J. Amaré, S. Cebrián, D. Cintas, I. Coarasa, E. García, M. Martínez, M. A. Oliván, Y. Ortigoza, A. Ortiz de Solórzano, J. Puimedón, A. Salinas, M. L. Sarsa, and P. Villar
Phys. Rev. D 103, 102005 (2021) - Published 27 May, 2021
The DAMA/LIBRA experiment’s potential dark matter detection went unconfirmed for 20 years. Now, a similar experiment offers evidence against the result.
Minsu Park, Marco Raveri, and Bhuvnesh Jain
Phys. Rev. D 103, 103530 (2021) - Published 21 May, 2021
Next to a cosmological constant ( in ), quintessence is the simplest concept for a physical source of cosmic acceleration which has been studied theoretically by a wide array of models. Here the authors take a “data first” approach, using numerous measurements, from CMB to galaxy lensing, to reconstruct a family of quintessence models via effective field theory (EFT) exclusively from the data and without any assumptions for the potential for the quintessence field.
Pablo A. Cano, Kwinten Fransen, and Thomas Hertog
Phys. Rev. D 103, 103531 (2021) - Published 21 May, 2021
By employing an effective field theory approach, the authors study novel extensions of Starobinsky inflation, involving higher-order curvature corrections that imply that (fluctuation) equations are of second order in time and lead to reasonable cosmologies. Embedding these theories into anti-de Sitter space, holographic unitarity bounds are derived for the dominant corrections which allow for observational predictions despite the additional parameters, which could be tested by the upcoming generation of CMB experiments.
José Luis Bernal, Licia Verde, Raul Jimenez, Marc Kamionkowski, David Valcin, and Benjamin D. Wandelt
Phys. Rev. D 103, 103533 (2021) - Published 26 May, 2021
The authors introduce a new actor in the current drama of the Hubble tension (conflicting measurements of ), namely the age of the Universe , as determined by the oldest globular clusters, and show that if local measurements are correct, the resolution of the Hubble tension implies a modification of the cosmological standard model CDM in the early and late Universe. Once systematic uncertainties are reduced, measuring will discriminate between the viable solutions for the tension, i.e. changing CDM or errors in the local measurements.
Fiona McCarthy, Simon Foreman, and Alexander van Engelen
Phys. Rev. D 103, 103538 (2021) - Published 28 May, 2021
One of the serious hindrances to achieving a major goal of the next generation CMB experiments, the measurement of the sum of the neutrino masses, is the lack of sufficient knowledge of baryonic effects on the matter power spectrum. In this paper, the authors propose several mitigating strategies, which, they show, will serve to reduce these baryonic effects to a negligible level, without significantly increasing the associated statistical uncertainty.
W. N. Polyzou
Phys. Rev. D 103, 105017 (2021) - Published 19 May, 2021
Dirac showed that relativity implied three different forms of quantum mechanics (instant, point, and light-front) depending on how boosts and translation generators account for interactions. However, it is non-trivial to prove that these representations are equivalent in quantum field theory. Here, the author demonstrates using non-perturbative techniques that equivalent representations between instant-form and light-front dynamics can be constructed, based on assumptions of a local quantum field theory.
Francesco Nozzoli and Cinzia Cernetti
Phys. Rev. D 103, L101101 (2021) - Published 19 May, 2021
M. E. Gusakov and A. I. Chugunov
Phys. Rev. D 103, L101301 (2021) - Published 4 May, 2021
Anna Ijjas and Roman Kolevatov
Phys. Rev. D 103, L101302 (2021) - Published 20 May, 2021
Yusuke Mikura, Yuichiro Tada, and Shuichiro Yokoyama
Phys. Rev. D 103, L101303 (2021) - Published 28 May, 2021
R. Abbasi et al. (IceCube Collaboration)
Phys. Rev. D 103, 102001 (2021) - Published 6 May, 2021
H. Abdallah et al. (H.E.S.S. Collaboration)
Phys. Rev. D 103, 102002 (2021) - Published 20 May, 2021
Grégory Baltus, Justin Janquart, Melissa Lopez, Amit Reza, Sarah Caudill, and Jean-René Cudell
Phys. Rev. D 103, 102003 (2021) - Published 18 May, 2021
D. Alesini, C. Braggio, G. Carugno, N. Crescini, D. D’Agostino, D. Di Gioacchino, R. Di Vora, P. Falferi, U. Gambardella, C. Gatti, G. Iannone, C. Ligi, A. Lombardi, G. Maccarrone, A. Ortolan, R. Pengo, A. Rettaroli, G. Ruoso, L. Taffarello, and S. Tocci
Phys. Rev. D 103, 102004 (2021) - Published 20 May, 2021
J. Amaré, S. Cebrián, D. Cintas, I. Coarasa, E. García, M. Martínez, M. A. Oliván, Y. Ortigoza, A. Ortiz de Solórzano, J. Puimedón, A. Salinas, M. L. Sarsa, and P. Villar
Phys. Rev. D 103, 102005 (2021) - Published 27 May, 2021
The DAMA/LIBRA experiment’s potential dark matter detection went unconfirmed for 20 years. Now, a similar experiment offers evidence against the result.
A. Corstanje, S. Buitink, H. Falcke, B. M. Hare, J. R. Hörandel, T. Huege, G. K. Krampah, P. Mitra, K. Mulrey, A. Nelles, H. Pandya, J. P. Rachen, O. Scholten, S. ter Veen, S. Thoudam, G. Trinh, and T. Winchen
Phys. Rev. D 103, 102006 (2021) - Published 28 May, 2021
Amit Bhoonah, Joseph Bramante, Brian Courtman, and Ningqiang Song
Phys. Rev. D 103, 103001 (2021) - Published 3 May, 2021
Andrew L. Miller, Pia Astone, Giacomo Bruno, Sébastien Clesse, Sabrina D’Antonio, Antoine Depasse, Federico De Lillo, Sergio Frasca, Iuri La Rosa, Paola Leaci, Cristiano Palomba, Ornella J. Piccinni, Lorenzo Pierini, Luca Rei, and Andres Tanasijczuk
Phys. Rev. D 103, 103002 (2021) - Published 3 May, 2021
Ting-Ting Sun, Zi-Yue Zheng, Huan Chen, G. Fiorella Burgio, and Hans-Josef Schulze
Phys. Rev. D 103, 103003 (2021) - Published 3 May, 2021
Wen-Cong Chen
Phys. Rev. D 103, 103004 (2021) - Published 4 May, 2021
Allan Sung, Gang Guo, and Meng-Ru Wu
Phys. Rev. D 103, 103005 (2021) - Published 4 May, 2021
Michael J. Williams, John Veitch, and Chris Messenger
Phys. Rev. D 103, 103006 (2021) - Published 5 May, 2021
S. Prohira et al. (Radar Echo Telescope)
Phys. Rev. D 103, 103007 (2021) - Published 6 May, 2021
Soma Mukherjee, Gaukhar Nurbek, and Oscar Valdez
Phys. Rev. D 103, 103008 (2021) - Published 6 May, 2021
Paolo Lipari
Phys. Rev. D 103, 103009 (2021) - Published 10 May, 2021
Odilon Lourenço, César H. Lenzi, Mariana Dutra, Efrain J. Ferrer, Vivian de la Incera, Laura Paulucci, and J. E. Horvath
Phys. Rev. D 103, 103010 (2021) - Published 11 May, 2021
Z. Sharifi, M. Bigdeli, and D. Alvarez-Castillo
Phys. Rev. D 103, 103011 (2021) - Published 12 May, 2021
Wenshuai Liu
Phys. Rev. D 103, 103012 (2021) - Published 14 May, 2021
Chao Zhang (张超), Yungui Gong (龚云贵), Hang Liu (刘航), Bin Wang (王斌), and Chunyu Zhang (张春雨)
Phys. Rev. D 103, 103013 (2021) - Published 14 May, 2021
Masato Shirasaki
Phys. Rev. D 103, 103014 (2021) - Published 18 May, 2021
Bhaskar Biswas, Prasanta Char, Rana Nandi, and Sukanta Bose
Phys. Rev. D 103, 103015 (2021) - Published 19 May, 2021
Michael Korsmeier and Alessandro Cuoco
Phys. Rev. D 103, 103016 (2021) - Published 25 May, 2021
Michael A. Fedderke, Peter W. Graham, and Surjeet Rajendran
Phys. Rev. D 103, 103017 (2021) - Published 21 May, 2021
Zhen Pan and Huan Yang
Phys. Rev. D 103, 103018 (2021) - Published 24 May, 2021
Barry T. Chiang, Hsi-Yu Schive (薛熙于), and Tzihong Chiueh (闕志鴻)
Phys. Rev. D 103, 103019 (2021) - Published 24 May, 2021
Viviana Niro
Phys. Rev. D 103, 103020 (2021) - Published 26 May, 2021
Zhen Zhang, Peng-Cheng Chu, Xiao-Hua Li, He Liu, and Xiao-Min Zhang
Phys. Rev. D 103, 103021 (2021) - Published 27 May, 2021
Federico Cattorini, Bruno Giacomazzo, Francesco Haardt, and Monica Colpi
Phys. Rev. D 103, 103022 (2021) - Published 28 May, 2021
Askar B. Abdikamalov, Dimitry Ayzenberg, Cosimo Bambi, Honghui Liu, and Yuexin Zhang
Phys. Rev. D 103, 103023 (2021) - Published 28 May, 2021
Man Leong Chan and Kazuhiro Hayama
Phys. Rev. D 103, 103024 (2021) - Published 28 May, 2021
J. Iguaz, P. D. Serpico, and T. Siegert
Phys. Rev. D 103, 103025 (2021) - Published 28 May, 2021
Ming-Yue Zhou, Xin-Chun Hu, Bobing Ye, Shoucun Hu, Dong-Dong Zhu, Xuefeng Zhang, Wei Su, and Yan Wang
Phys. Rev. D 103, 103026 (2021) - Published 28 May, 2021
Peter Adshead and Kaloian D. Lozanov
Phys. Rev. D 103, 103501 (2021) - Published 4 May, 2021
José Ramón Bermejo-Climent, Mario Ballardini, Fabio Finelli, Daniela Paoletti, Roy Maartens, José Alberto Rubiño-Martín, and Luca Valenziano
Phys. Rev. D 103, 103502 (2021) - Published 4 May, 2021
Charuhas Shiveshwarkar, Drew Jamieson, and Marilena Loverde
Phys. Rev. D 103, 103503 (2021) - Published 4 May, 2021
Oliver H. E. Philcox
Phys. Rev. D 103, 103504 (2021) - Published 5 May, 2021
Jose Beltrán Jiménez, Dario Bettoni, and Philippe Brax
Phys. Rev. D 103, 103505 (2021) - Published 5 May, 2021
Vivian I. Sabla and Robert R. Caldwell
Phys. Rev. D 103, 103506 (2021) - Published 7 May, 2021
A. Palmese and A. G. Kim
Phys. Rev. D 103, 103507 (2021) - Published 7 May, 2021
Adrienne L. Erickcek, Pranjal Ralegankar, and Jessie Shelton
Phys. Rev. D 103, 103508 (2021) - Published 10 May, 2021
C. Krishnan, E. Ó Colgáin, M. M. Sheikh-Jabbari, and Tao Yang
Phys. Rev. D 103, 103509 (2021) - Published 10 May, 2021
Y. Sultan Abylkairov, Omar Darwish, J. Colin Hill, and Blake D. Sherwin
Phys. Rev. D 103, 103510 (2021) - Published 11 May, 2021
Federico Di Gioia, Giulia Maniccia, Giovanni Montani, and Jacopo Niedda
Phys. Rev. D 103, 103511 (2021) - Published 10 May, 2021
Jose J. Blanco-Pillado, Ken D. Olum, and Jeremy M. Wachter
Phys. Rev. D 103, 103512 (2021) - Published 11 May, 2021
Rubén Arjona, Hai-Nan Lin, Savvas Nesseris, and Li Tang
Phys. Rev. D 103, 103513 (2021) - Published 11 May, 2021
Nikita Blinov, Matthew J. Dolan, Patrick Draper, and Jessie Shelton
Phys. Rev. D 103, 103514 (2021) - Published 12 May, 2021
Fiona McCarthy and Mathew S. Madhavacheril
Phys. Rev. D 103, 103515 (2021) - Published 12 May, 2021
Yi-Hsiung Hsu ((許藝薰)) and Tzihong Chiueh ((闕志鴻))
Phys. Rev. D 103, 103516 (2021) - Published 13 May, 2021
Asanka Amarasinghe and Philip D. Mannheim
Phys. Rev. D 103, 103517 (2021) - Published 14 May, 2021
Theodore Steele and Tobias Baldauf
Phys. Rev. D 103, 103518 (2021) - Published 14 May, 2021
R. A. C. Correa, P. H. R. S. Moraes, A. de Souza Dutra, O. L. Dors, W. de Paula, and T. Frederico
Phys. Rev. D 103, 103519 (2021) - Published 14 May, 2021
Xiao Wang, Fa Peng Huang, and Xinmin Zhang
Phys. Rev. D 103, 103520 (2021) - Published 17 May, 2021
Wompherdeiki Khyllep, Andronikos Paliathanasis, and Jibitesh Dutta
Phys. Rev. D 103, 103521 (2021) - Published 17 May, 2021
Drew Jamieson and Marilena Loverde
Phys. Rev. D 103, 103522 (2021) - Published 17 May, 2021
Joerg Jaeckel and Sebastian Schenk
Phys. Rev. D 103, 103523 (2021) - Published 17 May, 2021
Jorge Enrique García-Farieta, Wojciech A. Hellwing, Suhani Gupta, and Maciej Bilicki
Phys. Rev. D 103, 103524 (2021) - Published 17 May, 2021
Caroline Jonas, Jean-Luc Lehners, and Jerome Quintin
Phys. Rev. D 103, 103525 (2021) - Published 17 May, 2021
Mukul Bhattacharya, Pawan Kumar, and Eric V. Linder
Phys. Rev. D 103, 103526 (2021) - Published 19 May, 2021
Gong Cheng, Fengquan Wu, and Xuelei Chen
Phys. Rev. D 103, 103527 (2021) - Published 19 May, 2021
Tanmay Vachaspati and Alexander Vilenkin
Phys. Rev. D 103, 103528 (2021) - Published 20 May, 2021
Guillaume Boileau, Nelson Christensen, Renate Meyer, and Neil J. Cornish
Phys. Rev. D 103, 103529 (2021) - Published 21 May, 2021
Minsu Park, Marco Raveri, and Bhuvnesh Jain
Phys. Rev. D 103, 103530 (2021) - Published 21 May, 2021
Next to a cosmological constant ( in ), quintessence is the simplest concept for a physical source of cosmic acceleration which has been studied theoretically by a wide array of models. Here the authors take a “data first” approach, using numerous measurements, from CMB to galaxy lensing, to reconstruct a family of quintessence models via effective field theory (EFT) exclusively from the data and without any assumptions for the potential for the quintessence field.
Pablo A. Cano, Kwinten Fransen, and Thomas Hertog
Phys. Rev. D 103, 103531 (2021) - Published 21 May, 2021
By employing an effective field theory approach, the authors study novel extensions of Starobinsky inflation, involving higher-order curvature corrections that imply that (fluctuation) equations are of second order in time and lead to reasonable cosmologies. Embedding these theories into anti-de Sitter space, holographic unitarity bounds are derived for the dominant corrections which allow for observational predictions despite the additional parameters, which could be tested by the upcoming generation of CMB experiments.
Siyang Ling and Andrew J. Long
Phys. Rev. D 103, 103532 (2021) - Published 21 May, 2021
José Luis Bernal, Licia Verde, Raul Jimenez, Marc Kamionkowski, David Valcin, and Benjamin D. Wandelt
Phys. Rev. D 103, 103533 (2021) - Published 26 May, 2021
The authors introduce a new actor in the current drama of the Hubble tension (conflicting measurements of ), namely the age of the Universe , as determined by the oldest globular clusters, and show that if local measurements are correct, the resolution of the Hubble tension implies a modification of the cosmological standard model CDM in the early and late Universe. Once systematic uncertainties are reduced, measuring will discriminate between the viable solutions for the tension, i.e. changing CDM or errors in the local measurements.
Mark Hindmarsh, Joanes Lizarraga, Asier Lopez-Eiguren, and Jon Urrestilla
Phys. Rev. D 103, 103534 (2021) - Published 26 May, 2021
Tassia Ferreira, Tianqing Zhang, Nianyi Chen, and Scott Dodelson (LSST Dark Energy Science Collaboration)
Phys. Rev. D 103, 103535 (2021) - Published 28 May, 2021
Yohei Ema, Ryusuke Jinno, Kazunori Nakayama, and Jorinde van de Vis
Phys. Rev. D 103, 103536 (2021) - Published 28 May, 2021
Florian Niedermann and Martin S. Sloth
Phys. Rev. D 103, 103537 (2021) - Published 28 May, 2021
Fiona McCarthy, Simon Foreman, and Alexander van Engelen
Phys. Rev. D 103, 103538 (2021) - Published 28 May, 2021
One of the serious hindrances to achieving a major goal of the next generation CMB experiments, the measurement of the sum of the neutrino masses, is the lack of sufficient knowledge of baryonic effects on the matter power spectrum. In this paper, the authors propose several mitigating strategies, which, they show, will serve to reduce these baryonic effects to a negligible level, without significantly increasing the associated statistical uncertainty.
Rubén Arjona and Savvas Nesseris
Phys. Rev. D 103, 103539 (2021) - Published 28 May, 2021
Md Riajul Haque, Debaprasad Maity, and Sourav Pal
Phys. Rev. D 103, 103540 (2021) - Published 28 May, 2021
H. García-Compeán, V. S. Manko, and C. J. Ramírez-Valdez
Phys. Rev. D 103, 104001 (2021) - Published 3 May, 2021
Suman Kulkarni and Collin D. Capano
Phys. Rev. D 103, 104002 (2021) - Published 3 May, 2021
Yotam Sherf
Phys. Rev. D 103, 104003 (2021) - Published 3 May, 2021
Eryk Buk and Jerzy Lewandowski
Phys. Rev. D 103, 104004 (2021) - Published 4 May, 2021
Yuan-Ling Zhao, Yu-Jie Tan, Wen-Hao Wu, Jie Luo, and Cheng-Gang Shao
Phys. Rev. D 103, 104005 (2021) - Published 4 May, 2021
Miren Radia, Ulrich Sperhake, Emanuele Berti, and Robin Croft
Phys. Rev. D 103, 104006 (2021) - Published 6 May, 2021
Guillermo Lara, Mario Herrero-Valea, Enrico Barausse, and Sergey M. Sibiryakov
Phys. Rev. D 103, 104007 (2021) - Published 6 May, 2021
João Magueijo and Tom Zlosnik
Phys. Rev. D 103, 104008 (2021) - Published 6 May, 2021
Chloe B. Richards, Thomas W. Baumgarte, and Stuart L. Shapiro
Phys. Rev. D 103, 104009 (2021) - Published 6 May, 2021
Alexandre Arbey, Jérémy Auffinger, Marc Geiller, Etera R. Livine, and Francesco Sartini
Phys. Rev. D 103, 104010 (2021) - Published 7 May, 2021
S. H. Hendi and Kh. Jafarzade
Phys. Rev. D 103, 104011 (2021) - Published 10 May, 2021
Peng Wang, Houwen Wu, and Haitang Yang
Phys. Rev. D 103, 104012 (2021) - Published 11 May, 2021
Fotios K. Anagnostopoulos, Spyros Basilakos, and Emmanuel N. Saridakis
Phys. Rev. D 103, 104013 (2021) - Published 10 May, 2021
Scott A. Hughes, Niels Warburton, Gaurav Khanna, Alvin J. K. Chua, and Michael L. Katz
Phys. Rev. D 103, 104014 (2021) - Published 11 May, 2021
Rafkat Galeev, Ruslan Muharlyamov, Alexei A. Starobinsky, Sergey V. Sushkov, and Mikhail S. Volkov
Phys. Rev. D 103, 104015 (2021) - Published 12 May, 2021
Yuri Bonder and Christian Peterson
Phys. Rev. D 103, 104016 (2021) - Published 12 May, 2021
Nicholas Loutrel, Justin L. Ripley, Elena Giorgi, and Frans Pretorius
Phys. Rev. D 103, 104017 (2021) - Published 18 May, 2021
Justin L. Ripley, Nicholas Loutrel, Elena Giorgi, and Frans Pretorius
Phys. Rev. D 103, 104018 (2021) - Published 18 May, 2021
Oleg Yu. Tsupko
Phys. Rev. D 103, 104019 (2021) - Published 13 May, 2021
Di Wu and Puxun Wu
Phys. Rev. D 103, 104020 (2021) - Published 13 May, 2021
Alessandro Nagar, Alice Bonino, and Piero Rettegno
Phys. Rev. D 103, 104021 (2021) - Published 13 May, 2021
Asanka Amarasinghe, Tianye Liu, Daniel A. Norman, and Philip D. Mannheim
Phys. Rev. D 103, 104022 (2021) - Published 14 May, 2021
Gustavo P. de Brito, Antonio D. Pereira, and Arthur F. Vieira
Phys. Rev. D 103, 104023 (2021) - Published 14 May, 2021
Mohammad Bagher Jahani Poshteh and Robert B. Mann
Phys. Rev. D 103, 104024 (2021) - Published 14 May, 2021
Alfio Bonanno, Georgios Kofinas, and Vasilios Zarikas
Phys. Rev. D 103, 104025 (2021) - Published 14 May, 2021
Shammi Tahura, David A. Nichols, Alexander Saffer, Leo C. Stein, and Kent Yagi
Phys. Rev. D 103, 104026 (2021) - Published 14 May, 2021
Tousif Islam, Scott E. Field, Carl-Johan Haster, and Rory Smith
Phys. Rev. D 103, 104027 (2021) - Published 14 May, 2021
Takahisa Igata, Kazunori Kohri, and Kota Ogasawara
Phys. Rev. D 103, 104028 (2021) - Published 14 May, 2021
Jorge F. M. Delgado, Carlos A. R. Herdeiro, and Eugen Radu
Phys. Rev. D 103, 104029 (2021) - Published 14 May, 2021
Anupam A. H., Aniket Khairnar, and Arpan Kundu
Phys. Rev. D 103, 104030 (2021) - Published 14 May, 2021
Minyong Guo and Sijie Gao
Phys. Rev. D 103, 104031 (2021) - Published 17 May, 2021
Sayak Datta and Sajal Mukherjee
Phys. Rev. D 103, 104032 (2021) - Published 17 May, 2021
R. A. Konoplya and A. Zhidenko
Phys. Rev. D 103, 104033 (2021) - Published 17 May, 2021
Edgardo Franzin, Stefano Liberati, and Mauro Oi
Phys. Rev. D 103, 104034 (2021) - Published 17 May, 2021
Martín Enríquez Rojo and Till Heckelbacher
Phys. Rev. D 103, 104035 (2021) - Published 17 May, 2021
Dimitrios Psaltis, Colm Talbot, Ethan Payne, and Ilya Mandel
Phys. Rev. D 103, 104036 (2021) - Published 18 May, 2021
Tomoya Tachinami, Shinpei Tonosaki, and Yuuiti Sendouda
Phys. Rev. D 103, 104037 (2021) - Published 17 May, 2021
Shahar Hadar, Michael D. Johnson, Alexandru Lupsasca, and George N. Wong
Phys. Rev. D 103, 104038 (2021) - Published 17 May, 2021
Keita Takizawa and Hideki Asada
Phys. Rev. D 103, 104039 (2021) - Published 18 May, 2021
Grigoris Panotopoulos, Ángel Rincón, and Ilídio Lopes
Phys. Rev. D 103, 104040 (2021) - Published 18 May, 2021
L. Asprea, G. Gasbarri, and A. Bassi
Phys. Rev. D 103, 104041 (2021) - Published 19 May, 2021
M. P. Hobson and A. N. Lasenby
Phys. Rev. D 103, 104042 (2021) - Published 19 May, 2021
Raimon Luna, Miguel Zilhão, Vitor Cardoso, João L. Costa, and José Natário
Phys. Rev. D 103, 104043 (2021) - Published 19 May, 2021
Vitor Cardoso, Francisco Duque, and Arianna Foschi
Phys. Rev. D 103, 104044 (2021) - Published 19 May, 2021
Viktor Skoupý and Georgios Lukes-Gerakopoulos
Phys. Rev. D 103, 104045 (2021) - Published 19 May, 2021
José P. S. Lemos and Paulo Luz
Phys. Rev. D 103, 104046 (2021) - Published 19 May, 2021
Prashant Kocherlakota et al. (EHT Collaboration)
Phys. Rev. D 103, 104047 (2021) - Published 20 May, 2021
Arnab Dhani
Phys. Rev. D 103, 104048 (2021) - Published 20 May, 2021
Barry Wardell and Chris Kavanagh
Phys. Rev. D 103, 104049 (2021) - Published 21 May, 2021
Shinta Kasuya and Masataka Kobayashi
Phys. Rev. D 103, 104050 (2021) - Published 21 May, 2021
Angel D. D. Masa, Enesson S. de Oliveira, and Vilson T. Zanchin
Phys. Rev. D 103, 104051 (2021) - Published 21 May, 2021
Séverine Rosat and Josipa Majstorović
Phys. Rev. D 103, 104052 (2021) - Published 24 May, 2021
Itamar J. Allali and Mark P. Hertzberg
Phys. Rev. D 103, 104053 (2021) - Published 24 May, 2021
Baoyi Chen, Qingwen Wang, and Yanbei Chen
Phys. Rev. D 103, 104054 (2021) - Published 25 May, 2021
Yijun Wang, Rico K. L. Lo, Alvin K. Y. Li, and Yanbei Chen
Phys. Rev. D 103, 104055 (2021) - Published 24 May, 2021
Geraint Pratten, Cecilio García-Quirós, Marta Colleoni, Antoni Ramos-Buades, Héctor Estellés, Maite Mateu-Lucena, Rafel Jaume, Maria Haney, David Keitel, Jonathan E. Thompson, and Sascha Husa
Phys. Rev. D 103, 104056 (2021) - Published 25 May, 2021
Neil J. Cornish
Phys. Rev. D 103, 104057 (2021) - Published 26 May, 2021
F. Gómez, S. Lepe, C. Quinzacara, and P. Salgado
Phys. Rev. D 103, 104058 (2021) - Published 26 May, 2021
Isabela S. Matos, Maurício O. Calvão, and Ioav Waga
Phys. Rev. D 103, 104059 (2021) - Published 26 May, 2021
Noemi Frusciante and Micol Benetti
Phys. Rev. D 103, 104060 (2021) - Published 26 May, 2021
Luciano Petruzziello and Fabian Wagner
Phys. Rev. D 103, 104061 (2021) - Published 28 May, 2021
Filip Ficek
Phys. Rev. D 103, 104062 (2021) - Published 28 May, 2021
Tien Hsieh, Da-Shin Lee, and Chi-Yong Lin
Phys. Rev. D 103, 104063 (2021) - Published 28 May, 2021
Matheus C. Teodoro, Lucas G. Collodel, and Jutta Kunz
Phys. Rev. D 103, 104064 (2021) - Published 28 May, 2021
Pedro G. S. Fernandes
Phys. Rev. D 103, 104065 (2021) - Published 28 May, 2021
Chao Zhang (张超), Yungui Gong (龚云贵), Bin Wang (王斌), and Chunyu Zhang (张春雨)
Phys. Rev. D 103, 104066 (2021) - Published 28 May, 2021
Camilo Posada, Jan Hladík, and Zdeněk Stuchlík
Phys. Rev. D 103, 104067 (2021) - Published 28 May, 2021
Nicole Rosato, James Healy, and Carlos O. Lousto
Phys. Rev. D 103, 104068 (2021) - Published 28 May, 2021
João Luís Rosa
Phys. Rev. D 103, 104069 (2021) - Published 28 May, 2021
Javlon Rayimbaev, Ahmadjon Abdujabbarov, and Wen-Biao Han
Phys. Rev. D 103, 104070 (2021) - Published 28 May, 2021
Kinjal Banerjee, Rudranil Basu, Aditya Mehra, Akhila Mohan, and Aditya Sharma
Phys. Rev. D 103, 105001 (2021) - Published 4 May, 2021
Pau Beltrán-Palau, Adrián del Río, Sergi Nadal-Gisbert, and José Navarro-Salas
Phys. Rev. D 103, 105002 (2021) - Published 4 May, 2021
Silvia Pla, Ian M. Newsome, Robert S. Link, Paul R. Anderson, and Jose Navarro-Salas
Phys. Rev. D 103, 105003 (2021) - Published 6 May, 2021
Ivan Kolář and Jens Boos
Phys. Rev. D 103, 105004 (2021) - Published 6 May, 2021
Tal Schwartzman and Benni Reznik
Phys. Rev. D 103, 105005 (2021) - Published 7 May, 2021
Hun Jang and Massimo Porrati
Phys. Rev. D 103, 105006 (2021) - Published 12 May, 2021
S. Katuwal, S. P. Miao, and R. P. Woodard
Phys. Rev. D 103, 105007 (2021) - Published 14 May, 2021
P. A. Anempodistov
Phys. Rev. D 103, 105008 (2021) - Published 14 May, 2021
Marzieh Akbari Ahmadmahmoudi and Ehsan Bavarsad
Phys. Rev. D 103, 105009 (2021) - Published 17 May, 2021
Satoshi Iso, Takato Mori, and Katsuta Sakai
Phys. Rev. D 103, 105010 (2021) - Published 17 May, 2021
Vladimir Toussaint and Jorma Louko
Phys. Rev. D 103, 105011 (2021) - Published 17 May, 2021
Aleksey Cherman and Theodore Jacobson
Phys. Rev. D 103, 105012 (2021) - Published 17 May, 2021
A. Ahmadain and I. Klich
Phys. Rev. D 103, 105013 (2021) - Published 18 May, 2021
Hapé Fuhri Snethlage and Sergio Hörtner
Phys. Rev. D 103, 105014 (2021) - Published 18 May, 2021
Luis Fernández, Van Sérgio Alves, M. Gomes, Leandro O. Nascimento, and Francisco Peña
Phys. Rev. D 103, 105016 (2021) - Published 19 May, 2021
W. N. Polyzou
Phys. Rev. D 103, 105017 (2021) - Published 19 May, 2021
Dirac showed that relativity implied three different forms of quantum mechanics (instant, point, and light-front) depending on how boosts and translation generators account for interactions. However, it is non-trivial to prove that these representations are equivalent in quantum field theory. Here, the author demonstrates using non-perturbative techniques that equivalent representations between instant-form and light-front dynamics can be constructed, based on assumptions of a local quantum field theory.
Domenico Orlando, Vito Pellizzani, and Susanne Reffert
Phys. Rev. D 103, 105018 (2021) - Published 19 May, 2021
Benjamin Knorr and Chris Ripken
Phys. Rev. D 103, 105019 (2021) - Published 20 May, 2021
Jean Alexandre and Janos Polonyi
Phys. Rev. D 103, 105020 (2021) - Published 20 May, 2021
O. Corradini, E. Latini, and Andrew Waldron
Phys. Rev. D 103, 105021 (2021) - Published 25 May, 2021
D. Glavan, S. P. Miao, T. Prokopec, and R. P. Woodard
Phys. Rev. D 103, 105022 (2021) - Published 27 May, 2021
Vivishek Sudhir, Nadine Stritzelberger, and Achim Kempf
Phys. Rev. D 103, 105023 (2021) - Published 26 May, 2021
Juven Wang
Phys. Rev. D 103, 105024 (2021) - Published 27 May, 2021
Benjamin Koch and Enrique Muñoz
Phys. Rev. D 103, 105025 (2021) - Published 28 May, 2021
Domenico Orlando, Susanne Reffert, and Francesco Sannino
Phys. Rev. D 103, 105026 (2021) - Published 28 May, 2021
Edoardo Vescovi
Phys. Rev. D 103, 106001 (2021) - Published 3 May, 2021
Antonio M. García-García, Yiyang Jia (贾抑扬), Dario Rosa, and Jacobus J. M. Verbaarschot
Phys. Rev. D 103, 106002 (2021) - Published 3 May, 2021
Gautam Sengupta and Vinay Malvimat
Phys. Rev. D 103, 106003 (2021) - Published 4 May, 2021
Luis Inzunza and Mikhail S. Plyushchay
Phys. Rev. D 103, 106004 (2021) - Published 4 May, 2021
Raphael Bousso and Arvin Shahbazi-Moghaddam
Phys. Rev. D 103, 106005 (2021) - Published 4 May, 2021
Jose J. Blanco-Pillado, Kepa Sousa, Mikel A. Urkiola, and Jeremy M. Wachter
Phys. Rev. D 103, 106006 (2021) - Published 4 May, 2021
Masanori Hanada
Phys. Rev. D 103, 106007 (2021) - Published 6 May, 2021
Karthik Rajeev, Vikramaditya Mondal, and Sumanta Chakraborty
Phys. Rev. D 103, 106008 (2021) - Published 7 May, 2021
Nejc Čeplak and David Vegh
Phys. Rev. D 103, 106009 (2021) - Published 10 May, 2021
Refik Mansuroglu and Hanno Sahlmann
Phys. Rev. D 103, 106010 (2021) - Published 10 May, 2021
Sera Cremonini, Callum R. T. Jones, James T. Liu, Brian McPeak, and Yuezhang Tang
Phys. Rev. D 103, 106011 (2021) - Published 11 May, 2021
David Jorrin and Martin Schvellinger
Phys. Rev. D 103, 106012 (2021) - Published 11 May, 2021
O. Valba and A. Gorsky
Phys. Rev. D 103, 106013 (2021) - Published 11 May, 2021
Fabio D’Ambrosio, Marios Christodoulou, Pierre Martin-Dussaud, Carlo Rovelli, and Farshid Soltani
Phys. Rev. D 103, 106014 (2021) - Published 11 May, 2021
Michele Arzano, Andrea Bevilacqua, Jerzy Kowalski-Glikman, Giacomo Rosati, and Josua Unger
Phys. Rev. D 103, 106015 (2021) - Published 12 May, 2021
Yu Hamada, Jan M. Pawlowski, and Masatoshi Yamada
Phys. Rev. D 103, 106016 (2021) - Published 14 May, 2021
Yufan Wang and Yiwen Pan
Phys. Rev. D 103, 106017 (2021) - Published 14 May, 2021
Daniel Elander, Maurizio Piai, and John Roughley
Phys. Rev. D 103, 106018 (2021) - Published 18 May, 2021
M. Hameeda, B. Pourhassan, M. C. Rocca, and Aram Bahroz Brzo
Phys. Rev. D 103, 106019 (2021) - Published 21 May, 2021
G. Modanese
Phys. Rev. D 103, 106020 (2021) - Published 19 May, 2021
Roberto Auzzi, Stefano Baiguera, G. Bruno De Luca, Andrea Legramandi, Giuseppe Nardelli, and Nicolò Zenoni
Phys. Rev. D 103, 106021 (2021) - Published 19 May, 2021
Tom Banks, Patrick Draper, and Szilard Farkas
Phys. Rev. D 103, 106022 (2021) - Published 21 May, 2021
Antonio M. García-García, Jie Ping Zheng (郑杰平), and Vaios Ziogas
Phys. Rev. D 103, 106023 (2021) - Published 24 May, 2021
Roberto Ruiz
Phys. Rev. D 103, 106024 (2021) - Published 26 May, 2021
Iarley P. Lobo and Christian Pfeifer
Phys. Rev. D 103, 106025 (2021) - Published 28 May, 2021
Justin Kaidi
Phys. Rev. D 103, 106026 (2021) - Published 28 May, 2021
R. da Rocha
Phys. Rev. D 103, 106027 (2021) - Published 28 May, 2021
Anthony Ashmore and Fabian Ruehle
Phys. Rev. D 103, 106028 (2021) - Published 28 May, 2021
Yannick Dengler, Jürgen Schaffner-Bielich, and Laura Tolos
Phys. Rev. D 103, 109901 (2021) - Published 20 May, 2021