lett. 129, 261101] Published Mon Dec 19, 2022</p>]]></content:encoded>
611 <dc:title>Time-Dependent and Quasisteady Features of Fast Neutrino-Flavor Conversion</dc:title>
612 <dc:creator>Hiroki Nagakura and Masamichi Zaizen</dc:creator>
613 <dc:date>2022-12-19T10:00:00+00:00</dc:date>
614 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
615 <dc:source>Phys. Rev. Lett. 129, 261101 (2022)</dc:source>
616 <dc:type>article</dc:type>
617 <dc:identifier>doi:10.1103/PhysRevLett.129.261101</dc:identifier>
618 <prism:doi>10.1103/PhysRevLett.129.261101</prism:doi>
619 <prism:publicationName>Physical Review Letters</prism:publicationName>
620 <prism:volume>129</prism:volume>
621 <prism:number>26</prism:number>
622 <prism:publicationDate>2022-12-19T10:00:00+00:00</prism:publicationDate>
623 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.261101</prism:url>
624 <prism:startingPage>261101</prism:startingPage>
625 <dc:subject>Gravitation and Astrophysics</dc:subject>
626 <prism:section>Gravitation and Astrophysics</prism:section>
627 </item>
628 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.251103">
629 <title>Cosmic-Ray Boron Flux Measured from $8.4\text{ }\text{ }\mathrm{GeV}/n$ to $3.8\text{ }\text{ }\mathrm{TeV}/n$ with the Calorimetric Electron Telescope on the International Space Station</title>
630 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.251103</link>
631 <description>Author(s): O. Adriani <em>et al.</em> (CALET Collaboration)<br/><p>We present the measurement of the energy dependence of the boron flux in cosmic rays and its ratio to the carbon flux in an energy interval from $8.4\text{ }\text{ }\mathrm{GeV}/n$ to $3.8\text{ }\text{ }\mathrm{TeV}/n$ based on the data collected by the Calorimetric Electron Telescope (CALET) durin…</p><br/>[Phys. Rev. Lett. 129, 251103] Published Fri Dec 16, 2022</description>
632 <content:encoded><![CDATA[<p>Author(s): O. Adriani <em>et al.</em> (CALET Collaboration)</p><p>We present the measurement of the energy dependence of the boron flux in cosmic rays and its ratio to the carbon flux in an energy interval from <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>8.4</mn><mtext> </mtext><mtext> </mtext><mi>GeV</mi><mo>/</mo><mi>n</mi></mrow></math> to <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mn>3.8</mn><mtext> </mtext><mtext> </mtext><mi>TeV</mi><mo>/</mo><mi>n</mi></mrow></math> based on the data collected by the Calorimetric Electron Telescope (CALET) during <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mo>∼</mo><mn>6.4</mn><mtext> </mtext><mtext> </mtext><mi>yr</mi></math> of operation on the International Space…</p><br/><p>[Phys. Rev. Lett. 129, 251103] Published Fri Dec 16, 2022</p>]]></content:encoded>
633 <dc:title>Cosmic-Ray Boron Flux Measured from $8.4\text{ }\text{ }\mathrm{GeV}/n$ to $3.8\text{ }\text{ }\mathrm{TeV}/n$ with the Calorimetric Electron Telescope on the International Space Station</dc:title>
634 <dc:creator>O. Adriani <em>et al.</em> (CALET Collaboration)</dc:creator>
635 <dc:date>2022-12-16T10:00:00+00:00</dc:date>
636 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
637 <dc:source>Phys. Rev. Lett. 129, 251103 (2022)</dc:source>
638 <dc:type>article</dc:type>
639 <dc:identifier>doi:10.1103/PhysRevLett.129.251103</dc:identifier>
640 <prism:doi>10.1103/PhysRevLett.129.251103</prism:doi>
641 <prism:publicationName>Physical Review Letters</prism:publicationName>
642 <prism:volume>129</prism:volume>
643 <prism:number>25</prism:number>
644 <prism:publicationDate>2022-12-16T10:00:00+00:00</prism:publicationDate>
645 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.251103</prism:url>
646 <prism:startingPage>251103</prism:startingPage>
647 <dc:subject>Gravitation and Astrophysics</dc:subject>
648 <prism:section>Gravitation and Astrophysics</prism:section>
649 </item>
650 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.251104">
651 <title>de Sitter Bubbles from Anti–de Sitter Fluctuations</title>
652 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.251104</link>
653 <description>Author(s): Anxo Biasi, Oleg Evnin, and Spyros Sypsas<br/><p>A theoretical model shows that de Sitter geometries may emerge locally in globally anti-de Sitter spacetimes via unstable fluctuations.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.251104.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 129, 251104] Published Fri Dec 16, 2022</description>
654 <content:encoded><![CDATA[<p>Author(s): Anxo Biasi, Oleg Evnin, and Spyros Sypsas</p><p>A theoretical model shows that de Sitter geometries may emerge locally in globally anti-de Sitter spacetimes via unstable fluctuations.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.251104.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 129, 251104] Published Fri Dec 16, 2022</p>]]></content:encoded>
655 <dc:title>de Sitter Bubbles from Anti–de Sitter Fluctuations</dc:title>
656 <dc:creator>Anxo Biasi, Oleg Evnin, and Spyros Sypsas</dc:creator>
657 <dc:date>2022-12-16T10:00:00+00:00</dc:date>
658 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
659 <dc:source>Phys. Rev. Lett. 129, 251104 (2022)</dc:source>
660 <dc:type>article</dc:type>
661 <dc:identifier>doi:10.1103/PhysRevLett.129.251104</dc:identifier>
662 <prism:doi>10.1103/PhysRevLett.129.251104</prism:doi>
663 <prism:publicationName>Physical Review Letters</prism:publicationName>
664 <prism:volume>129</prism:volume>
665 <prism:number>25</prism:number>
666 <prism:publicationDate>2022-12-16T10:00:00+00:00</prism:publicationDate>
667 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.251104</prism:url>
668 <prism:startingPage>251104</prism:startingPage>
669 <dc:subject>Gravitation and Astrophysics</dc:subject>
670 <prism:section>Gravitation and Astrophysics</prism:section>
671 </item>
672 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.251101">
673 <title>Optimal Transport Reconstruction of Baryon Acoustic Oscillations</title>
674 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.251101</link>
675 <description>Author(s): Farnik Nikakhtar, Ravi K. Sheth, Bruno Lévy, and Roya Mohayaee<br/><p>A weighted, semidiscrete, fast optimal transport (OT) algorithm for reconstructing the Lagrangian positions of protohalos from their evolved Eulerian positions is presented. The algorithm makes use of a mass estimate of the biased tracers and of the distribution of the remaining mass (the “dust”) bu…</p><br/>[Phys. Rev. Lett. 129, 251101] Published Wed Dec 14, 2022</description>
676 <content:encoded><![CDATA[<p>Author(s): Farnik Nikakhtar, Ravi K. Sheth, Bruno Lévy, and Roya Mohayaee</p><p>A weighted, semidiscrete, fast optimal transport (OT) algorithm for reconstructing the Lagrangian positions of protohalos from their evolved Eulerian positions is presented. The algorithm makes use of a mass estimate of the biased tracers and of the distribution of the remaining mass (the “dust”) bu…</p><br/><p>[Phys. Rev. Lett. 129, 251101] Published Wed Dec 14, 2022</p>]]></content:encoded>
677 <dc:title>Optimal Transport Reconstruction of Baryon Acoustic Oscillations</dc:title>
678 <dc:creator>Farnik Nikakhtar, Ravi K. Sheth, Bruno Lévy, and Roya Mohayaee</dc:creator>
679 <dc:date>2022-12-14T10:00:00+00:00</dc:date>
680 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
681 <dc:source>Phys. Rev. Lett. 129, 251101 (2022)</dc:source>
682 <dc:type>article</dc:type>
683 <dc:identifier>doi:10.1103/PhysRevLett.129.251101</dc:identifier>
684 <prism:doi>10.1103/PhysRevLett.129.251101</prism:doi>
685 <prism:publicationName>Physical Review Letters</prism:publicationName>
686 <prism:volume>129</prism:volume>
687 <prism:number>25</prism:number>
688 <prism:publicationDate>2022-12-14T10:00:00+00:00</prism:publicationDate>
689 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.251101</prism:url>
690 <prism:startingPage>251101</prism:startingPage>
691 <dc:subject>Gravitation and Astrophysics</dc:subject>
692 <prism:section>Gravitation and Astrophysics</prism:section>
693 </item>
694 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.251102">
695 <title>Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey</title>
696 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.251102</link>
697 <description>Author(s): Joshua W. Foster, Samuel J. Witte, Matthew Lawson, Tim Linden, Vishal Gajjar, Christoph Weniger, and Benjamin R. Safdi<br/><p>A neutron star’s ultrastrong magnetic field could create the conditions for uncloaking a promising dark matter candidate.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.251102.png" width="200" height=\"100\"><br/>[Phys. Rev. Lett. 129, 251102] Published Tue Dec 13, 2022</description>
698 <content:encoded><![CDATA[<p>Author(s): Joshua W. Foster, Samuel J. Witte, Matthew Lawson, Tim Linden, Vishal Gajjar, Christoph Weniger, and Benjamin R. Safdi</p><p>A neutron star’s ultrastrong magnetic field could create the conditions for uncloaking a promising dark matter candidate.</p><img src="//cdn.journals.aps.org/journals/PRL/key_images/10.1103/PhysRevLett.129.251102.png" width="200" height=\"100\"><br/><p>[Phys. Rev. Lett. 129, 251102] Published Tue Dec 13, 2022</p>]]></content:encoded>
699 <dc:title>Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey</dc:title>
700 <dc:creator>Joshua W. Foster, Samuel J. Witte, Matthew Lawson, Tim Linden, Vishal Gajjar, Christoph Weniger, and Benjamin R. Safdi</dc:creator>
701 <dc:date>2022-12-13T10:00:00+00:00</dc:date>
702 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
703 <dc:source>Phys. Rev. Lett. 129, 251102 (2022)</dc:source>
704 <dc:type>article</dc:type>
705 <dc:identifier>doi:10.1103/PhysRevLett.129.251102</dc:identifier>
706 <prism:doi>10.1103/PhysRevLett.129.251102</prism:doi>
707 <prism:publicationName>Physical Review Letters</prism:publicationName>
708 <prism:volume>129</prism:volume>
709 <prism:number>25</prism:number>
710 <prism:publicationDate>2022-12-13T10:00:00+00:00</prism:publicationDate>
711 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.251102</prism:url>
712 <prism:startingPage>251102</prism:startingPage>
713 <dc:subject>Gravitation and Astrophysics</dc:subject>
714 <prism:section>Gravitation and Astrophysics</prism:section>
715 </item>
716 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.241102">
717 <title>Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way</title>
718 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.241102</link>
719 <description>Author(s): Akash Biswas, Bidya Binay Karak, and Robert Cameron<br/><p>A striking feature of the solar cycle is that at the beginning, sunspots appear around midlatitudes, and over time the latitudes of emergences migrate toward the equator. The maximum level of activity (e.g., sunspot number) varies from cycle to cycle. For strong cycles, the activity begins early and…</p><br/>[Phys. Rev. Lett. 129, 241102] Published Wed Dec 07, 2022</description>
720 <content:encoded><![CDATA[<p>Author(s): Akash Biswas, Bidya Binay Karak, and Robert Cameron</p><p>A striking feature of the solar cycle is that at the beginning, sunspots appear around midlatitudes, and over time the latitudes of emergences migrate toward the equator. The maximum level of activity (e.g., sunspot number) varies from cycle to cycle. For strong cycles, the activity begins early and…</p><br/><p>[Phys. Rev. Lett. 129, 241102] Published Wed Dec 07, 2022</p>]]></content:encoded>
721 <dc:title>Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way</dc:title>
722 <dc:creator>Akash Biswas, Bidya Binay Karak, and Robert Cameron</dc:creator>
723 <dc:date>2022-12-07T10:00:00+00:00</dc:date>
724 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
725 <dc:source>Phys. Rev. Lett. 129, 241102 (2022)</dc:source>
726 <dc:type>article</dc:type>
727 <dc:identifier>doi:10.1103/PhysRevLett.129.241102</dc:identifier>
728 <prism:doi>10.1103/PhysRevLett.129.241102</prism:doi>
729 <prism:publicationName>Physical Review Letters</prism:publicationName>
730 <prism:volume>129</prism:volume>
731 <prism:number>24</prism:number>
732 <prism:publicationDate>2022-12-07T10:00:00+00:00</prism:publicationDate>
733 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.241102</prism:url>
734 <prism:startingPage>241102</prism:startingPage>
735 <dc:subject>Gravitation and Astrophysics</dc:subject>
736 <prism:section>Gravitation and Astrophysics</prism:section>
737 </item>
738 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.241103">
739 <title>Gravitational Waves from Extreme-Mass-Ratio Systems in Astrophysical Environments</title>
740 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.241103</link>
741 <description>Author(s): Vitor Cardoso, Kyriakos Destounis, Francisco Duque, Rodrigo Panosso Macedo, and Andrea Maselli<br/><p>We establish a generic, fully relativistic formalism to study gravitational-wave emission by extreme-mass-ratio systems in spherically symmetric, nonvacuum black hole spacetimes. The potential applications to astrophysical setups range from black holes accreting baryonic matter to those within axion…</p><br/>[Phys. Rev. Lett. 129, 241103] Published Wed Dec 07, 2022</description>
742 <content:encoded><![CDATA[<p>Author(s): Vitor Cardoso, Kyriakos Destounis, Francisco Duque, Rodrigo Panosso Macedo, and Andrea Maselli</p><p>We establish a generic, fully relativistic formalism to study gravitational-wave emission by extreme-mass-ratio systems in spherically symmetric, nonvacuum black hole spacetimes. The potential applications to astrophysical setups range from black holes accreting baryonic matter to those within axion…</p><br/><p>[Phys. Rev. Lett. 129, 241103] Published Wed Dec 07, 2022</p>]]></content:encoded>
743 <dc:title>Gravitational Waves from Extreme-Mass-Ratio Systems in Astrophysical Environments</dc:title>
744 <dc:creator>Vitor Cardoso, Kyriakos Destounis, Francisco Duque, Rodrigo Panosso Macedo, and Andrea Maselli</dc:creator>
745 <dc:date>2022-12-07T10:00:00+00:00</dc:date>
746 <dc:rights>Personal use only, all commercial or other reuse prohibited</dc:rights>
747 <dc:source>Phys. Rev. Lett. 129, 241103 (2022)</dc:source>
748 <dc:type>article</dc:type>
749 <dc:identifier>doi:10.1103/PhysRevLett.129.241103</dc:identifier>
750 <prism:doi>10.1103/PhysRevLett.129.241103</prism:doi>
751 <prism:publicationName>Physical Review Letters</prism:publicationName>
752 <prism:volume>129</prism:volume>
753 <prism:number>24</prism:number>
754 <prism:publicationDate>2022-12-07T10:00:00+00:00</prism:publicationDate>
755 <prism:url>http://link.aps.org/doi/10.1103/PhysRevLett.129.241103</prism:url>
756 <prism:startingPage>241103</prism:startingPage>
757 <dc:subject>Gravitation and Astrophysics</dc:subject>
758 <prism:section>Gravitation and Astrophysics</prism:section>
759 </item>
760 <item rdf:about="http://link.aps.org/doi/10.1103/PhysRevLett.129.241301">
761 <title>Search for Ultralight Dark Matter from Long-Term Frequency Comparisons of Optical and Microwave Atomic Clocks</title>
762 <link>http://link.aps.org/doi/10.1103/PhysRevLett.129.241301</link>
763 <description>Author(s): Takumi Kobayashi, Akifumi Takamizawa, Daisuke Akamatsu, Akio Kawasaki, Akiko Nishiyama, Kazumoto Hosaka, Yusuke Hisai, Masato Wada, Hajime Inaba, Takehiko Tanabe, and Masami Yasuda<br/><p>We search for ultralight scalar dark matter candidates that induce oscillations of the fine structure constant, the electron and quark masses, and the quantum chromodynamics energy scale with frequency comparison data between a $^{171}\mathrm{Yb}$ optical lattice clock and a $^{133}\mathrm{Cs}$ foun…</p><br/>[Phys. Rev. Lett. 129, 241301] Published Wed Dec 07, 2022</description>
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