A. Brodzeller et al. (DESI Collaboration)
Phys. Rev. D 112, 083510 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
K. Lodha et al. (DESI Collaboration)
Phys. Rev. D 112, 083511 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
U. Andrade et al. (DESI Collaboration)
Phys. Rev. D 112, 083512 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
W. Elbers et al. (DESI Collaboration)
Phys. Rev. D 112, 083513 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
M. Abdul Karim et al. (DESI Collaboration)
Phys. Rev. D 112, 083514 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
M. Abdul Karim et al. (DESI Collaboration)
Phys. Rev. D 112, 083515 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
Tomasz Baka, Harsh Narola, Justin Janquart, Anuradha Samajdar, Tim Dietrich, and Chris Van Den Broeck
Phys. Rev. D 112, 082001 (2025) - Published 3 October, 2025
The problem of overlapping signals in gravitational wave astronomy refers to situations where signals from distinct events overlap in time. They pose a challenge for distinguishing the sources of the signals and accurately performing parameter estimation. This paper proposes an approach to addressing this issue for next-generation gravitational wave detectors.
Pranjal Ralegankar, Daniele Perri, and Takeshi Kobayashi
Phys. Rev. D 112, 083019 (2025) - Published 9 October, 2025
Cosmic history between inflation and Big Bang nucleosynthesis remains largely unconstrained. The authors explore a novel scenario in which self-interacting particles driving early matter domination can form halos that undergo gravothermal collapse, leading to primordial black holes in the asteroid-mass range or exotic compact objects such as cannibal stars and boson stars. This unveils a new pathway for early universe structure formation with distinctive observable implications.
N. A. Moraga, F. Castillo, D. D. Ofengeim, A. Reisenegger, J. A. Valdivia, M. E. Gusakov, E. M. Kantor, and A. Y. Potekhin
Phys. Rev. D 112, 083022 (2025) - Published 10 October, 2025
Magnetars are neutron stars with extremely strong magnetic fields; typically they are about 1000x stronger than the “garden variety” radio pulsars. They are also extremely hot and bright and it is generally thought that this extra luminosity is powered by the decay of their strong magnetic fields. The authors study this decay with a detailed numerical model of both the magnetic field decay and its thermal evolution. They show that unless the spatially large-scale magnetic field is extremely strong, the effect of magnetic field decay cannot explain the large luminosities observed from magnetars.
Keisuke Inomata, Marc Kamionkowski, Kentaro Kasai, and Bibhushan Shakya
Phys. Rev. D 112, 083523 (2025) - Published 14 October, 2025
In this paper, the authors discuss a new source of gravitational waves from first order phase transitions. The collision of bubbles in the new phase can efficiently produce particles that couple to the background field undergoing the transition, transferring a significant amount of the released vacuum energy into particle populations that long outlive the bubbles and provide a novel source of gravitational waves.
David Camarena, Kylar Greene, John Houghteling, and Francis-Yan Cyr-Racine
Phys. Rev. D 112, 083526 (2025) - Published 14 October, 2025
The authors use the latest Baryon Acoustic Oscillation (BAO)- and supernova-based distance data to extend ΛCDM, demonstrating that local cosmological overdensities can provide an alternative explanation to evolving Dark Energy’s “phantom crossing”.
Ian Holst, Gordan Krnjaic, and Huangyu Xiao
Phys. Rev. D 112, 083527 (2025) - Published 14 October, 2025
Light Primordial Black Holes (PBH) can dominate the universe before the onset of the radiation epoch and may evaporate prior to Big Bang Nucleosynthesis (BBN). The authors show that if this PBH-dominated phase lasts sufficiently long, PBHs can form dense clusters whose mergers exhibit runaway behavior, producing massive black holes that survive beyond BBN. Such relics can significantly alter the PBH mass distribution and yield distinctive observational signatures, thereby constraining regions of parameter space that were previously considered viable.
Dogan Akpinar, Vittorio del Duca, and Riccardo Gonzo
Phys. Rev. D 112, 084014 (2025) - Published 7 October, 2025
The gravitational self-force approach to the two-body problem is experiencing rapid development. This paper reports on incorporating spin into the effective field theory approach to gravitational self-force.
Tristan Pitre and Eric Poisson
Phys. Rev. D 112, 084017 (2025) - Published 7 October, 2025
Tidal deformations of neutron stars in binary inspiral leave an imprint on gravitational-wave emissions. Dynamical tides – in which the timescales of the tidal field and the internal hydrodynamics of neutron stars are comparable – display rich nonlinear phenomena only recently uncovered in the framework of Newtonian gravity. In this paper, an intrinsically general relativistic approach is developed eschewing the modal description of Newtonian theory. The nonlinearities of dynamical tides now find an inherently relativistic expression.
Guangzhou Guo, Peng Wang, and Yu-Peng Zhang
Phys. Rev. D 112, 084023 (2025) - Published 9 October, 2025
Ultracompact objects have been recently found to be susceptible to a new nonlinear instability known as light-ring instability, triggered by stable light rings, thereby raising concerns about the viability of the compact objects as black hole alternatives. Here, the authors study a particular type of scalarized black holes, known to admit stable light rings and through rigorous numerical simulation, demonstrate the long-term stability of these objects, thereby showing that a stable light ring need not necessarily imply light-ring instability.
Kai-Peng Lu and H. Lü
Phys. Rev. D 112, 084030 (2025) - Published 14 October, 2025
Black holes aren’t just cold graves of gravity – they have temperature and entropy. Previous studies have emphasized black holes’ role as the most entropic objects in the universe, that the entropy of a region of space is bounded above by the area that encloses it. This work instead suggests a thermodynamic constraint, that black hole entropy is bounded above by their specific heat. The bound is rigorously proven for some symmetric, static cases and checked on spinning and charged ones. The conjecture turns a stability diagnostic – specific heat – into a universal ceiling on disorder, hinting at new links between geometry and thermodynamics.
Dongjun Li, Colin Weller, Patrick Bourg, Michael LaHaye, Nicolás Yunes, and Huan Yang
Phys. Rev. D 112, 084057 (2025) - Published 22 October, 2025
Extreme-mass-ratio binaries are important sources of gravitational waves (GW) for space-based GW detectors such as LISA. Employing the newly developed modified Teukolsky formalism, the present paper develops a systematic method for computing scalar radiation from binary inspirals into supermassive black holes in a scalar cloud environment.
Qu Cao and Fan Zhu
Phys. Rev. D 112, 085012 (2025) - Published 16 October, 2025
Calculating higher-loop scattering amplitudes in pure Yang-Mills theory is a long-standing challenge. By using a novel geometric framework for scattering amplitudes, the authors develop a recursive method based on “cut equations” to compute all-loop integrands in pure Yang-Mills theory in the limit of large number of colors (planar limit). They explicitly provide the results for the two-loop five-point integrand.
Adriel I. Santoso and Le Bin Ho
Phys. Rev. D 112, L081301 (2025) - Published 1 October, 2025
Yang Xiao, Huai-Ke Guo, Jia-Hang Hu, Jin Min Yang, and Yang Zhang
Phys. Rev. D 112, L081302 (2025) - Published 6 October, 2025
Albert Escrivà and Chul-Moon Yoo
Phys. Rev. D 112, L081304 (2025) - Published 9 October, 2025
Biswanath Layek, Brijesh Kumar Saini, and Deepthi Godaba Venkata
Phys. Rev. D 112, L081305 (2025) - Published 8 October, 2025
Chen Yuan, Zu-Cheng Chen, and Lang Liu
Phys. Rev. D 112, L081306 (2025) - Published 14 October, 2025
Sebastian Zell
Phys. Rev. D 112, L081307 (2025) - Published 17 October, 2025
Ken Van Tilburg, Masha Baryakhtar, Marios Galanis, and Neal Weiner
Phys. Rev. D 112, L081308 (2025) - Published 27 October, 2025
Chengcheng Han, Hong-Jian He, Linghao Song, and Jingtao You
Phys. Rev. D 112, L081309 (2025) - Published 31 October, 2025
J. François and L. Ravera
Phys. Rev. D 112, L081501 (2025) - Published 6 October, 2025
P. George Christopher and S. Shankaranarayanan
Phys. Rev. D 112, L081502 (2025) - Published 22 October, 2025
Andre G. Campos, Karen Z. Hatsagortsyan, and Christoph H. Keitel
Phys. Rev. D 112, L081701 (2025) - Published 8 October, 2025
Rong-Xin Miao
Phys. Rev. D 112, L081901 (2025) - Published 2 October, 2025
Carlos Nunez and Dibakar Roychowdhury
Phys. Rev. D 112, L081902 (2025) - Published 3 October, 2025
Carlos Hoyos, Niko Jokela, and José Manuel Penín
Phys. Rev. D 112, L081903 (2025) - Published 10 October, 2025
Aditya Cowsik, Matteo Ippoliti, and Xiao-Liang Qi
Phys. Rev. D 112, L081904 (2025) - Published 23 October, 2025
Xi-Yang Ran, Feng Hao, and Hao Ouyang
Phys. Rev. D 112, L081905 (2025) - Published 23 October, 2025
Xin Jiang, Peng Wang, Houwen Wu, and Haitang Yang
Phys. Rev. D 112, L081906 (2025) - Published 29 October, 2025
Tomasz Baka, Harsh Narola, Justin Janquart, Anuradha Samajdar, Tim Dietrich, and Chris Van Den Broeck
Phys. Rev. D 112, 082001 (2025) - Published 3 October, 2025
The problem of overlapping signals in gravitational wave astronomy refers to situations where signals from distinct events overlap in time. They pose a challenge for distinguishing the sources of the signals and accurately performing parameter estimation. This paper proposes an approach to addressing this issue for next-generation gravitational wave detectors.
Yun-Jing Huang, Chad Hanna, Becca Ewing, Patrick Godwin, Joshua Gonsalves, Ryan Magee, Cody Messick, Leo Tsukada, Zach Yarbrough, Prathamesh Joshi, James Kennington, Wanting Niu, Jameson Rollins, and Urja Shah
Phys. Rev. D 112, 082002 (2025) - Published 6 October, 2025
Namisha Chabbra, Andrew Wade, Kirk McKenzie, Nicholas Demos, Slawomir Gras, and Matthew Evans
Phys. Rev. D 112, 082003 (2025) - Published 6 October, 2025
R. Abbasi et al. (IceCube Collaboration)
Phys. Rev. D 112, 082004 (2025) - Published 17 October, 2025
Alvise Pizzella, Miguel Dovale-Álvarez, Pablo Martínez Cano, Rodrigo García Álvarez, Christoph Bode, Juan José Esteban Delgado, and Gerhard Heinzel
Phys. Rev. D 112, 082005 (2025) - Published 28 October, 2025
Yi Shuen C. Lee, Marek J. Szczepańczyk, Tanmaya Mishra, Margaret Millhouse, and Andrew Melatos
Phys. Rev. D 112, 082006 (2025) - Published 30 October, 2025
Yen-Hsun Lin and Meng-Ru Wu
Phys. Rev. D 112, 083001 (2025) - Published 1 October, 2025
M. Pillas et al.
Phys. Rev. D 112, 083002 (2025) - Published 1 October, 2025
Vinh Tran, Xuejian Shen, Daniel Gilman, Mark Vogelsberger, Stephanie O’Neil, Donghua Xiong, Jiayi Hu, and Ziang Wu
Phys. Rev. D 112, 083003 (2025) - Published 2 October, 2025
Fangzhou Guo and Jibo He
Phys. Rev. D 112, 083004 (2025) - Published 2 October, 2025
Cameron Cook, Carlos Blanco, and Juri Smirnov
Phys. Rev. D 112, 083005 (2025) - Published 2 October, 2025
Alan Tsz-Lok Lam, Masaru Shibata, Kyohei Kawaguchi, and Joaquin Pelle
Phys. Rev. D 112, 083006 (2025) - Published 2 October, 2025
Enis Belgacem, Francesco Iacovelli, Michele Maggiore, Michele Mancarella, and Niccolò Muttoni
Phys. Rev. D 112, 083007 (2025) - Published 3 October, 2025
Damiano F. G. Fiorillo, Tetyana Pitik, and Edoardo Vitagliano
Phys. Rev. D 112, 083008 (2025) - Published 3 October, 2025
Shao-Peng Tang, Yong-Jia Huang, and Yi-Zhong Fan
Phys. Rev. D 112, 083009 (2025) - Published 3 October, 2025
João V. Zastrow, Jonas P. Pereira, Rafael C. R. de Lima, and Jorge E. Horvath
Phys. Rev. D 112, 083010 (2025) - Published 3 October, 2025
Daneng Yang, Yue-Lin Sming Tsai, and Yi-Zhong Fan
Phys. Rev. D 112, 083011 (2025) - Published 6 October, 2025
L. F. Araújo, G. Lugones, and J. A. S. Lima
Phys. Rev. D 112, 083012 (2025) - Published 6 October, 2025
Hwan Bae, Adrienne L. Erickcek, M. Sten Delos, and Julian B. Muñoz
Phys. Rev. D 112, 083013 (2025) - Published 6 October, 2025
R. A. Konoplya, Z. Stuchlík, and A. Zhidenko
Phys. Rev. D 112, 083014 (2025) - Published 6 October, 2025
Salvatore Vitale and Matthew Mould (Society of Physicists Interested in Non-aligned Spins, SPINS)
Phys. Rev. D 112, 083015 (2025) - Published 6 October, 2025
Zhen-Jie Wang, Ruo-Yu Liu, and Xiang-Yu Wang
Phys. Rev. D 112, 083016 (2025) - Published 7 October, 2025
Mattia Di Mauro, Adil Jueid, Jordan Koechler, and Roberto Ruiz de Austri
Phys. Rev. D 112, 083017 (2025) - Published 7 October, 2025
Hajime Sotani, Bernhard Müller, and Tomoya Takiwaki
Phys. Rev. D 112, 083018 (2025) - Published 8 October, 2025
Pranjal Ralegankar, Daniele Perri, and Takeshi Kobayashi
Phys. Rev. D 112, 083019 (2025) - Published 9 October, 2025
Cosmic history between inflation and Big Bang nucleosynthesis remains largely unconstrained. The authors explore a novel scenario in which self-interacting particles driving early matter domination can form halos that undergo gravothermal collapse, leading to primordial black holes in the asteroid-mass range or exotic compact objects such as cannibal stars and boson stars. This unveils a new pathway for early universe structure formation with distinctive observable implications.
Hibiki Iwanaga, Mahoro Matsuyama, and Yousuke Itoh
Phys. Rev. D 112, 083020 (2025) - Published 9 October, 2025
Malachy Bloom, Alexander W. Criswell, and Vuk Mandic
Phys. Rev. D 112, 083021 (2025) - Published 10 October, 2025
N. A. Moraga, F. Castillo, D. D. Ofengeim, A. Reisenegger, J. A. Valdivia, M. E. Gusakov, E. M. Kantor, and A. Y. Potekhin
Phys. Rev. D 112, 083022 (2025) - Published 10 October, 2025
Magnetars are neutron stars with extremely strong magnetic fields; typically they are about 1000x stronger than the “garden variety” radio pulsars. They are also extremely hot and bright and it is generally thought that this extra luminosity is powered by the decay of their strong magnetic fields. The authors study this decay with a detailed numerical model of both the magnetic field decay and its thermal evolution. They show that unless the spatially large-scale magnetic field is extremely strong, the effect of magnetic field decay cannot explain the large luminosities observed from magnetars.
Yi-Fan Wang (王一帆), Collin D. Capano, Jahed Abedi, Shilpa Kastha, Badri Krishnan, Alex B. Nielsen, Alexander H. Nitz, and Julian Westerweck
Phys. Rev. D 112, 083023 (2025) - Published 10 October, 2025
Zhenyu Zhang, Yehui Hou, Minyong Guo, Yosuke Mizuno, and Bin Chen
Phys. Rev. D 112, 083024 (2025) - Published 14 October, 2025
V. A. Allakhverdyan et al. (Baikal–GVD Collaboration)
Phys. Rev. D 112, 083025 (2025) - Published 14 October, 2025
Helena Ubach, Mark Gieles, and Jordi Miralda-Escudé
Phys. Rev. D 112, 083026 (2025) - Published 14 October, 2025
Lisa Johanna Schumacher, Mauricio Bustamante, Matteo Agostini, Foteini Oikonomou, and Elisa Resconi
Phys. Rev. D 112, 083027 (2025) - Published 15 October, 2025
Jam Sadiq, Thomas Dent, and Ana Lorenzo-Medina
Phys. Rev. D 112, 083028 (2025) - Published 14 October, 2025
Lorenz Zwick, Deniz Soyuer, Daniel J. D’Orazio, David O’Neill, Andrea Derdzinski, Prasenjit Saha, Diego Blas, Alexander C. Jenkins, and Luke Zoltan Kelley
Phys. Rev. D 112, 083029 (2025) - Published 14 October, 2025
Zhao Li and Wen Zhao
Phys. Rev. D 112, 083030 (2025) - Published 14 October, 2025
Bradley Shapiro
Phys. Rev. D 112, 083031 (2025) - Published 15 October, 2025
Xue-Zhi Liu, Premachand Mahapatra, Chun Huang, Ayush Hazarika, Chiranjeeb Singha, and Prasanta Kumar Das
Phys. Rev. D 112, 083032 (2025) - Published 15 October, 2025
Prabir Banik, Arunava Bhadra, and Sanjay K. Ghosh
Phys. Rev. D 112, 083033 (2025) - Published 16 October, 2025
Luis A. Anchordoqui, Francis Halzen, and Dieter Lüst
Phys. Rev. D 112, 083034 (2025) - Published 16 October, 2025
Aiden Gundersen and Neil J. Cornish
Phys. Rev. D 112, 083035 (2025) - Published 17 October, 2025
Minghui Du, Ziren Luo, and Peng Xu
Phys. Rev. D 112, 083036 (2025) - Published 17 October, 2025
Sergio Gimeno-Soler, Sayantani Lahiri, and Claus Lämmerzahl
Phys. Rev. D 112, 083037 (2025) - Published 17 October, 2025
Else Magnus, Jannes Loonen, Rose S. Stanley, Krijn D. de Vries, Nick van Eijndhoven, and Paul Coppin
Phys. Rev. D 112, 083038 (2025) - Published 17 October, 2025
Laura Barrio, Kotaro Fujisawa, Ryuichiro Akaho, Hiroki Nagakura, and Shoichi Yamada
Phys. Rev. D 112, 083039 (2025) - Published 17 October, 2025
Jeong Han Kim and Xing-Yu Yang
Phys. Rev. D 112, 083040 (2025) - Published 17 October, 2025
Bikai Gao, Yuk-Kei Kong, and Yong-Liang Ma
Phys. Rev. D 112, 083041 (2025) - Published 17 October, 2025
Clara E. Leitgeb, Robert D. Parsons, Andrew M. Taylor, Kenneth J. Ragan, David Berge, and Cigdem Issever
Phys. Rev. D 112, 083042 (2025) - Published 17 October, 2025
Johann Fernandes, Archana Pai, and Koustav Chandra
Phys. Rev. D 112, 083043 (2025) - Published 17 October, 2025
Valéria Carvalho, Márcio Ferreira, Michał Bejger, and Constança Providência
Phys. Rev. D 112, 083044 (2025) - Published 17 October, 2025
D. O. Chernyshov, A. V. Ivlev, and V. A. Dogiel
Phys. Rev. D 112, 083045 (2025) - Published 17 October, 2025
Pranaba K. Nayak, Rupraj Biswasharma, Pravata K. Mohanty, Shashi R. Dugad, V. Gopalkrishnan, Sunil K. Gupta, B. Hariharan, Y. Hayashi, P. Jagadeesan, Atul Jain, S. Kawakami, A. Oshima, Sunil D. Pawar, M. Rameez, and K. Ramesh (GRAPES-3 Collaboration)
Phys. Rev. D 112, 083046 (2025) - Published 21 October, 2025
Gargi Sen, Debaprasad Maity, and Santabrata Das
Phys. Rev. D 112, 083047 (2025) - Published 22 October, 2025
Arthur G. Suvorov, Petros Stefanou, and José A. Pons
Phys. Rev. D 112, 083048 (2025) - Published 22 October, 2025
Fahimeh Rahimi, Zeinab Rezaei, and Adamu Issifu
Phys. Rev. D 112, 083049 (2025) - Published 22 October, 2025
Valentin Thoss and Abraham Loeb
Phys. Rev. D 112, 083050 (2025) - Published 23 October, 2025
Claudio Salvadore, Iuri La Rosa, Paola Leaci, Francesco Amicucci, Pia Astone, Sabrina D’Antonio, Luca D’Onofrio, Cristiano Palomba, Lorenzo Pierini, and Francesco Safai Tehrani
Phys. Rev. D 112, 083051 (2025) - Published 23 October, 2025
Chingam Fong, Kenny C. Y. Ng, and Qishan Liu
Phys. Rev. D 112, 083052 (2025) - Published 23 October, 2025
R. Weizmann Kiendrebeogo, Muhammed Saleem, Marie Anne Bizouard, Andy H. Y. Chen, Nelson Christensen, Chia-Jui Chou, Michael W. Coughlin, Kamiel Janssens, S. Zacharie Kam, Jean Koulidiati, and Shu-Wei Yeh
Phys. Rev. D 112, 083053 (2025) - Published 23 October, 2025
S. L. Kranzhoff, S. L. Danilishin, S. Steinlechner, M. Vardaro, T. Zhang, and S. Hild
Phys. Rev. D 112, 083054 (2025) - Published 23 October, 2025
Dmitry D. Ofengeim and Tsvi Piran
Phys. Rev. D 112, 083055 (2025) - Published 27 October, 2025
D. Suárez-Fontanella, C. Albertus, and M. Ángeles Pérez-García
Phys. Rev. D 112, 083056 (2025) - Published 27 October, 2025
Marios Galanis, Ken Van Tilburg, Masha Baryakhtar, and Neal Weiner
Phys. Rev. D 112, 083057 (2025) - Published 27 October, 2025
Márcio Ferreira and Constança Providência
Phys. Rev. D 112, 083058 (2025) - Published 28 October, 2025
Ruben Lier, Akash Jain, Jay Armas, and Oliver Porth
Phys. Rev. D 112, 083059 (2025) - Published 28 October, 2025
Sarah Soares Sippert, Carlos Magno R. da Costa, Rogerio M. de Almeida, Rafael Alves Batista, and João R. T. de Mello Neto
Phys. Rev. D 112, 083060 (2025) - Published 29 October, 2025
Alexander S. Sakharov, Rostislav Konoplich, and Merab Gogberashvili
Phys. Rev. D 112, 083061 (2025) - Published 31 October, 2025
Farshad Kamalinejad and Zachary Slepian
Phys. Rev. D 112, 083501 (2025) - Published 1 October, 2025
Fumihiro Chuman and Masamune Oguri
Phys. Rev. D 112, 083502 (2025) - Published 1 October, 2025
Samuel Goldstein, Oliver H. E. Philcox, Emanuele Fondi, and William R. Coulton
Phys. Rev. D 112, 083503 (2025) - Published 1 October, 2025
Md. Wali Hossain and Afaq Maqsood
Phys. Rev. D 112, 083504 (2025) - Published 2 October, 2025
Leia Barrowes, Fred C. Adams, Anthony M. Bloch, and Scott Watson
Phys. Rev. D 112, 083505 (2025) - Published 3 October, 2025
Nanoom Lee, Matteo Braglia, and Yacine Ali-Haïmoud
Phys. Rev. D 112, 083506 (2025) - Published 6 October, 2025
Elena Massara, ChangHoon Hahn, Michael Eickenberg, Shirley Ho, Jiamin Hou, Pablo Lemos, Chirag Modi, Azadeh Moradinezhad Dizgah, Liam Parker, and Bruno Régaldo-Saint Blancard
Phys. Rev. D 112, 083507 (2025) - Published 6 October, 2025
Angelo Caravano, Gabriele Franciolini, and Sébastien Renaux-Petel
Phys. Rev. D 112, 083508 (2025) - Published 6 October, 2025
B. Hadzhiyska et al.
Phys. Rev. D 112, 083509 (2025) - Published 6 October, 2025
A. Brodzeller et al. (DESI Collaboration)
Phys. Rev. D 112, 083510 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
K. Lodha et al. (DESI Collaboration)
Phys. Rev. D 112, 083511 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
U. Andrade et al. (DESI Collaboration)
Phys. Rev. D 112, 083512 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
W. Elbers et al. (DESI Collaboration)
Phys. Rev. D 112, 083513 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
M. Abdul Karim et al. (DESI Collaboration)
Phys. Rev. D 112, 083514 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
M. Abdul Karim et al. (DESI Collaboration)
Phys. Rev. D 112, 083515 (2025) - Published 6 October, 2025
The new map of the Universe’s expansion history released by the DESI Collaboration offers hints at a breakdown of the standard model of cosmology.
Yuchen Zhang, Yang Liu, Hongwei Yu, and Puxun Wu
Phys. Rev. D 112, 083516 (2025) - Published 7 October, 2025
Kai Schmitz and Tobias Schröder
Phys. Rev. D 112, 083517 (2025) - Published 8 October, 2025
Albert Escrivà and Chul-Moon Yoo
Phys. Rev. D 112, 083518 (2025) - Published 9 October, 2025
Zhengyangguang Gong, Alexandre Barthelemy, and Sandrine Codis
Phys. Rev. D 112, 083519 (2025) - Published 9 October, 2025
Ashraf Shahriar, Mohammad Abbasiyan-Motlaq, Majid Mohsenzadeh, and Ebrahim Yusofi
Phys. Rev. D 112, 083520 (2025) - Published 10 October, 2025
James M. Sullivan, Carolina Cuesta-Lazaro, Mikhail M. Ivanov, Yueying Ni, Sownak Bose, Boryana Hadzhiyska, César Hernández-Aguayo, Lars Hernquist, and Rahul Kannan
Phys. Rev. D 112, 083521 (2025) - Published 10 October, 2025
James M. Sullivan and Uroš Seljak
Phys. Rev. D 112, 083522 (2025) - Published 14 October, 2025
Keisuke Inomata, Marc Kamionkowski, Kentaro Kasai, and Bibhushan Shakya
Phys. Rev. D 112, 083523 (2025) - Published 14 October, 2025
In this paper, the authors discuss a new source of gravitational waves from first order phase transitions. The collision of bubbles in the new phase can efficiently produce particles that couple to the background field undergoing the transition, transferring a significant amount of the released vacuum energy into particle populations that long outlive the bubbles and provide a novel source of gravitational waves.
Gopal Kashyap, Naveen K. Singh, and Pankaj Jain
Phys. Rev. D 112, 083524 (2025) - Published 14 October, 2025
Naonori Sugiyama
Phys. Rev. D 112, 083525 (2025) - Published 14 October, 2025
David Camarena, Kylar Greene, John Houghteling, and Francis-Yan Cyr-Racine
Phys. Rev. D 112, 083526 (2025) - Published 14 October, 2025
The authors use the latest Baryon Acoustic Oscillation (BAO)- and supernova-based distance data to extend ΛCDM, demonstrating that local cosmological overdensities can provide an alternative explanation to evolving Dark Energy’s “phantom crossing”.
Ian Holst, Gordan Krnjaic, and Huangyu Xiao
Phys. Rev. D 112, 083527 (2025) - Published 14 October, 2025
Light Primordial Black Holes (PBH) can dominate the universe before the onset of the radiation epoch and may evaporate prior to Big Bang Nucleosynthesis (BBN). The authors show that if this PBH-dominated phase lasts sufficiently long, PBHs can form dense clusters whose mergers exhibit runaway behavior, producing massive black holes that survive beyond BBN. Such relics can significantly alter the PBH mass distribution and yield distinctive observational signatures, thereby constraining regions of parameter space that were previously considered viable.
Jia-Le Ling, Guo-Hong Du, Tian-Nuo Li, Jing-Fei Zhang, Shao-Jiang Wang, and Xin Zhang
Phys. Rev. D 112, 083528 (2025) - Published 14 October, 2025
C. Garcia-Quintero et al. (DESI Collaboration)
Phys. Rev. D 112, 083529 (2025) - Published 15 October, 2025
Kai-Ge Zhang, Jian-Feng He, Chengjie Fu, and Zong-Kuan Guo
Phys. Rev. D 112, 083530 (2025) - Published 16 October, 2025
Claudia de Rham, Sadra Jazayeri, and Andrew J. Tolley
Phys. Rev. D 112, 083531 (2025) - Published 16 October, 2025
Özgür Akarsu, Bilal Bulduk, Antonio De Felice, Nihan Kat𝚤rc𝚤, and N. Merve Uzun
Phys. Rev. D 112, 083532 (2025) - Published 16 October, 2025
Rayff de Souza, Gabriel Rodrigues, and Jailson Alcaniz
Phys. Rev. D 112, 083533 (2025) - Published 17 October, 2025
Noah Sailer, Boryana Hadzhiyska, and Simone Ferraro
Phys. Rev. D 112, 083534 (2025) - Published 17 October, 2025
T. M. C. Abbott et al. (DES Collaboration)
Phys. Rev. D 112, 083535 (2025) - Published 17 October, 2025
Íñigo Zubeldia, Boris Bolliet, Anthony Challinor, and William Handley
Phys. Rev. D 112, 083536 (2025) - Published 17 October, 2025
Anton Chudaykin, Martin Kunz, and Julien Carron
Phys. Rev. D 112, 083537 (2025) - Published 17 October, 2025
Louis Legrand and Julien Carron
Phys. Rev. D 112, 083538 (2025) - Published 21 October, 2025
Wataru Chiba, Ryusuke Jinno, and Kimihiro Nomura
Phys. Rev. D 112, 083539 (2025) - Published 21 October, 2025
Shibsankar Si, Vivekanand Mohapatra, Pravin Kumar Natwariya, and Alekha C. Nayak
Phys. Rev. D 112, 083540 (2025) - Published 20 October, 2025
Lorenzo Gervani, Daniele Bertacca, and Nicola Bartolo
Phys. Rev. D 112, 083541 (2025) - Published 24 October, 2025
Vikramaditya Mondal and Shinji Mukohyama
Phys. Rev. D 112, 083542 (2025) - Published 22 October, 2025
Gabriel P. Lynch and Lloyd Knox
Phys. Rev. D 112, 083543 (2025) - Published 23 October, 2025
Philippe Brax
Phys. Rev. D 112, 083544 (2025) - Published 23 October, 2025
Adeela Afzal, Maria Mehmood, Mansoor Ur Rehman, and Qaisar Shafi
Phys. Rev. D 112, 083545 (2025) - Published 23 October, 2025
Keith R. Dienes, Lucien Heurtier, Fei Huang, Doojin Kim, Tim M. P. Tait, and Brooks Thomas
Phys. Rev. D 112, 083546 (2025) - Published 23 October, 2025
Keith R. Dienes, Lucien Heurtier, Fei Huang, Tim M. P. Tait, and Brooks Thomas
Phys. Rev. D 112, 083547 (2025) - Published 23 October, 2025
Philippe Brax and Patrick Valageas
Phys. Rev. D 112, 083548 (2025) - Published 23 October, 2025
Nobuchika Okada and Osamu Seto
Phys. Rev. D 112, 083549 (2025) - Published 23 October, 2025
Anastasiia M. Osipova and Sergey V. Pilipenko
Phys. Rev. D 112, 083550 (2025) - Published 24 October, 2025
Jiaming Pan, Meng-Xiang Lin, Gen Ye, Marco Raveri, and Alessandra Silvestri
Phys. Rev. D 112, 083551 (2025) - Published 27 October, 2025
Sarah Libanore, Julian B. Muñoz, and Ely D. Kovetz
Phys. Rev. D 112, 083552 (2025) - Published 27 October, 2025
Hao Wang and Yun-Song Piao
Phys. Rev. D 112, 083553 (2025) - Published 28 October, 2025
Margaret Johnston, Marios Kalomenopoulos, and Carl-Johan Haster
Phys. Rev. D 112, 083554 (2025) - Published 28 October, 2025
Jingtao You, Linghao Song, Hong-Jian He, and Chengcheng Han
Phys. Rev. D 112, 083555 (2025) - Published 31 October, 2025
Ryo Terasawa, Masahiro Takada, Toshiki Kurita, and Sunao Sugiyama
Phys. Rev. D 112, 083556 (2025) - Published 29 October, 2025
David Benisty
Phys. Rev. D 112, 083557 (2025) - Published 29 October, 2025
N. M. Jiménez Cruz, Ameek Malhotra, Gianmassimo Tasinato, and Ivonne Zavala
Phys. Rev. D 112, 083558 (2025) - Published 30 October, 2025
Tristan L. Smith and Nils Schöneberg
Phys. Rev. D 112, 083559 (2025) - Published 30 October, 2025
David Rønne Sallingboe and Sofie Marie Koksbang
Phys. Rev. D 112, 083560 (2025) - Published 30 October, 2025
R. Henry Liu et al.
Phys. Rev. D 112, 083561 (2025) - Published 31 October, 2025
Shu-Fan Chen and Mikhail M. Ivanov
Phys. Rev. D 112, 083562 (2025) - Published 31 October, 2025
Massimo Porrati and Xilin Sheng
Phys. Rev. D 112, 084001 (2025) - Published 1 October, 2025
H. V. Ovcharenko and O. B. Zaslavskii
Phys. Rev. D 112, 084002 (2025) - Published 2 October, 2025
Torben C. Frost
Phys. Rev. D 112, 084003 (2025) - Published 3 October, 2025
D. Fernando, Richard O’Shaughnessy, and Daniel Williams
Phys. Rev. D 112, 084004 (2025) - Published 3 October, 2025
Daniel Coumbe and Aria Rahmaty
Phys. Rev. D 112, 084005 (2025) - Published 6 October, 2025
Sophie Hourihane and Katerina Chatziioannou
Phys. Rev. D 112, 084006 (2025) - Published 6 October, 2025
Eugeny Babichev
Phys. Rev. D 112, 084007 (2025) - Published 6 October, 2025
Kenta Kiuchi
Phys. Rev. D 112, 084008 (2025) - Published 6 October, 2025
Guglielmo Faggioli, Maarten van de Meent, Alessandra Buonanno, and Gaurav Khanna
Phys. Rev. D 112, 084009 (2025) - Published 6 October, 2025
Hong Guo, Wei-Liang Qian, and Bean Wang
Phys. Rev. D 112, 084010 (2025) - Published 6 October, 2025
Fabiano Feleppa, Gaetano Lambiase, and Sunny Vagnozzi
Phys. Rev. D 112, 084011 (2025) - Published 6 October, 2025
Makana Silva, Harrison G. Blake-Goszyk, and Christopher M. Hirata
Phys. Rev. D 112, 084012 (2025) - Published 6 October, 2025
Georgios Antoniou, Thomas D. Pappas, and Panagiota Kanti
Phys. Rev. D 112, 084013 (2025) - Published 6 October, 2025
Dogan Akpinar, Vittorio del Duca, and Riccardo Gonzo
Phys. Rev. D 112, 084014 (2025) - Published 7 October, 2025
The gravitational self-force approach to the two-body problem is experiencing rapid development. This paper reports on incorporating spin into the effective field theory approach to gravitational self-force.
Gonzalo Morras
Phys. Rev. D 112, 084015 (2025) - Published 7 October, 2025
Mengfei Sun, Jie Wu, Jin Li, Brendan Mccane, Nan Yang, Xianghe Ma, Borui Wang, and Minghui Zhang
Phys. Rev. D 112, 084016 (2025) - Published 7 October, 2025
Tristan Pitre and Eric Poisson
Phys. Rev. D 112, 084017 (2025) - Published 7 October, 2025
Tidal deformations of neutron stars in binary inspiral leave an imprint on gravitational-wave emissions. Dynamical tides – in which the timescales of the tidal field and the internal hydrodynamics of neutron stars are comparable – display rich nonlinear phenomena only recently uncovered in the framework of Newtonian gravity. In this paper, an intrinsically general relativistic approach is developed eschewing the modal description of Newtonian theory. The nonlinearities of dynamical tides now find an inherently relativistic expression.
Nitesh K. Dubey and Sanved Kolekar
Phys. Rev. D 112, 084018 (2025) - Published 7 October, 2025
Hao Wang, Bin Liu, Yuan-Chuan Zou, and Qing-Wen Wu
Phys. Rev. D 112, 084019 (2025) - Published 8 October, 2025
Pietro Farina, Mariafelicia De Laurentis, Hideki Asada, Ivan De Martino, and Riccardo Della Monica
Phys. Rev. D 112, 084020 (2025) - Published 8 October, 2025
Maria Rosselló-Sastre, Sascha Husa, Sayantani Bera, and Yumeng Xu
Phys. Rev. D 112, 084021 (2025) - Published 8 October, 2025
Llibert Aresté Saló, Daniela D. Doneva, Katy Clough, Pau Figueras, and Stoytcho S. Yazadjiev
Phys. Rev. D 112, 084022 (2025) - Published 8 October, 2025
Guangzhou Guo, Peng Wang, and Yu-Peng Zhang
Phys. Rev. D 112, 084023 (2025) - Published 9 October, 2025
Ultracompact objects have been recently found to be susceptible to a new nonlinear instability known as light-ring instability, triggered by stable light rings, thereby raising concerns about the viability of the compact objects as black hole alternatives. Here, the authors study a particular type of scalarized black holes, known to admit stable light rings and through rigorous numerical simulation, demonstrate the long-term stability of these objects, thereby showing that a stable light ring need not necessarily imply light-ring instability.
Marcus Haberland, Alessandra Buonanno, and Jan Steinhoff
Phys. Rev. D 112, 084024 (2025) - Published 9 October, 2025
Ruijun Shi, Zun Wang, Xiaolin Liu, Tianyu Zhao, Zhixiang Ren, and Zhoujian Cao
Phys. Rev. D 112, 084025 (2025) - Published 9 October, 2025
Marcos R. A. Arcodía, Gaston Giribet, and Juan Laurnagaray
Phys. Rev. D 112, 084026 (2025) - Published 10 October, 2025
Utkarsh Kumar
Phys. Rev. D 112, 084027 (2025) - Published 10 October, 2025
Pedro G. S. Fernandes
Phys. Rev. D 112, 084028 (2025) - Published 10 October, 2025
Roberto D. Alba Q., Javier Chagoya, and Armando A. Roque
Phys. Rev. D 112, 084029 (2025) - Published 14 October, 2025
Kai-Peng Lu and H. Lü
Phys. Rev. D 112, 084030 (2025) - Published 14 October, 2025
Black holes aren’t just cold graves of gravity – they have temperature and entropy. Previous studies have emphasized black holes’ role as the most entropic objects in the universe, that the entropy of a region of space is bounded above by the area that encloses it. This work instead suggests a thermodynamic constraint, that black hole entropy is bounded above by their specific heat. The bound is rigorously proven for some symmetric, static cases and checked on spinning and charged ones. The conjecture turns a stability diagnostic – specific heat – into a universal ceiling on disorder, hinting at new links between geometry and thermodynamics.
Ana Alonso-Serrano, Marco de Cesare, and Manuel Del Piano
Phys. Rev. D 112, 084031 (2025) - Published 14 October, 2025
Sarp Akçay, Charlie Hoy, and Jake Mac Uilliam
Phys. Rev. D 112, 084032 (2025) - Published 14 October, 2025
Shengzhi Li and Yongge Ma
Phys. Rev. D 112, 084033 (2025) - Published 14 October, 2025
Avinash Tiwari, Aditya Vijaykumar, Shasvath J. Kapadia, Sourav Chatterjee, and Giacomo Fragione
Phys. Rev. D 112, 084034 (2025) - Published 14 October, 2025
Hideki Maeda and Cristián Martínez
Phys. Rev. D 112, 084035 (2025) - Published 15 October, 2025
Sebastiano Bernuzzi, Joan Fontbuté, Simone Albanesi, and An𝚤l Zenginoğlu
Phys. Rev. D 112, 084036 (2025) - Published 17 October, 2025
Shammi Tahura, David A. Nichols, and Kent Yagi
Phys. Rev. D 112, 084037 (2025) - Published 15 October, 2025
Mallika R. Sinha, Ling Sun, and Sizheng Ma
Phys. Rev. D 112, 084038 (2025) - Published 15 October, 2025
Qian Hu and John Veitch
Phys. Rev. D 112, 084039 (2025) - Published 15 October, 2025
Yu-Qi Chen and Hai-Shan Liu
Phys. Rev. D 112, 084040 (2025) - Published 15 October, 2025
W. Barker, G. K. Karananas, and H. Tu
Phys. Rev. D 112, 084041 (2025) - Published 15 October, 2025
Andrew Laeuger, Colin Weller, Dongjun Li, and Yanbei Chen
Phys. Rev. D 112, 084042 (2025) - Published 15 October, 2025
Soham Acharya, Shuvayu Roy, and Sudipta Sarkar
Phys. Rev. D 112, 084043 (2025) - Published 16 October, 2025
Terrence Pierre Jacques, Samuel Cupp, Leonardo R. Werneck, Samuel D. Tootle, Maria C. Babiuc Hamilton, and Zachariah B. Etienne
Phys. Rev. D 112, 084044 (2025) - Published 17 October, 2025
Renjie Wang, Yumeng Xu, Gang Wang, Bin Hu, and Rong-Gen Cai
Phys. Rev. D 112, 084045 (2025) - Published 17 October, 2025
Philip Beltracchi and Camilo Posada
Phys. Rev. D 112, 084046 (2025) - Published 17 October, 2025
Ludovico Machet and Llibert Aresté Saló
Phys. Rev. D 112, 084047 (2025) - Published 17 October, 2025
Lennox S. Keeble and Alejandro Cárdenas-Avendaño
Phys. Rev. D 112, 084048 (2025) - Published 17 October, 2025
Maxime De Sousa, Aurélien Barrau, and Killian Martineau
Phys. Rev. D 112, 084049 (2025) - Published 17 October, 2025
Alessandro Santini, Martina Muratore, Jonathan Gair, and Olaf Hartwig
Phys. Rev. D 112, 084050 (2025) - Published 17 October, 2025
Ioannis D. Gialamas and Kyriakos Tamvakis
Phys. Rev. D 112, 084051 (2025) - Published 17 October, 2025
Kyosuke Tomonari and Daniel Blixt
Phys. Rev. D 112, 084052 (2025) - Published 22 October, 2025
Ran Chen, Rohit S. Chandramouli, Federico Pozzoli, Riccardo Buscicchio, and Enrico Barausse
Phys. Rev. D 112, 084053 (2025) - Published 22 October, 2025
Giulia Huez, Sebastiano Bernuzzi, Matteo Breschi, and Rossella Gamba
Phys. Rev. D 112, 084054 (2025) - Published 22 October, 2025
Gökhan Alkaç, Murat Mesta, and Gönül Ünal
Phys. Rev. D 112, 084055 (2025) - Published 22 October, 2025
Benjamin Koch, Ali Riahinia, and Angel Rincon
Phys. Rev. D 112, 084056 (2025) - Published 22 October, 2025
Dongjun Li, Colin Weller, Patrick Bourg, Michael LaHaye, Nicolás Yunes, and Huan Yang
Phys. Rev. D 112, 084057 (2025) - Published 22 October, 2025
Extreme-mass-ratio binaries are important sources of gravitational waves (GW) for space-based GW detectors such as LISA. Employing the newly developed modified Teukolsky formalism, the present paper develops a systematic method for computing scalar radiation from binary inspirals into supermassive black holes in a scalar cloud environment.
Martín G. Richarte and Júnior D. Toniato
Phys. Rev. D 112, 084058 (2025) - Published 22 October, 2025
Gonzalo J. Olmo, João Luís Rosa, Diego Rubiera-Garcia, Alejandro Rueda, and Diego Sáez-Chillón Gómez
Phys. Rev. D 112, 084059 (2025) - Published 22 October, 2025
Robert Rosati and Tyson B. Littenberg
Phys. Rev. D 112, 084060 (2025) - Published 23 October, 2025
Hajime Kobayashi, Shinji Mukohyama, Naritaka Oshita, Kazufumi Takahashi, and Vicharit Yingcharoenrat
Phys. Rev. D 112, 084061 (2025) - Published 23 October, 2025
Leonardo de Lima and Davi C. Rodrigues
Phys. Rev. D 112, 084062 (2025) - Published 23 October, 2025
Yi Zhou and Rodrigo Panosso Macedo
Phys. Rev. D 112, 084063 (2025) - Published 23 October, 2025
Xiao-Xiao Kou, Muhammed Saleem, Vuk Mandic, Colm Talbot, and Eric Thrane
Phys. Rev. D 112, 084064 (2025) - Published 24 October, 2025
Rajendra Prasad Bhatt, Sumanta Chakraborty, and Sukanta Bose
Phys. Rev. D 112, 084065 (2025) - Published 24 October, 2025
Sousuke Noda and Masaaki Takahashi
Phys. Rev. D 112, 084066 (2025) - Published 24 October, 2025
L. Gavassino
Phys. Rev. D 112, 084067 (2025) - Published 24 October, 2025
Alex Kehagias and Antonio Riotto
Phys. Rev. D 112, 084068 (2025) - Published 28 October, 2025
Jenna Bruton, Peter Dunsby, and Álvaro de la Cruz-Dombriz
Phys. Rev. D 112, 084069 (2025) - Published 28 October, 2025
Ilya Peshkov, Héctor Olivares, and Evgeniy Romenski
Phys. Rev. D 112, 084070 (2025) - Published 27 October, 2025
Maïté Dupuis, Laurent Freidel, Florian Girelli, Abdulmajid Osumanu, and Julian Rennert
Phys. Rev. D 112, 084071 (2025) - Published 27 October, 2025
Suprovo Ghosh, José Luis Hernández, Bikram Keshari Pradhan, Cristina Manuel, Debarati Chatterjee, and Laura Tolos
Phys. Rev. D 112, 084072 (2025) - Published 28 October, 2025
João P. B. Brito, Atsushi Higuchi, and Luís C. B. Crispino
Phys. Rev. D 112, 084073 (2025) - Published 29 October, 2025
Yong Xiao, Qiang Wang, and Aonan Zhang
Phys. Rev. D 112, 084074 (2025) - Published 29 October, 2025
Xiaobo Zou, Xingyu Zhong, Wen-Biao Han, and Soumya D. Mohanty
Phys. Rev. D 112, 084075 (2025) - Published 29 October, 2025
Sebastian H. Völkel and Arnab Dhani
Phys. Rev. D 112, 084076 (2025) - Published 29 October, 2025
Gabriel Luz Almeida, Alan Müller, Stefano Foffa, and Riccardo Sturani
Phys. Rev. D 112, 084077 (2025) - Published 29 October, 2025
Samson H. W. Leong, Alejandro Florido Tomé, Juan Calderón Bustillo, Adrián del Río, and Nicolas Sanchis-Gual
Phys. Rev. D 112, 084078 (2025) - Published 29 October, 2025
Hanno Sahlmann and Cong Zhang
Phys. Rev. D 112, 084079 (2025) - Published 30 October, 2025
R. Abbott et al. (The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)
Phys. Rev. D 112, 084080 (2025) - Published 31 October, 2025
Adrian Lopez-Raven, Robert B. Mann, and Jorma Louko
Phys. Rev. D 112, 085001 (2025) - Published 6 October, 2025
Christoph Bartsch, Karol Kampf, Jiří Novotný, and Jaroslav Trnka
Phys. Rev. D 112, 085002 (2025) - Published 6 October, 2025
I. H. Kloß and Andre G. Campos
Phys. Rev. D 112, 085003 (2025) - Published 6 October, 2025
Lukas W. Lindwasser
Phys. Rev. D 112, 085004 (2025) - Published 6 October, 2025
Andre G. Campos, Karen Z. Hatsagortsyan, and Christoph H. Keitel
Phys. Rev. D 112, 085005 (2025) - Published 8 October, 2025
Sumanta Chakraborty, Anupam Mazumdar, and Ritapriya Pradhan
Phys. Rev. D 112, 085006 (2025) - Published 8 October, 2025
André Benevides and Atish Dabholkar
Phys. Rev. D 112, 085007 (2025) - Published 8 October, 2025
Bin Chen, Zezhou Hu, and Xin-Cheng Mao
Phys. Rev. D 112, 085008 (2025) - Published 9 October, 2025
M. S. Guimaraes, I. Roditi, and S. P. Sorella
Phys. Rev. D 112, 085009 (2025) - Published 14 October, 2025
Duncan MacIntyre and Gordon W. Semenoff
Phys. Rev. D 112, 085010 (2025) - Published 15 October, 2025
István Gábor Márián, Andrea Trombettoni, and István Nándori
Phys. Rev. D 112, 085011 (2025) - Published 15 October, 2025
Qu Cao and Fan Zhu
Phys. Rev. D 112, 085012 (2025) - Published 16 October, 2025
Calculating higher-loop scattering amplitudes in pure Yang-Mills theory is a long-standing challenge. By using a novel geometric framework for scattering amplitudes, the authors develop a recursive method based on “cut equations” to compute all-loop integrands in pure Yang-Mills theory in the limit of large number of colors (planar limit). They explicitly provide the results for the two-loop five-point integrand.
Christopher J. Shallue and Sean M. Carroll
Phys. Rev. D 112, 085013 (2025) - Published 16 October, 2025
Si-Wei Han, Wenjing Chen, Langxuan Chen, Zhichun Ouyang, and Jun Feng
Phys. Rev. D 112, 085014 (2025) - Published 17 October, 2025
Giordano Cintia, Federico Piazza, and Samuel Ramos
Phys. Rev. D 112, 085015 (2025) - Published 17 October, 2025
Morgan H. Lynch
Phys. Rev. D 112, 085016 (2025) - Published 17 October, 2025
J. Alfaro
Phys. Rev. D 112, 085017 (2025) - Published 21 October, 2025
Samim Akhtar, Yilber Fabian Bautista, Cristoforo Iossa, and Zihan Zhou
Phys. Rev. D 112, 085018 (2025) - Published 23 October, 2025
Kuan-Nan Lin and Pisin Chen
Phys. Rev. D 112, 085019 (2025) - Published 23 October, 2025
Anna Tokareva and Yongjun Xu
Phys. Rev. D 112, 085020 (2025) - Published 23 October, 2025
Alexey Litvinov, Pavel Meshcheriakov, and Egor Shestopalov
Phys. Rev. D 112, 085021 (2025) - Published 24 October, 2025
Sven Bjarke Gudnason and Muneto Nitta
Phys. Rev. D 112, 085022 (2025) - Published 24 October, 2025
Adrian del Rio, Javier Olmedo, and António Torres Manso
Phys. Rev. D 112, 085023 (2025) - Published 24 October, 2025
Kensuke Gallock-Yoshimura and Erickson Tjoa
Phys. Rev. D 112, 085024 (2025) - Published 27 October, 2025
Rupak Chatterjee
Phys. Rev. D 112, 085025 (2025) - Published 28 October, 2025
M. Bordag and D. N. Voskresensky
Phys. Rev. D 112, 085026 (2025) - Published 29 October, 2025
Bruno S. Felipe and João P. M. Pitelli
Phys. Rev. D 112, 085027 (2025) - Published 29 October, 2025
Álvaro Álvarez-Domínguez and Álvaro Parra-López
Phys. Rev. D 112, 085028 (2025) - Published 30 October, 2025
J. A. Gracey, A. Maier, P. Marquard, and Y. Schröder
Phys. Rev. D 112, 085029 (2025) - Published 30 October, 2025
Nada Eissa, Carlos R. Ordóñez, and Gustavo Valdivia-Mera
Phys. Rev. D 112, 085030 (2025) - Published 30 October, 2025
Joseph Bunao, Pietropaolo Frisoni, Athanasios Kogios, and Jared Wogan
Phys. Rev. D 112, 086001 (2025) - Published 2 October, 2025
Felipe Díaz-Jaramillo, Silvia Nagy, and Giorgio Pizzolo
Phys. Rev. D 112, 086002 (2025) - Published 7 October, 2025
Lucas Martin, Martin Parlanti, and Martin Schvellinger
Phys. Rev. D 112, 086003 (2025) - Published 8 October, 2025
Pavan Dharanipragada and B. Sathiapalan
Phys. Rev. D 112, 086004 (2025) - Published 8 October, 2025
Fei-Jie Huang, Qi-Hui Chen, Yong-Ping Fu, Qing-Yuan Chen, Yi-Fen Zhao, and Wei Guo
Phys. Rev. D 112, 086005 (2025) - Published 9 October, 2025
Alvaro Herráez, Dieter Lüst, and Carmine Montella
Phys. Rev. D 112, 086006 (2025) - Published 10 October, 2025
Pei Zheng, Yidian Chen, Danning Li, Mei Huang, and Yu-xin Liu
Phys. Rev. D 112, 086007 (2025) - Published 10 October, 2025
Yaser Tavakoli, Ahad Khaleghi Ardabili, and Sara Mosaddegh
Phys. Rev. D 112, 086008 (2025) - Published 14 October, 2025
Pabitra Tripathy and Amit Ghosh
Phys. Rev. D 112, 086009 (2025) - Published 14 October, 2025
Siddhi Swarupa Jena, Arpan Bhattacharjee, David Dudal, and Subhash Mahapatra
Phys. Rev. D 112, 086010 (2025) - Published 14 October, 2025
Arkapal Mondal, Sarthak Parikh, Pulak Pradhan, and Ritu Sengar
Phys. Rev. D 112, 086011 (2025) - Published 17 October, 2025
Dmitry S. Ageev, Vasilii V. Pushkarev, and Anastasia N. Zueva
Phys. Rev. D 112, 086012 (2025) - Published 20 October, 2025
Yongjun Ahn, Matteo Baggioli, Yanyan Bu, Masataka Matsumoto, and Xiyang Sun
Phys. Rev. D 112, 086013 (2025) - Published 22 October, 2025
Gabriele Barca and Steffen Gielen
Phys. Rev. D 112, 086014 (2025) - Published 24 October, 2025
Gary T. Horowitz and Guanyu (Ricky) Lu
Phys. Rev. D 112, 086015 (2025) - Published 28 October, 2025
Akash Singh and K. P. Yogendran
Phys. Rev. D 112, 086016 (2025) - Published 28 October, 2025
Filipe H. C. Menezes and N. Yokomizo
Phys. Rev. D 112, 086017 (2025) - Published 28 October, 2025
José Barrientos, Nicolás Cáceres, Felipe Diaz, and Ulises Hernandez-Vera
Phys. Rev. D 112, 086018 (2025) - Published 28 October, 2025
Sanjay Pant, Shagun Kaushal, Arpit Maurya, and Himanshu Parihar
Phys. Rev. D 112, 086019 (2025) - Published 28 October, 2025
Wu-zhong Guo, Song He, and Yu-Xuan Zhang
Phys. Rev. D 112, 086020 (2025) - Published 29 October, 2025
Isabella Marzola, Everson H. Rodrigues, Anderson F. Coelho, and Odilon Lourenço
Phys. Rev. D 112, 089901 (2025) - Published 6 October, 2025
I. F. Cunha and A. C. Lehum
Phys. Rev. D 112, 089902 (2025) - Published 29 October, 2025