Yong Gao, Hao-Jui Kuan, Cheng-Jun Xia, Hector O. Silva, and Masaru Shibata
Phys. Rev. D 112, 123006 (2025) - Published 3 December, 2025
As binary neutron stars inspiral toward each other, the tides raise can excite fluid and elastic modes on these neutron stars. The authors show using a realistic stellar model that these modes can a small phase shift in the merger waveforms. In addition, these modes can reach such amplitudes that they can lead to crust breaking, which potentially can release tremendous amounts of energy into the magnetosphere, which would be a powerful precursor to the final merger.
Henrique Gieg, Maximiliano Ujevic, Armen Sedrakian, and Tim Dietrich
Phys. Rev. D 112, 123008 (2025) - Published 3 December, 2025
This paper provides a new set of numerical relativity simulations of merging binary neutron stars, geared towards identifying possible observable signatures of the slope of the symmetry energy. It discusses the role played by different definitions of tidal deformability and differences in the gravitational wave signals and ejecta.
Yiwei Bao, Ruo-Yu Liu, Gwenael Giacinti, Hai-Ming Zhang, and Yang Chen
Phys. Rev. D 112, 123017 (2025) - Published 5 December, 2025
GeV gamma-ray emission is frequently observed both at large angular separation from pulsars and are not always centered around these pulsars. Using GPU-acceleration monte-carlo simulations, the authors provide a compelling explanation that the propogation of 100 GeV electrons that produce these gamma-rays in the turbulent interstellar magnetic field both leads to off-center peaks and wide separation, e.g., a gamma-ray mirage. These mirages can help constrain the properties of the interstellar magnetic field.
Swarnim Shashank, Askar B. Abdikamalov, Honghui Liu, Abdurakhmon Nosirov, Cosimo Bambi, Indu K. Dihingia, and Yosuke Mizuno
Phys. Rev. D 112, 123030 (2025) - Published 18 December, 2025
The authors use accretion-disk general relativistic magnetohydrodynamic simulations to simulate NuSTAR spectra and assess the ability of widely used X-ray reflection models to recover black hole spins. They demonstrate that only high spins are likely to be correctly predicted, and discuss limitations of lamppost models.
C. Prévotat, Zh. Zhu, S. Koldobskiy, A. Neronov, D. Semikoz, and M. Ahlers
Phys. Rev. D 112, 123033 (2025) - Published 19 December, 2025
As cosmic rays propagate through the Galaxy, they produce gamma rays and contribute to the gamma-ray background. The authors compute the expected gamma-ray background based on the observed cosmic ray flux. They show an overproduction of gamma-ray above 100 TeV, which they suggest is due to the rarity of 1 PeV cosmic-ray sources. Their work helps constrain the sources of high energy cosmic rays.
R. C. H. Gomes et al. (DES Collaboration)
Phys. Rev. D 112, 123515 (2025) - Published 4 December, 2025
The authors demonstrate that combining the third-order aperture mass statistic with the two point correlation function on Dark Energy Survey Year 3 cosmic shear data leads to a 111% (22%) improved figure-of-merit on the joint Ωₘ-S₈ (S₈-w₀) constraint. They further show that the tension to Planck data is thus at the 2.3σ level.
Laura Bernard, Suvendu Giri, Luis Lehner, and Riccardo Sturani
Phys. Rev. D 112, 124013 (2025) - Published 3 December, 2025
Treating deviations from general relativity (GR) in the framework of effective field theories (EFT), the authors develop a formalism for computing gravitational waveforms in the inspiral phase of binary black hole coalescence. The authors work within the post-Newtonian expansion to characterize the deviations. These results can be used in ongoing experimental tests of GR in the inspiral phase.
V. Niarchos, C. Papageorgakis, A. Stratoudakis, and M. Woolley
Phys. Rev. D 112, 126012 (2025) - Published 16 December, 2025
The authors present a new numerical method for studying thermal quantum field theories, where ordinary techniques often struggle. The work is part of a larger ”bootstrap” effort in the theoretical physics community, where instead of solving a particular theory, the aim is to constrain the space of theories, in some cases enough to isolate a particular theory of interest. Here the constraints come from the Kubo-Martin-Schwinger condition and thermal dispersion relations. Additionally, connecting this work to progress in machine learning, the strategy uses a neural network to model the contribution from an infinite number of higher spin operators.
Gen Ye and Yong Cai
Phys. Rev. D 112, L121301 (2025) - Published 2 December, 2025
Pier Giuseppe Catinari, Loris Del Grosso, Luca Di Giovanni, and Alfredo Urbano
Phys. Rev. D 112, L121302 (2025) - Published 3 December, 2025
Alexander J. Silenko
Phys. Rev. D 112, L121303 (2025) - Published 29 December, 2025
Daniele Malafarina, Hrishikesh Chakrabarty, and Ilia Musco
Phys. Rev. D 112, L121304 (2025) - Published 30 December, 2025
Jinsu Kim, Danho Ahn, Soohyung Lee, Saebyeok Ahn, Woohyun Chung, Ohjoon Kwon, Andrei Matlashov, Sergey V. Uchaikin, Boris I. Ivanov, Ki Woong Lee, Arjan Ferdinand van Loo, Yasunobu Nakamura, Seongtae Park, HeeSu Byun, Seonjeong Oh, Dojun Youm, and Yannis K. Semertzidis
Phys. Rev. D 112, L121305 (2025) - Published 30 December, 2025
Joan Fontbuté, Sebastiano Bernuzzi, Piero Rettegno, Simone Albanesi, and Wolfgang Tichy
Phys. Rev. D 112, L121501 (2025) - Published 1 December, 2025
Max Joseph Fahn and Alessandro Pesci
Phys. Rev. D 112, L121502 (2025) - Published 8 December, 2025
Simone Albanesi, Rossella Gamba, Sebastiano Bernuzzi, Joan Fontbuté, Alejandra Gonzalez, and Alessandro Nagar
Phys. Rev. D 112, L121503 (2025) - Published 15 December, 2025
Ivan Kolář, David Kubizňák, and Poula Tadros
Phys. Rev. D 112, L121504 (2025) - Published 18 December, 2025
Florian Niedermann and Antonio Padilla
Phys. Rev. D 112, L121505 (2025) - Published 30 December, 2025
Jia-Ming Dong, Yueshui Zhang, Kai-Wen Huang, Hong-Hao Tu, and Ying-Hai Wu
Phys. Rev. D 112, L121701 (2025) - Published 3 December, 2025
Aleksander Głódkowski, Paweł Matus, Francisco Peña-Benítez, and Lazaros Tsaloukidis
Phys. Rev. D 112, L121702 (2025) - Published 15 December, 2025
Roberto Balbinot, Alessandro Fabbri, Giorgio Ciliberto, and Nicolas Pavloff
Phys. Rev. D 112, L121703 (2025) - Published 15 December, 2025
Jiaju Zhang
Phys. Rev. D 112, L121901 (2025) - Published 5 December, 2025
Jacques Ding, Eleonora Capocasa, Isander Ahrend, Fangfei Liu, Yuhang Zhao, and Matteo Barsuglia
Phys. Rev. D 112, 122001 (2025) - Published 1 December, 2025
Anthony D. Manni, Christopher R. Schwarze, David S. Simon, Abdoulaye Ndao, and Alexander V. Sergienko
Phys. Rev. D 112, 122002 (2025) - Published 5 December, 2025
Wenshuai Liu, Yiming Dong, Ziming Wang, and Lijing Shao
Phys. Rev. D 112, 122003 (2025) - Published 4 December, 2025
Yohei Nishino
Phys. Rev. D 112, 122004 (2025) - Published 5 December, 2025
J. Hou et al.
Phys. Rev. D 112, 122005 (2025) - Published 15 December, 2025
Daniel Voigt and Oliver Gerberding
Phys. Rev. D 112, 122006 (2025) - Published 15 December, 2025
Keisi Kacanja, Kanchan Soni, and Alexander H. Nitz
Phys. Rev. D 112, 122007 (2025) - Published 22 December, 2025
Marcos O. Celi, Mauro Mariani, Milva G. Orsaria, Ignacio F. Ranea-Sandoval, and Germán Lugones
Phys. Rev. D 112, 123001 (2025) - Published 1 December, 2025
Hadrien Paugnat, Tommaso Treu, and Daniel Gilman
Phys. Rev. D 112, 123002 (2025) - Published 1 December, 2025
Slava G. Turyshev
Phys. Rev. D 112, 123003 (2025) - Published 1 December, 2025
Maria de Lluc Planas, Antoni Ramos-Buades, Cecilio García-Quirós, Héctor Estellés, Sascha Husa, and Maria Haney
Phys. Rev. D 112, 123004 (2025) - Published 1 December, 2025
K. Kunnumkai, A. Palmese, M. Bulla, T. Dietrich, A. M. Farah, and P. T. H. Pang
Phys. Rev. D 112, 123005 (2025) - Published 4 December, 2025
Yong Gao, Hao-Jui Kuan, Cheng-Jun Xia, Hector O. Silva, and Masaru Shibata
Phys. Rev. D 112, 123006 (2025) - Published 3 December, 2025
As binary neutron stars inspiral toward each other, the tides raise can excite fluid and elastic modes on these neutron stars. The authors show using a realistic stellar model that these modes can a small phase shift in the merger waveforms. In addition, these modes can reach such amplitudes that they can lead to crust breaking, which potentially can release tremendous amounts of energy into the magnetosphere, which would be a powerful precursor to the final merger.
Alexey Lichkunov, Konstantin Stankevich, and Alexander Studenikin
Phys. Rev. D 112, 123007 (2025) - Published 4 December, 2025
Henrique Gieg, Maximiliano Ujevic, Armen Sedrakian, and Tim Dietrich
Phys. Rev. D 112, 123008 (2025) - Published 3 December, 2025
This paper provides a new set of numerical relativity simulations of merging binary neutron stars, geared towards identifying possible observable signatures of the slope of the symmetry energy. It discusses the role played by different definitions of tidal deformability and differences in the gravitational wave signals and ejecta.
Uddipan Banik and Amitava Bhattacharjee
Phys. Rev. D 112, 123009 (2025) - Published 3 December, 2025
Elena Pinetti, Veronika Vodeb, Aurelio Amerio, Alessandro Cuoco, Stefano Camera, Nicolao Fornengo, and Gabrijela Zaharijas
Phys. Rev. D 112, 123010 (2025) - Published 4 December, 2025
Sandra Robles, Drona Vatsyayan, and Giorgio Busoni
Phys. Rev. D 112, 123011 (2025) - Published 4 December, 2025
Ashish Kumar Meena and Prasenjit Saha
Phys. Rev. D 112, 123012 (2025) - Published 4 December, 2025
Jaiyul Yoo, Matteo Magi, and Dragan Huterer
Phys. Rev. D 112, 123013 (2025) - Published 4 December, 2025
Hermano Velten, Felipe S. Escórcio, and Nadson J. S. Trindade
Phys. Rev. D 112, 123014 (2025) - Published 4 December, 2025
B. Theodore Zhang, Shigeo S. Kimura, and Kohta Murase
Phys. Rev. D 112, 123015 (2025) - Published 5 December, 2025
Carlos Blanco, Dan Hooper, Tim Linden, and Elena Pinetti
Phys. Rev. D 112, 123016 (2025) - Published 5 December, 2025
Yiwei Bao, Ruo-Yu Liu, Gwenael Giacinti, Hai-Ming Zhang, and Yang Chen
Phys. Rev. D 112, 123017 (2025) - Published 5 December, 2025
GeV gamma-ray emission is frequently observed both at large angular separation from pulsars and are not always centered around these pulsars. Using GPU-acceleration monte-carlo simulations, the authors provide a compelling explanation that the propogation of 100 GeV electrons that produce these gamma-rays in the turbulent interstellar magnetic field both leads to off-center peaks and wide separation, e.g., a gamma-ray mirage. These mirages can help constrain the properties of the interstellar magnetic field.
Gabriela Sato-Polito, Matias Zaldarriaga, and Eliot Quataert
Phys. Rev. D 112, 123018 (2025) - Published 8 December, 2025
Nabendu Kumar Khan, Anupam Ray, Girish Kulkarni, and Basudeb Dasgupta
Phys. Rev. D 112, 123019 (2025) - Published 9 December, 2025
Le-Feng Chen, Heng-Yi Yuan, Meng-Hua Zhou, Kun Lu, Jing-Yi Wu, and Kilar Zhang
Phys. Rev. D 112, 123020 (2025) - Published 9 December, 2025
Anirudh Chandra Shekar, Chiara Lisotti, Nityasa Mishra, Ciaran A. J. O’Hare, and Louis E. Strigari
Phys. Rev. D 112, 123021 (2025) - Published 9 December, 2025
Cannon M. Vogel, Helena García Escudero, and Kevork N. Abazajian
Phys. Rev. D 112, 123022 (2025) - Published 11 December, 2025
Beverly Lowell, Jonatan Jacquemin-Ide, Matthew Liska, and Alexander Tchekhovskoy
Phys. Rev. D 112, 123023 (2025) - Published 11 December, 2025
Gabriel Luis Dizon
Phys. Rev. D 112, 123024 (2025) - Published 15 December, 2025
Colter J. Richardson, Anthony Mezzacappa, Kya Schluterman, Haakon Andresen, Eric J. Lentz, Pedro Marronetti, R. Daniel Murphy, and Michele Zanolin
Phys. Rev. D 112, 123025 (2025) - Published 15 December, 2025
Meng-Jie Zhao, Xing-Jian Lv, Xiao-Jun Bi, Kun Fang, and Peng-Fei Yin
Phys. Rev. D 112, 123026 (2025) - Published 16 December, 2025
Tomoki Wada
Phys. Rev. D 112, 123027 (2025) - Published 15 December, 2025
Martin Lemoine, Virginia Bresci, and Laurent Gremillet
Phys. Rev. D 112, 123028 (2025) - Published 15 December, 2025
Tamaz Kereselidze, Irakli Noselidze, and Malcolm Druett
Phys. Rev. D 112, 123029 (2025) - Published 16 December, 2025
Swarnim Shashank, Askar B. Abdikamalov, Honghui Liu, Abdurakhmon Nosirov, Cosimo Bambi, Indu K. Dihingia, and Yosuke Mizuno
Phys. Rev. D 112, 123030 (2025) - Published 18 December, 2025
The authors use accretion-disk general relativistic magnetohydrodynamic simulations to simulate NuSTAR spectra and assess the ability of widely used X-ray reflection models to recover black hole spins. They demonstrate that only high spins are likely to be correctly predicted, and discuss limitations of lamppost models.
Tingyu Zhang, Hiroyuki Tajima, and Motoi Tachibana
Phys. Rev. D 112, 123031 (2025) - Published 18 December, 2025
A. Neronov, O. Kalashev, D. V. Semikoz, D. Savchenko, and M. Poleshchuk
Phys. Rev. D 112, 123032 (2025) - Published 19 December, 2025
C. Prévotat, Zh. Zhu, S. Koldobskiy, A. Neronov, D. Semikoz, and M. Ahlers
Phys. Rev. D 112, 123033 (2025) - Published 19 December, 2025
As cosmic rays propagate through the Galaxy, they produce gamma rays and contribute to the gamma-ray background. The authors compute the expected gamma-ray background based on the observed cosmic ray flux. They show an overproduction of gamma-ray above 100 TeV, which they suggest is due to the rarity of 1 PeV cosmic-ray sources. Their work helps constrain the sources of high energy cosmic rays.
Yu-Mei Wu, Yan-Chen Bi, and Qing-Guo Huang
Phys. Rev. D 112, 123034 (2025) - Published 19 December, 2025
B. X. Zhou (周博修), H. C. Das, J. B. Wei (魏金标), G. F. Burgio, Z. H. Li (李增花), and H.-J. Schulze
Phys. Rev. D 112, 123035 (2025) - Published 19 December, 2025
Andrew Eberhardt, Qiuyue Liang, and Elisa G. M. Ferreira
Phys. Rev. D 112, 123036 (2025) - Published 19 December, 2025
Adya Shukla, A. Gopakumar, and Paramasivan Arumugam
Phys. Rev. D 112, 123037 (2025) - Published 19 December, 2025
N. V. Krishnendu, Frank Ohme, and K. G. Arun
Phys. Rev. D 112, 123038 (2025) - Published 22 December, 2025
Yi Qiu, David Radice, Sherwood Richers, Federico Maria Guercilena, Albino Perego, and Maitraya Bhattacharyya
Phys. Rev. D 112, 123039 (2025) - Published 23 December, 2025
Amit Kumar, Sayan Chakrabarti, and Santabrata Das
Phys. Rev. D 112, 123040 (2025) - Published 23 December, 2025
Sebastian Blacker and Andreas Bauswein
Phys. Rev. D 112, 123041 (2025) - Published 23 December, 2025
A. Abdul Halim et al. (The Pierre Auger Collaboration)
Phys. Rev. D 112, 123042 (2025) - Published 23 December, 2025
Sailesh Ranjan Mohanty, Utkarsh Mali, H. C. Das, Bharat Kumar, and Philippe Landry
Phys. Rev. D 112, 123043 (2025) - Published 26 December, 2025
Aretaios Lalakos, Alexander Tchekhovskoy, Elias R. Most, Bart Ripperda, Koushik Chatterjee, and Matthew Liska
Phys. Rev. D 112, 123044 (2025) - Published 26 December, 2025
Zoha Laraib and Sherwood Richers
Phys. Rev. D 112, 123045 (2025) - Published 29 December, 2025
Sviatoslav Khukhlaev and Stanislav Babak
Phys. Rev. D 112, 123046 (2025) - Published 29 December, 2025
Rodrigo Fernández, Silas Janke, Coleman Dean, and Irene Tamborra
Phys. Rev. D 112, 123047 (2025) - Published 29 December, 2025
P. S. Aswathi, William E. East, Nils Siemonsen, Ling Sun, and Dana Jones
Phys. Rev. D 112, 123048 (2025) - Published 29 December, 2025
Basudeb Dasgupta and Dwaipayan Mukherjee
Phys. Rev. D 112, 123049 (2025) - Published 29 December, 2025
Francisco R. Candón, Pablo Casaseca, Maurizio Giannotti, Mathieu Kaltschmidt, Jaime Ruz, and Julia K. Vogel
Phys. Rev. D 112, 123050 (2025) - Published 29 December, 2025
Zhen Cao et al. (LHAASO Collaboration)
Phys. Rev. D 112, 123051 (2025) - Published 29 December, 2025
Prasanna. M. Joshi and Reinhard Prix
Phys. Rev. D 112, 123052 (2025) - Published 29 December, 2025
Yadong Xue and Zhoujian Cao
Phys. Rev. D 112, 123053 (2025) - Published 30 December, 2025
Jam Sadiq, Thomas Dent, and Ana Lorenzo-Medina
Phys. Rev. D 112, 123054 (2025) - Published 30 December, 2025
Raniere de Menezes, Francesco Massaro, Elisa Visentin, Federico Di Pierro, and Haocheng Zhang
Phys. Rev. D 112, 123055 (2025) - Published 30 December, 2025
Y. S. Abylkairov, M. C. Edwards, A. Ostrikov, Y. Tleukhanov, A. Torres-Forné, P. Cerdá-Durán, J. A. Font, M. J. Szczepańczyk, and E. Abdikamalov
Phys. Rev. D 112, 123056 (2025) - Published 31 December, 2025
Clelia Altomonte, Malcolm Fairbairn, and Lucien Heurtier
Phys. Rev. D 112, 123057 (2025) - Published 31 December, 2025
P. Agnes et al. (DarkSide-50 Collaboration)
Phys. Rev. D 112, 123058 (2025) - Published 31 December, 2025
M. M. Musakhanov
Phys. Rev. D 112, 123501 (2025) - Published 1 December, 2025
Jiamin Hou, Zachary Slepian, and Drew Jamieson
Phys. Rev. D 112, 123502 (2025) - Published 1 December, 2025
Saeed Fakhry, Reyhaneh Vojoudi Salmani, and Javad T. Firouzjaee
Phys. Rev. D 112, 123503 (2025) - Published 1 December, 2025
Naonori Sugiyama
Phys. Rev. D 112, 123504 (2025) - Published 1 December, 2025
Sunao Sugiyama and Minsu Park
Phys. Rev. D 112, 123505 (2025) - Published 2 December, 2025
C. Winckler, P. P. Avelino, and L. Sousa
Phys. Rev. D 112, 123506 (2025) - Published 3 December, 2025
Boryana Hadzhiyska, Simone Ferraro, Gerrit S. Farren, Noah Sailer, and Rongpu Zhou
Phys. Rev. D 112, 123507 (2025) - Published 3 December, 2025
Cannon M. Vogel, Helena García Escudero, Julien Froustey, and Kevork N. Abazajian
Phys. Rev. D 112, 123508 (2025) - Published 3 December, 2025
Zachary J. Hoelscher, Thomas W. Kephart, and Kelly Holley-Bockelmann
Phys. Rev. D 112, 123509 (2025) - Published 4 December, 2025
Liang Xiao, Limin Lai, Zhujun Jiang, Xiao-Dong Li, and Le Zhang
Phys. Rev. D 112, 123510 (2025) - Published 4 December, 2025
Simon Biquard, Josquin Errard, and Radek Stompor
Phys. Rev. D 112, 123511 (2025) - Published 4 December, 2025
Juan Gutiérrez and Macarena Lagos
Phys. Rev. D 112, 123512 (2025) - Published 4 December, 2025
Toshiya Namikawa, Kai Murai, and Fumihiro Naokawa
Phys. Rev. D 112, 123513 (2025) - Published 5 December, 2025
R. C. H. Gomes et al. (DES Collaboration)
Phys. Rev. D 112, 123514 (2025) - Published 4 December, 2025
R. C. H. Gomes et al. (DES Collaboration)
Phys. Rev. D 112, 123515 (2025) - Published 4 December, 2025
The authors demonstrate that combining the third-order aperture mass statistic with the two point correlation function on Dark Energy Survey Year 3 cosmic shear data leads to a 111% (22%) improved figure-of-merit on the joint Ωₘ-S₈ (S₈-w₀) constraint. They further show that the tension to Planck data is thus at the 2.3σ level.
Nahuel Mirón-Granese and Claudia G. Scóccola
Phys. Rev. D 112, 123516 (2025) - Published 5 December, 2025
Zhen-Min Zeng, Cheng-Jun Fang, and Zong-Kuan Guo
Phys. Rev. D 112, 123517 (2025) - Published 5 December, 2025
Simran Arora, Antonio De Felice, and Shinji Mukohyama
Phys. Rev. D 112, 123518 (2025) - Published 5 December, 2025
Ze-Yu Peng, Jun-Qian Jiang, Hao Wang, and Yun-Song Piao
Phys. Rev. D 112, 123519 (2025) - Published 8 December, 2025
J. A. Zebrowski et al. (SPT-3G Collaboration)
Phys. Rev. D 112, 123520 (2025) - Published 8 December, 2025
I. Dankovsky, S. Ramazanov, E. Babichev, D. Gorbunov, and A. Vikman
Phys. Rev. D 112, 123521 (2025) - Published 10 December, 2025
Yu. Kulinich, B. Novosyadlyj, M. Tsizh, and N. Fortuna
Phys. Rev. D 112, 123522 (2025) - Published 12 December, 2025
Anton A. Smirnov, Anisa T. Bajkova, Vadim V. Bobylev, and Viktor D. Zozulia
Phys. Rev. D 112, 123523 (2025) - Published 12 December, 2025
Kimihiro Nomura, Hidetoshi Omiya, and Takahiro Tanaka
Phys. Rev. D 112, 123524 (2025) - Published 12 December, 2025
John McDonald
Phys. Rev. D 112, 123525 (2025) - Published 15 December, 2025
Yuting Liu and Masamune Oguri
Phys. Rev. D 112, 123526 (2025) - Published 15 December, 2025
Zhi-Chao Zhao, Dong-Mei Xia, and Sai Wang
Phys. Rev. D 112, 123527 (2025) - Published 15 December, 2025
Thomas W. Baumgarte, Katy Clough, and John T. Giblin, Jr.
Phys. Rev. D 112, 123528 (2025) - Published 17 December, 2025
Jessica Santiago, Justin Feng, Sebastian Schuster, and Matt Visser
Phys. Rev. D 112, 123529 (2025) - Published 17 December, 2025
John Ellis, Tony Gherghetta, Kunio Kaneta, Wenqi Ke, and Keith A. Olive
Phys. Rev. D 112, 123530 (2025) - Published 17 December, 2025
P. P. Avelino, A. R. Gomes, and D. A. Tamayo
Phys. Rev. D 112, 123531 (2025) - Published 17 December, 2025
Sheng-Han Zhou, Tian-Nuo Li, Guo-Hong Du, Jun-Qian Jiang, Jing-Fei Zhang, and Xin Zhang
Phys. Rev. D 112, 123532 (2025) - Published 17 December, 2025
A. S. Dmitriev, D. G. Levkov, A. G. Panin, and I. I. Tkachev
Phys. Rev. D 112, 123533 (2025) - Published 18 December, 2025
Mathieu Gross, Yann Mambrini, and Md Riajul Haque
Phys. Rev. D 112, 123534 (2025) - Published 19 December, 2025
Shengzhu Wang, Antón Baleato Lizancos, and José Luis Bernal
Phys. Rev. D 112, 123535 (2025) - Published 19 December, 2025
Jose J. Blanco-Pillado, Daniel Jiménez-Aguilar, and Oriol Pujolàs
Phys. Rev. D 112, 123536 (2025) - Published 23 December, 2025
Mazaharul Abedin, Luis A. Escamilla, Supriya Pan, Eleonora Di Valentino, and Weiqiang Yang
Phys. Rev. D 112, 123537 (2025) - Published 23 December, 2025
Aya Ghaleb, Ameek Malhotra, Gianmassimo Tasinato, and Ivonne Zavala
Phys. Rev. D 112, 123538 (2025) - Published 24 December, 2025
Tonghua Liu, Shuo Cao, and Jieci Wang
Phys. Rev. D 112, 123539 (2025) - Published 26 December, 2025
Santabrata Das, Md Riajul Haque, Jitumani Kalita, Rajesh Karmakar, and Debaprasad Maity
Phys. Rev. D 112, 123540 (2025) - Published 26 December, 2025
Hassan Firouzjahi and Amin Nassiri-Rad
Phys. Rev. D 112, 123541 (2025) - Published 26 December, 2025
Martina La Rosa and Gianmassimo Tasinato
Phys. Rev. D 112, 123542 (2025) - Published 26 December, 2025
Andrew Eberhardt and Lam Hui
Phys. Rev. D 112, 123543 (2025) - Published 30 December, 2025
Utkarsh Giri, Moritz Münchmeyer, and Kendrick M. Smith
Phys. Rev. D 112, 123544 (2025) - Published 29 December, 2025
Sunao Sugiyama, Rafael C. H. Gomes, and Bhuvnesh Jain
Phys. Rev. D 112, 123545 (2025) - Published 29 December, 2025
José Correia, Mark Hindmarsh, Kari Rummukainen, and David J. Weir
Phys. Rev. D 112, 123546 (2025) - Published 29 December, 2025
Ayan Chakraborty, Debaprasad Maity, and Rajesh Mondal
Phys. Rev. D 112, 123547 (2025) - Published 30 December, 2025
Alireza Talebian and Hassan Firouzjahi
Phys. Rev. D 112, 123548 (2025) - Published 31 December, 2025
Shinta Kasuya and Masahiro Kawasaki
Phys. Rev. D 112, 123549 (2025) - Published 31 December, 2025
Nilanjandev Bhaumik, Huai-Ke Guo, and Si-Jiang Liu
Phys. Rev. D 112, 123550 (2025) - Published 31 December, 2025
Matteo Breschi, Rossella Gamba, Gregorio Carullo, Ssohrab Borhanian, and Sebastiano Bernuzzi
Phys. Rev. D 112, 124001 (2025) - Published 1 December, 2025
Haorong Wu, Xilong Fan, and Lixiang Chen
Phys. Rev. D 112, 124002 (2025) - Published 1 December, 2025
Arnab Dhani, Alessandro Camilletti, David Radice, Rahul Kashyap, Bangalore Sathyaprakash, Domenico Logoteta, and Albino Perego
Phys. Rev. D 112, 124003 (2025) - Published 1 December, 2025
Sajad A. Bhat, Avinash Tiwari, Md Arif Shaikh, and Shasvath J. Kapadia
Phys. Rev. D 112, 124004 (2025) - Published 1 December, 2025
Henry W. Y. Wong, Lok W. L. Chan, Isaac C. F. Wong, Rico K. L. Lo, and Tjonnie G. F. Li
Phys. Rev. D 112, 124005 (2025) - Published 1 December, 2025
Eugenio Bianchi and Mauricio Gamonal
Phys. Rev. D 112, 124006 (2025) - Published 1 December, 2025
Matheus F. S. Alves, Bruno P. Pônquio, and L. G. Medeiros
Phys. Rev. D 112, 124007 (2025) - Published 1 December, 2025
Giuseppe Fabiano, Domenico Frattulillo, Christian Pfeifer, and Fabian Wagner
Phys. Rev. D 112, 124008 (2025) - Published 2 December, 2025
Balázs Endre Szigeti, Imre Ferenc Barna, and Gergely Gábor Barnaföldi
Phys. Rev. D 112, 124009 (2025) - Published 2 December, 2025
Ana Lorenzo-Medina, Juan Calderón Bustillo, and Samson H. W. Leong
Phys. Rev. D 112, 124010 (2025) - Published 2 December, 2025
Soichiro Kuwahara and Leo Tsukada
Phys. Rev. D 112, 124011 (2025) - Published 3 December, 2025
Abhishek Hegade K. R., Charles F. Gammie, and Nicolás Yunes
Phys. Rev. D 112, 124012 (2025) - Published 3 December, 2025
Laura Bernard, Suvendu Giri, Luis Lehner, and Riccardo Sturani
Phys. Rev. D 112, 124013 (2025) - Published 3 December, 2025
Treating deviations from general relativity (GR) in the framework of effective field theories (EFT), the authors develop a formalism for computing gravitational waveforms in the inspiral phase of binary black hole coalescence. The authors work within the post-Newtonian expansion to characterize the deviations. These results can be used in ongoing experimental tests of GR in the inspiral phase.
Roberto Onofrio, Alexander R. H. Smith, and Lorenza Viola
Phys. Rev. D 112, 124014 (2025) - Published 3 December, 2025
Marco Calzà, Davide Pedrotti, Guan-Wen Yuan, and Sunny Vagnozzi
Phys. Rev. D 112, 124015 (2025) - Published 3 December, 2025
Xi-Jing Wang, Yuan Meng, Xiao-Mei Kuang, and Kai Liao
Phys. Rev. D 112, 124016 (2025) - Published 3 December, 2025
Tamanna Jain and Piero Rettegno
Phys. Rev. D 112, 124017 (2025) - Published 3 December, 2025
Anirban Dasgupta and Indrani Banerjee
Phys. Rev. D 112, 124018 (2025) - Published 3 December, 2025
Sudhagar Suyamprakasam, Sreekanth Harikumar, Paweł Ciecieląg, Przemysław Figura, Michał Bejger, and Marek Biesiada
Phys. Rev. D 112, 124019 (2025) - Published 4 December, 2025
Harkirat Singh Sahota, Suprit Singh, and Ashish Pandita
Phys. Rev. D 112, 124020 (2025) - Published 4 December, 2025
Michela Silvestrini, Elisa Maggio, Sumanta Chakraborty, and Paolo Pani
Phys. Rev. D 112, 124021 (2025) - Published 4 December, 2025
Li-Ming Cao, Ming-Fei Ji, Liang-Bi Wu, and Yu-Sen Zhou
Phys. Rev. D 112, 124022 (2025) - Published 4 December, 2025
Ajit Kumar Mehta, Digvijay Wadekar, Isha Anantpurkar, Javier Roulet, Tejaswi Venumadhav, Tousif Islam, Jonathan Mushkin, Barak Zackay, and Matias Zaldarriaga
Phys. Rev. D 112, 124023 (2025) - Published 4 December, 2025
Wangyu Ai (艾望余) and Di Wu (吴迪)
Phys. Rev. D 112, 124024 (2025) - Published 4 December, 2025
Prasad Padhye, Kajol Paithankar, and Sanved Kolekar
Phys. Rev. D 112, 124025 (2025) - Published 4 December, 2025
Ana Alonso-Serrano, Luis J. Garay, Marek Liška, and Celia López Pineros
Phys. Rev. D 112, 124026 (2025) - Published 4 December, 2025
Parthajit Biswas, Alokananda Kar, and Anowar Shaikh
Phys. Rev. D 112, 124027 (2025) - Published 4 December, 2025
Raghotham A Kulkarni, Rahul, Soham Bhattacharyya, and Dawood Kothawala
Phys. Rev. D 112, 124028 (2025) - Published 4 December, 2025
Julio Arrechea, Stefano Liberati, Hooman Neshat, and Vania Vellucci
Phys. Rev. D 112, 124029 (2025) - Published 4 December, 2025
Taylor Knapp, Patrick M. Meyers, and Arianna I. Renzini
Phys. Rev. D 112, 124030 (2025) - Published 5 December, 2025
Nils Siemonsen
Phys. Rev. D 112, 124031 (2025) - Published 5 December, 2025
Hassan Firouzjahi
Phys. Rev. D 112, 124032 (2025) - Published 5 December, 2025
Qian Li, Qianchuan Wang, and Junji Jia
Phys. Rev. D 112, 124033 (2025) - Published 5 December, 2025
Lennox S. Keeble and Frans Pretorius
Phys. Rev. D 112, 124034 (2025) - Published 8 December, 2025
Victor H. M. Ramos, João Paulo M. Pitelli, and João C. A. Barata
Phys. Rev. D 112, 124035 (2025) - Published 8 December, 2025
Max Joseph Fahn and Alessandro Pesci
Phys. Rev. D 112, 124036 (2025) - Published 8 December, 2025
Ye Zhang and Zichang Huang
Phys. Rev. D 112, 124037 (2025) - Published 9 December, 2025
Oliver Long, Harald P. Pfeiffer, Lawrence E. Kidder, and Mark A. Scheel
Phys. Rev. D 112, 124038 (2025) - Published 9 December, 2025
Oliver Long, Harald P. Pfeiffer, Alessandra Buonanno, Gustav Uhre Jakobsen, Gustav Mogull, Antoni Ramos-Buades, Hannes R. Rüter, Lawrence E. Kidder, and Mark A. Scheel
Phys. Rev. D 112, 124039 (2025) - Published 9 December, 2025
Aimeric Colléaux, Ivan Kolář, and Tomáš Málek
Phys. Rev. D 112, 124040 (2025) - Published 11 December, 2025
Sojeong Cheong and Wontae Kim
Phys. Rev. D 112, 124041 (2025) - Published 11 December, 2025
Yan Liu, Jie Jiang, and Bing Sun
Phys. Rev. D 112, 124042 (2025) - Published 11 December, 2025
Kitaro Taniguchi, Shunta Nishimura, Naoki Tsukamoto, and Ryotaro Kase
Phys. Rev. D 112, 124043 (2025) - Published 11 December, 2025
Manuel Piarulli, Sylvain Marsat, Elise M. Sänger, Alessandra Buonanno, Jan Steinhoff, and Nicola Tamanini
Phys. Rev. D 112, 124044 (2025) - Published 11 December, 2025
Christopher Whittall, Leor Barack, and Oliver Long
Phys. Rev. D 112, 124045 (2025) - Published 11 December, 2025
Erick I. Duque
Phys. Rev. D 112, 124046 (2025) - Published 11 December, 2025
Shinya Tomizawa, Jun-ichi Sakamoto, and Ryotaku Suzuki
Phys. Rev. D 112, 124047 (2025) - Published 12 December, 2025
Riccardo Falcone and Claudio Conti
Phys. Rev. D 112, 124048 (2025) - Published 12 December, 2025
Iago B. Mendes, Nils L. Vu, Oliver Long, Harald P. Pfeiffer, and Robert Owen
Phys. Rev. D 112, 124049 (2025) - Published 12 December, 2025
Sara Gliorio, Emanuele Berti, Andrea Maselli, and Nicholas Speeney
Phys. Rev. D 112, 124050 (2025) - Published 12 December, 2025
Anuj Kankani and Sean T. McWilliams
Phys. Rev. D 112, 124051 (2025) - Published 15 December, 2025
Ercan Kilicarslan
Phys. Rev. D 112, 124052 (2025) - Published 15 December, 2025
Ernesto Contreras, Mikaela Carrasco-Hidalgo, Pedro Bargueño, and Arthur G. Suvorov
Phys. Rev. D 112, 124053 (2025) - Published 15 December, 2025
Viktor Skoupý, Gabriel Andres Piovano, and Vojtěch Witzany
Phys. Rev. D 112, 124054 (2025) - Published 15 December, 2025
Fabrizio Corelli, Paolo Pani, and Andrea P. Sanna
Phys. Rev. D 112, 124055 (2025) - Published 15 December, 2025
Alexandru Dima, Pierre Heidmann, Marco Melis, Paolo Pani, and Gela Patashuri
Phys. Rev. D 112, 124056 (2025) - Published 15 December, 2025
H. Khodabakhshi, H. Lü, and F. Shojai
Phys. Rev. D 112, 124057 (2025) - Published 15 December, 2025
Prashant Kocherlakota and Ramesh Narayan
Phys. Rev. D 112, 124058 (2025) - Published 16 December, 2025
Maria Rosselló-Sastre and Sascha Husa
Phys. Rev. D 112, 124059 (2025) - Published 16 December, 2025
Andrea Placidi, Elisa Grilli, Marta Orselli, Matteo Pegorin, Nicola Bartolo, and Pierpaolo Mastrolia
Phys. Rev. D 112, 124060 (2025) - Published 17 December, 2025
Gerasimos Kouniatalis, P. A. González, Eleftherios Papantonopoulos, and Yerko Vásquez
Phys. Rev. D 112, 124061 (2025) - Published 17 December, 2025
Gerasimos Kouniatalis, Arthur G. Suvorov, and Kyriakos Destounis
Phys. Rev. D 112, 124062 (2025) - Published 18 December, 2025
Sophia Yi, Francesco Iacovelli, Sylvain Marsat, Digvijay Wadekar, and Emanuele Berti
Phys. Rev. D 112, 124063 (2025) - Published 18 December, 2025
C. N. Pope, D. O. Rohrer, and B. F. Whiting
Phys. Rev. D 112, 124064 (2025) - Published 19 December, 2025
Siddharth Mahesh, Sean T. McWilliams, and Zachariah Etienne
Phys. Rev. D 112, 124065 (2025) - Published 22 December, 2025
Muhammad Haider Khan and Volker Perlick
Phys. Rev. D 112, 124066 (2025) - Published 22 December, 2025
Manuel O. Mariano and C. A. R. Herdeiro
Phys. Rev. D 112, 124067 (2025) - Published 22 December, 2025
Abhishek Hegade K. R., Charles F. Gammie, and Nicolás Yunes
Phys. Rev. D 112, 124068 (2025) - Published 22 December, 2025
Travis Seth Rippentrop, Avijit Bera, and Mustapha Ishak
Phys. Rev. D 112, 124069 (2025) - Published 23 December, 2025
Jeff Steinhauer, Kyriakos Destounis, and Richard Brito
Phys. Rev. D 112, 124070 (2025) - Published 24 December, 2025
Zexin Hu, Daniela D. Doneva, Ziming Wang, Vasileios Paschalidis, Gabriele Bozzola, Stoytcho S. Yazadjiev, and Lijing Shao
Phys. Rev. D 112, 124071 (2025) - Published 24 December, 2025
Reggie C. Pantig and Ali Övgün
Phys. Rev. D 112, 124072 (2025) - Published 24 December, 2025
Christian G. Böhmer and Eissa Al-Nasrallah
Phys. Rev. D 112, 124073 (2025) - Published 24 December, 2025
Sudhir Gholap, Kanchan Soni, Shasvath J. Kapadia, and Sanjeev Dhurandhar
Phys. Rev. D 112, 124074 (2025) - Published 24 December, 2025
Jorge V. Rocha and Diogo L. F. G. Silva
Phys. Rev. D 112, 124075 (2025) - Published 24 December, 2025
Gustav Mogull, Jan Plefka, and Kathrin Stoldt
Phys. Rev. D 112, 124076 (2025) - Published 26 December, 2025
Ratindranath Akhoury, Arielle Schutz, and David Garfinkle
Phys. Rev. D 112, 124077 (2025) - Published 26 December, 2025
Pulkit Bansal, Joseph P. Johnson, and S. Shankaranarayanan
Phys. Rev. D 112, 124078 (2025) - Published 26 December, 2025
Felix Willenborg, Dennis Philipp, and Claus Lämmerzahl
Phys. Rev. D 112, 124079 (2025) - Published 26 December, 2025
Bo-Xuan Ge, Eugene A. Lim, Ulrich Sperhake, Tamara Evstafyeva, Daniela Cors, Eloy de Jong, Robin Croft, and Thomas Helfer
Phys. Rev. D 112, 124080 (2025) - Published 26 December, 2025
Vincent Moncrief and Nathalie E. Rieger
Phys. Rev. D 112, 124081 (2025) - Published 26 December, 2025
Gabriel P. Ribeiro, Renan B. Magalhães, and Luís C. B. Crispino
Phys. Rev. D 112, 124082 (2025) - Published 26 December, 2025
Soichiro Morisaki, Hayato Motohashi, Motoki Suzuki, and Daiki Watarai
Phys. Rev. D 112, 124083 (2025) - Published 29 December, 2025
David Rumler
Phys. Rev. D 112, 124084 (2025) - Published 29 December, 2025
Lars Fischer, Tom Krokotsch, and Gudrid Moortgat-Pick
Phys. Rev. D 112, 124085 (2025) - Published 30 December, 2025
Hyat Huang, Burkhard Kleihaus, Jutta Kunz, Meng-Yun Lai, Eugen Radu, and De-Cheng Zou
Phys. Rev. D 112, 124086 (2025) - Published 30 December, 2025
Gerui Chen, Xiyao Guo, Xin Lan, Hongbao Zhang, and Wei Zhang
Phys. Rev. D 112, 124087 (2025) - Published 31 December, 2025
Antonio Enea Romano
Phys. Rev. D 112, 124088 (2025) - Published 31 December, 2025
Evgenii Ievlev and Mikhail Shifman
Phys. Rev. D 112, 125001 (2025) - Published 1 December, 2025
Yutaro Shoji and Masahide Yamaguchi
Phys. Rev. D 112, 125002 (2025) - Published 1 December, 2025
Pavel Meshcheriakov
Phys. Rev. D 112, 125003 (2025) - Published 1 December, 2025
C. Fulgado-Claudio, P. Sala, D. González-Cuadra, and A. Bermudez
Phys. Rev. D 112, 125004 (2025) - Published 1 December, 2025
Jake C. Stirling
Phys. Rev. D 112, 125005 (2025) - Published 1 December, 2025
Tim Stoetzel, Rebekka Fechtner, and Stefan Floerchinger
Phys. Rev. D 112, 125006 (2025) - Published 3 December, 2025
Shono Shibuya and Sotaro Sugishita
Phys. Rev. D 112, 125007 (2025) - Published 3 December, 2025
Nada Eissa, Carlos R. Ordóñez, and Gustavo Valdivia-Mera
Phys. Rev. D 112, 125008 (2025) - Published 3 December, 2025
Yuanyuan Fang, Jing Feng, and Dan Xie
Phys. Rev. D 112, 125009 (2025) - Published 4 December, 2025
Amiya Mishra
Phys. Rev. D 112, 125010 (2025) - Published 4 December, 2025
João Paulo M. Pitelli, Ricardo A. Mosna, Victor H. M. Ramos, and João C. A. Barata
Phys. Rev. D 112, 125011 (2025) - Published 4 December, 2025
Dario Sauro
Phys. Rev. D 112, 125012 (2025) - Published 5 December, 2025
Carles Batlle, Roberto Casalbuoni, Daniele Dominici, José Figueroa-O’Farrill, and Joaquim Gomis
Phys. Rev. D 112, 125013 (2025) - Published 5 December, 2025
Alessandro Monteverdi and Elizabeth Winstanley
Phys. Rev. D 112, 125014 (2025) - Published 8 December, 2025
D. M. Ghilencea
Phys. Rev. D 112, 125015 (2025) - Published 10 December, 2025
Bitan Roy
Phys. Rev. D 112, 125016 (2025) - Published 12 December, 2025
Emerson B. S. Corrêa, Michelli S. R. Sarges, and José A. Helayël-Neto
Phys. Rev. D 112, 125017 (2025) - Published 15 December, 2025
José Manuel Montes-Armenteros and Javier Olmedo
Phys. Rev. D 112, 125018 (2025) - Published 15 December, 2025
L. A. Ferreira and L. R. Livramento
Phys. Rev. D 112, 125019 (2025) - Published 16 December, 2025
Davide Fioravanti and Daniele Gregori
Phys. Rev. D 112, 125020 (2025) - Published 17 December, 2025
M. Rodriguez Zarate and T. Thiemann
Phys. Rev. D 112, 125021 (2025) - Published 18 December, 2025
V. P. Nair
Phys. Rev. D 112, 125022 (2025) - Published 22 December, 2025
Meer Ashwinkumar, Domenico Orlando, Susanne Reffert, and Giacomo Sberveglieri
Phys. Rev. D 112, 125023 (2025) - Published 19 December, 2025
Jorma Louko, Guillermo A. Mena Marugán, and Alvaro Torres-Caballeros
Phys. Rev. D 112, 125024 (2025) - Published 22 December, 2025
S. Nagy and J. Polonyi
Phys. Rev. D 112, 125025 (2025) - Published 22 December, 2025
A. J. D. Farias Junior, Andrea Erdas, and Herondy F. Santana Mota
Phys. Rev. D 112, 125026 (2025) - Published 22 December, 2025
Giacomo Contri, Gia Dvali, and Otari Sakhelashvili
Phys. Rev. D 112, 125027 (2025) - Published 23 December, 2025
Chiang-Mei Chen, Chun-Chih Huang, Sang Pyo Kim, and Kuan-Yen Lin
Phys. Rev. D 112, 125028 (2025) - Published 24 December, 2025
J. François and L. Ravera
Phys. Rev. D 112, 125029 (2025) - Published 24 December, 2025
Andrés Boasso and Francisco D. Mazzitelli
Phys. Rev. D 112, 125030 (2025) - Published 29 December, 2025
Timothy Gargett and Igor Samsonov
Phys. Rev. D 112, 125031 (2025) - Published 29 December, 2025
Fateme Shojaei Arani, Brahim Lamine, Alain Blanchard, and Malek Bagheri Harouni
Phys. Rev. D 112, 125032 (2025) - Published 31 December, 2025
Seth K. Asante and Björn Borgolte
Phys. Rev. D 112, 126001 (2025) - Published 1 December, 2025
Dongsu Bak, Chanju Kim, and Sang-Heon Yi
Phys. Rev. D 112, 126002 (2025) - Published 2 December, 2025
Anja Alfano, Nick Evans, and Wanxiang Fan
Phys. Rev. D 112, 126003 (2025) - Published 2 December, 2025
Malcolm Perry and Maria J. Rodriguez
Phys. Rev. D 112, 126004 (2025) - Published 3 December, 2025
Nick Evans and Wanxiang Fan
Phys. Rev. D 112, 126005 (2025) - Published 5 December, 2025
Rachel Brown, A. Meenakshi McNamara, Sahil Saini, and Parampreet Singh
Phys. Rev. D 112, 126006 (2025) - Published 10 December, 2025
Irina Ya. Aref’eva, Ali Hajilou, Alexander Nikolaev, and Pavel Slepov
Phys. Rev. D 112, 126007 (2025) - Published 10 December, 2025
Byoungjoon Ahn, Hyun-Sik Jeong, Chang-Woo Ji, Keun-Young Kim, and Kwan Yun
Phys. Rev. D 112, 126008 (2025) - Published 12 December, 2025
Cesar Arias
Phys. Rev. D 112, 126009 (2025) - Published 15 December, 2025
Jonathan J. Heckman, Max Hübner, and Chitraang Murdia
Phys. Rev. D 112, 126010 (2025) - Published 15 December, 2025
Naoto Kan, Masashi Kawahira, and Hiroki Wada
Phys. Rev. D 112, 126011 (2025) - Published 15 December, 2025
V. Niarchos, C. Papageorgakis, A. Stratoudakis, and M. Woolley
Phys. Rev. D 112, 126012 (2025) - Published 16 December, 2025
The authors present a new numerical method for studying thermal quantum field theories, where ordinary techniques often struggle. The work is part of a larger ”bootstrap” effort in the theoretical physics community, where instead of solving a particular theory, the aim is to constrain the space of theories, in some cases enough to isolate a particular theory of interest. Here the constraints come from the Kubo-Martin-Schwinger condition and thermal dispersion relations. Additionally, connecting this work to progress in machine learning, the strategy uses a neural network to model the contribution from an infinite number of higher spin operators.
Michael Gutperle and Christina Yeo
Phys. Rev. D 112, 126013 (2025) - Published 16 December, 2025
Sergio E. Aguilar-Gutierrez, Hugo A. Camargo, Viktor Jahnke, Keun-Young Kim, and Mitsuhiro Nishida
Phys. Rev. D 112, 126014 (2025) - Published 18 December, 2025
A. M. Rodriguez Zarate and T. Thiemann
Phys. Rev. D 112, 126015 (2025) - Published 18 December, 2025
Minyan Ou and Xiangdong Zhang
Phys. Rev. D 112, 126016 (2025) - Published 18 December, 2025
Jong-Hyun Baek and Kang-Sin Choi
Phys. Rev. D 112, 126017 (2025) - Published 18 December, 2025
Thales Azevedo, Alfonso Ballon-Bayona, and Leonardo Pazito
Phys. Rev. D 112, 126018 (2025) - Published 19 December, 2025
Zheng Jiang, Jun Nian, Caiying Shao, Yu Tian, and Hongbao Zhang
Phys. Rev. D 112, 126019 (2025) - Published 19 December, 2025
Daniel Elander, Antón F. Faedo, Maurizio Piai, Ronnie Rodgers, and Javier G. Subils
Phys. Rev. D 112, 126020 (2025) - Published 19 December, 2025
Samuel Kováčik and Katarína Magdolenová
Phys. Rev. D 112, 126021 (2025) - Published 23 December, 2025
S. P. Miao, N. C. Tsamis, and R. P. Woodard
Phys. Rev. D 112, 126022 (2025) - Published 23 December, 2025
Vatche Sahakian
Phys. Rev. D 112, 126023 (2025) - Published 26 December, 2025
Diego Buccio, Gustavo P. de Brito, and Luca Parente
Phys. Rev. D 112, 126024 (2025) - Published 26 December, 2025
Xun Chen, Yidian Chen, and Kai Zhou
Phys. Rev. D 112, 126025 (2025) - Published 26 December, 2025
Patharadanai Nuchino and Parinya Karndumri
Phys. Rev. D 112, 126026 (2025) - Published 30 December, 2025
Gabriel H. S. Aguiar and George E. A. Matsas
Phys. Rev. D 112, 126027 (2025) - Published 30 December, 2025
Nelson R. F. Braga and William S. Cunha
Phys. Rev. D 112, 126028 (2025) - Published 31 December, 2025
Jacob L. Bourjaily, Song He (何颂), Canxin Shi (施灿欣), and Yichao Tang (唐一朝)
Phys. Rev. D 112, 126029 (2025) - Published 31 December, 2025
