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Axion-like particles (ALPs) can couple to photons in strong magnetic fields, producing characteristic fluctuations in X-ray spectra. Using data from NASA's Neutron Star Interior Composition Explorer (NICER), we analyzed three pulsars: PSR…

High Energy Astrophysical Phenomena · Physics 2026-02-10 Yen-Jhen Liu , Yi Yang

The Pseudo-Goldstone Boson (PGB) emission could provide a very efficient mechanism for explaining the cosmic Gamma Ray Bursts (GRBs). The PGBs could be produced during the merging of two compact objects like two neutron stars or neutron…

High Energy Physics - Phenomenology · Physics 2009-10-31 Zurab Berezhiani , Alessandro Drago

We use multimessenger observations of the neutron star merger event GW170817 to derive new constraints on axion-like particles (ALPs) coupling to photons. ALPs are produced via Primakoff and photon coalescence processes in the merger,…

High Energy Physics - Phenomenology · Physics 2025-11-24 P. S. Bhupal Dev , Jean-François Fortin , Steven P. Harris , Kuver Sinha , Yongchao Zhang

Gamma-rays from cosmological sources contain information about gamma-ray interactions. Standard model and non-standard model photon interactions along the path between the source and the observer can lead to changes in the energy or state…

High Energy Astrophysical Phenomena · Physics 2014-08-19 Rebecca Reesman , T. P. Walker

Recently it has been pointed out that a cosmic background of relativistic axion-like particles (ALPs) would be produced by the primordial decays of heavy fields in the post-inflation epoch, contributing to the extra-radiation content in the…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-25 Carmelo Evoli , Matteo Leo , Alessandro Mirizzi , Daniele Montanino

Proto-neutron stars formed during core-collapse supernovae are hot and dense environments that contain a sizable population of muons. If these interact with new long-lived particles with masses up to roughly 100 MeV, the latter can be…

High Energy Physics - Phenomenology · Physics 2025-06-19 Claudio Andrea Manzari , Jorge Martin Camalich , Jonas Spinner , Robert Ziegler

The growing interest in axion-like particles (ALPs) stems from the fact that they provide successful theoretical explanations of physics phenomena, from the anomaly of the CP-symmetry conservation in strong interactions to the observation…

High Energy Astrophysical Phenomena · Physics 2021-06-08 Ivana Batković , Alessandro De Angelis , Michele Doro , Marina Manganaro

We present a search for the direct production of a light pseudoscalar $a$ decaying into two photons with the Belle II detector at the SuperKEKB collider. We search for the process ${e^+e^-\to\gamma a, a \to\gamma\gamma}$ in the mass range…

High Energy Physics - Experiment · Physics 2020-10-21 Belle II collaboration , F. Abudinen , I. Adachi , H. Aihara , N. Akopov , A. Aloisio , F. Ameli , N. Anh Ky , D. M. Asner , T. Aushev , V. Aushev , V. Babu , S. Baehr , S. Bahinipati , P. Bambade , Sw. Banerjee , S. Bansal , J. Baudot , J. Becker , P. K. Behera , J. V. Bennett , E. Bernieri , F. U. Bernlochner , M. Bertemes , M. Bessner , S. Bettarini , V. Bhardwaj , F. Bianchi , T. Bilka , S. Bilokin , D. Biswas , M. Bračko , P. Branchini , N. Braun , T. E. Browder , A. Budano , S. Bussino , M. Campajola , G. Casarosa , C. Cecchi , D. Červenkov , M. -C. Chang , P. Chang , R. Cheaib , V. Chekelian , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , D. Cinabro , L. Corona , L. M. Cremaldi , S. Cunliffe , N. Dash , F. Dattola , E. De La Cruz-Burelo , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , M. Destefanis , A. De Yta-Hernandez , F. Di Capua , Z. Doležal , T. V. Dong , K. Dort , D. Dossett , G. Dujany , S. Eidelman , T. Ferber , D. Ferlewicz , S. Fiore , A. Fodor , F. Forti , B. G. Fulsom , E. Ganiev , R. Garg , A. Garmash , V. Gaur , A. Gaz , U. Gebauer , A. Gellrich , T. Geßler , R. Giordano , A. Giri , B. Gobbo , R. Godang , P. Goldenzweig , B. Golob , P. Gomis , W. Gradl , E. Graziani , D. Greenwald , C. Hadjivasiliou , S. Halder , O. Hartbrich , K. Hayasaka , H. Hayashii , C. Hearty , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , H. Hirata , M. Hoek , M. Hohmann , C. -L. Hsu , Y. Hu , K. Inami , G. Inguglia , J. Irakkathil Jabbar , A. Ishikawa , R. Itoh , P. Jackson , W. W. Jacobs , D. E. Jaffe , E. -J. Jang , S. Jia , Y. Jin , C. Joo , A. B. Kaliyar , J. Kandra , G. Karyan , Y. Kato , H. Kichimi , C. Kiesling , C. -H. Kim , D. Y. Kim , H. J. Kim , S. -H. Kim , Y. -K. Kim , T. D. Kimmel , K. Kinoshita , C. Kleinwort , P. Kodyš , T. Koga , S. Kohani , I. Komarov , S. Korpar , T. M. G. Kraetzschmar , P. Križan , P. Krokovny , T. Kuhr , M. Kumar , R. Kumar , K. Kumara , S. Kurz , Y. -J. Kwon , S. Lacaprara , C. La Licata , L. Lanceri , J. S. Lange , I. -S. Lee , S. C. Lee , P. Leitl , D. Levit , P. M. Lewis , C. Li , L. K. Li , Y. B. Li , J. Libby , K. Lieret , L. Li Gioi , Z. Liptak , Q. Y. Liu , D. Liventsev , S. Longo , T. Luo , C. MacQueen , Y. Maeda , R. Manfredi , E. Manoni , S. Marcello , C. Marinas , A. Martini , M. Masuda , K. Matsuoka , D. Matvienko , F. Meggendorfer , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , R. Mizuk , K. Azmi , G. B. Mohanty , H. -G. Moser , M. Mrvar , F. J. Müller , R. Mussa , I. Nakamura , M. Nakao , H. Nakazawa , A. Natochii , C. Niebuhr , N. K. Nisar , S. Nishida , M. H. A. Nouxman , K. Ogawa , S. Ogawa , H. Ono , P. Oskin , H. Ozaki , P. Pakhlov , A. Paladino , A. Panta , E. Paoloni , S. Pardi , H. Park , S. -H. Park , B. Paschen , A. Passeri , A. Pathak , S. Patra , S. Paul , T. K. Pedlar , I. Peruzzi , R. Peschke , M. Piccolo , L. E. Piilonen , G. Polat , V. Popov , C. Praz , E. Prencipe , M. T. Prim , M. V. Purohit , N. Rad , P. Rados , R. Rasheed , M. Reif , S. Reiter , M. Remnev , I. Ripp-Baudot , M. Ritter , M. Ritzert , G. Rizzo , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , C. Rosenfeld , A. Rostomyan , N. Rout , D. Sahoo , Y. Sakai , D. A. Sanders , S. Sandilya , A. Sangal , L. Santelj , Y. Sato , V. Savinov , B. Scavino , C. Schwanda , A. J. Schwartz , R. M. Seddon , Y. Seino , A. Selce , K. Senyo , J. Serrano , M. E. Sevior , C. Sfienti , J. -G. Shiu , A. Sibidanov , F. Simon , R. J. Sobie , A. Soffer , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , J. Strube , M. Sumihama , T. Sumiyoshi , D. J. Summers , W. Sutcliffe , H. Svidras , M. Tabata , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , P. Taras , F. Tenchini , D. Tonelli , E. Torassa , K. Trabelsi , M. Uchida , T. Uglov , K. Unger , Y. Unno , S. Uno , P. Urquijo , Y. Ushiroda , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , E. Waheed , M. Wakai , H. M. Wakeling , C. H. Wang , M. -Z. Wang , X. L. Wang , A. Warburton , M. Watanabe , S. Watanuki , J. Webb , S. Wehle , M. Welsch , C. Wessel , J. Wiechczynski , H. Windel , E. Won , L. J. Wu , X. P. Xu , B. Yabsley , W. Yan , S. B. Yang , H. Ye , M. Yonenaga , C. Z. Yuan , Y. Yusa , L. Zani , Q. D. Zhou , V. I. Zhukova

Axion-like particles (ALPs), a class of pseudoscalars common to many extensions of the Standard Model, have the capacity to drain energy from the interiors of stars. Consequently, stellar evolution can be used to derive many constraints on…

High Energy Physics - Phenomenology · Physics 2021-09-16 Matthew J. Dolan , Frederick J. Hiskens , Raymond R. Volkas

Future gamma-ray experiments, such as the e-ASTROGAM and AMEGO telescopes, can detect the Hawking radiation of photons from primordial black holes (PBHs) if they make up a fraction or all of dark matter. PBHs can analogously also Hawking…

High Energy Physics - Phenomenology · Physics 2025-08-08 Kaustubh Agashe , Jae Hyeok Chang , Steven J. Clark , Bhaskar Dutta , Yuhsin Tsai , Tao Xu

Axion-like particles (ALPs) can provide a portal to new states of a dark sector. We study the phenomenology of this portal when the ALP mainly decays invisibly, while its interaction with the standard model sector proceeds essentially via…

High Energy Physics - Phenomenology · Physics 2021-06-16 Luc Darmé , Federica Giacchino , Enrico Nardi , Mauro Raggi

We propose a three-beam stimulated resonant photon collider with focused laser fields in order to directly produce an axion-like particle (ALP) with the two beams and to stimulate its decay by the remaining one. The expected sensitivity…

High Energy Physics - Phenomenology · Physics 2023-01-05 Kensuke Homma , Fumiya Ishibashi , Yuri Kirita , Takumi Hasada

Axion-like particles (ALPs), hypothetical extensions of the Standard Model, can convert into photons in an external magnetic field. Two recent studies~\cite{Todarello:2023ptf, Ruz:2024gkl} explored the phenomenology of ALP-photon conversion…

High Energy Physics - Phenomenology · Physics 2025-01-28 Elisa Todarello

Dark Matter (DM) may be comprised of axion-like particles (ALPs) with couplings to photons and the standard model fermions. In this paper we study photon signals arising from cosmic ray (CR) electron scattering on background ALPs. For a…

High Energy Physics - Phenomenology · Physics 2021-10-04 James B. Dent , Bhaskar Dutta , Jayden L. Newstead , Alejandro Rodriguez , Ian M. Shoemaker , Zahra Tabrizi , Natalia Tapia Arellano

New light particles produced in supernovae can lead to additional energy loss and a consequent deficit in neutrino production in conflict with the neutrinos observed from Supernova 1987A (SN1987A). Contrary to the majority of previous…

High Energy Physics - Phenomenology · Physics 2021-02-03 Djuna Croon , Gilly Elor , Rebecca K. Leane , Samuel D. McDermott

We show that interactions of fast particles with the boundary shell of the local hot bubble could make an important contribution to the 0.5-1 keV diffuse X-ray background observed with ROSAT. The bulk of these nonthermal X-rays are due to…

Astrophysics · Physics 2009-10-30 V. Tatischeff , R. Ramaty

One interpretation of the unexplained signature observed in the PVLAS experiment invokes a new axion-like particle (ALP) with a two-photon vertex, allowing for photon-ALP oscillations in the presence of magnetic fields. In the range of…

Astrophysics · Physics 2008-11-26 Alessandro Mirizzi , Georg G. Raffelt , Pasquale D. Serpico

Axion-like particles (ALPs) are well-motivated examples of light, weakly coupled particles in theories beyond the Standard Model. In this work, we study long-lived ALPs coupled exclusively to leptons in the mass range between $2 m_e$ and…

High Energy Physics - Phenomenology · Physics 2025-07-22 Yohei Ema , Patrick J. Fox , Matheus Hostert , Tony Menzo , Maxim Pospelov , Anupam Ray , Jure Zupan

Galaxy clusters can efficiently convert axion-like particles (ALPs) to photons. We propose that the recently claimed detection of a 3.55--3.57 keV line in the stacked spectra of a large number of galaxy clusters and the Andromeda galaxy may…

High Energy Physics - Phenomenology · Physics 2014-07-30 Michele Cicoli , Joseph P. Conlon , M. C. David Marsh , Markus Rummel

Axion-like particles (ALPs) coupled to nucleons can be efficiently produced in the interior of protoneutron stars (PNS) during supernova (SN) explosions. If these ALPs are also coupled to photons they can convert into gamma rays in the…