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Magnetic fields in galaxies and galaxy clusters are believed to be the result of the amplification of intergalactic seed fields during the formation of large-scale structures in the universe. However, the origin, strength, and morphology of…

High Energy Astrophysical Phenomena · Physics 2023-06-22 H. E. S. S. , Fermi-LAT Collaborations , : , F. Aharonian , J. Aschersleben , M. Backes , V. Barbosa Martins , R. Batzofin , Y. Becherini , D. Berge , B. Bi , M. Bouyahiaoui , M. Breuhaus , R. Brose , F. Brun , B. Bruno , T. Bulik , C. Burger-Scheidlin , T. Bylund , S. Caroff , S. Casanova , J. Celic , M. Cerruti , T. Chand , S. Chandra , A. Chen , J. Chibueze , O. Chibueze , G. Cotter , M. de Bony , K. Egberts , J. -P. Ernenwein , G. Fichet de Clairfontaine , M. Filipovic , G. Fontaine , M. Füßling , S. Funk , S. Gabici , S. Ghafourizadeh , G. Giavitto , D. Glawion , J. F. Glicenstein , P. Goswami , M. -H. Grondin , L. Haerer , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , F. Jankowsky , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzynński , R. Khatoon , B. Khélifi , W. Kluźniak , Nu. Komin , K. Kosack , D. Kostunin , R. G. Lang , S. Le Stum , F. Leitl , A. Lemière , J. -P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , D. Malyshev , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Martí-Devesa , R. Marx , M. Meyer , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , J. Muller , T. Murach , K. Nakashima , J. Niemiec , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , S. Panny , M. Panter , R. D. Parsons , G. Peron , D. A. Prokhorov , H. Prokoph , G. Pühlhofer , M. Punch , A. Quirrenbach , P. Reichherzer , A. Reimer , O. Reimer , B. Reville , F. Rieger , G. Rowell , B. Rudak , E. Ruiz-Velasco , V. Sahakian , D. A. Sanchez , M. Sasaki , F. Schüussler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , H. Sol , S. Spencer , S. Steinmassl , H. Suzuki , T. Takahashi , T. Tanaka , A. M. Taylor , R. Terrier , C. Thorpe-Morgan , M. Tsirou , N. Tsuji , Y. Uchiyama , C. van Eldik , J. Veh , C. Venter , S. J. Wagner , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , S. Zouari , N. Zywucka

Non-abelian gauge theories may have a ferromagnet-like vacuum with a non-zero magnetic field, which also exists at finite temperature. We argue that the formation of the ferromagnet-like vacuum at GUT scales gives rise to a Maxwell magnetic…

High Energy Physics - Phenomenology · Physics 2010-11-30 Kari Enqvist , Poul Olesen

An interesting strategy for indirect detection of Dark Matter comes through the amounts of electrons and positrons usually emitted by DM pair annihilation. The e+e- gyrating in the galactic magnetic field then produce secondary synchrotron…

Astrophysics · Physics 2010-01-08 Enrico Borriello , Alessandro Cuoco , Gennaro Miele

We study the effect of variations of the electromagnetic coupling on the process of generation of primordial magnetic fields. We find that only through a significant growth of the electromagnetic coupling minimum seed fields can be…

Astrophysics · Physics 2009-03-24 O. Bertolami , R. Monteiro

The puzzle of ultra-high energy cosmic rays (UHECRs) still remains unresolved. With the progress in preparation of next generation experiments (AUGER, EUSO, OWL) grows also the importance of directional analysis of existing and future…

Astrophysics · Physics 2009-11-10 Michael Prouza , Radomir Smida

Magnetic fields on a range of scales play a large role in the ecosystems of galaxies, both in the galactic disk and in the extended layers of gas away from the plane. Observing magnetic field strength, structure and orientation is complex,…

Astrophysics of Galaxies · Physics 2015-05-27 Marijke Haverkorn , Volker Heesen

A new $U(1)$ dark gauge group coupled to the Standard Model (SM) via the kinetic mixing portal provides a natural dark matter candidate in the form of the Higgs field, $h_d$, responsible for generating the mass of the dark photon,…

High Energy Physics - Phenomenology · Physics 2021-03-03 Cristina Mondino , Maxim Pospelov , Joshua T. Ruderman , Oren Slone

We demonstrate that the Biermann battery mechanism for the creation of large scale magnetic fields can arise in a simple model protogalaxy. Analytic calculations and numerical simulations follow explicitly the generation of vorticity (and…

Astrophysics · Physics 2007-05-23 George Davies , Lawrence M. Widrow

Strong magnetic fields in magnetospheres of neutron stars (especially magnetars) and other astrophysical objects may release their energy in violent, intense episodes of magnetic reconnection. While reconnection has been studied…

High Energy Astrophysical Phenomena · Physics 2019-01-16 K. M. Schoeffler , T. Grismayer , D. Uzdensky , R. A. Fonseca , L. O. Silva

Primordial magnetic fields in the dark sector can be transferred to magnetic fields in the visible sector due to a gauge kinetic mixing term. We show that the transfer occurs when the evolution of magnetic fields is dominated by dissipation…

High Energy Physics - Phenomenology · Physics 2018-08-08 Kohei Kamada , Yuhsin Tsai , Tanmay Vachaspati

We derive the minimal seed magnetic field which unavoidably arises in the radiation and matter eras, prior to recombination, by the rotational velocity of ions and electrons, gravitationally induced by the non-linear evolution of primordial…

Astrophysics · Physics 2009-11-10 S. Matarrese , S. Mollerach , A. Notari , A. Riotto

The magnetic field within a few hundred parsecs of the center of the Galaxy is an essential component of any description of that region. The field has several pronounced observational manifestations: 1) morphological structures such as…

Astrophysics · Physics 2007-05-23 Mark Morris

We consider a broad class of interactions between radiation and a light scalar field, including both conformal and disformal couplings. Such a scalar field potentially acts on cosmological scales as dark energy and could also appear in…

High Energy Astrophysical Phenomena · Physics 2015-10-07 Philippe Brax , Pierre Brun , Denis Wouters

Molecular magnets, although analogous to familiar macroscopic magnets, offer a platform for next generation magnetic storage technologies with far higher data densities and prospective applications in quantum information science. When…

High Energy Physics - Phenomenology · Physics 2026-01-06 Jose R. Alves , Manfred Lindner , Farinaldo S. Queiroz , Manoel S. Vasconcelos

Dark photons, a generic class of light gauge bosons that interact with the Standard Model (SM) exclusively through kinetic mixing, arise naturally in many gauge extensions of the SM. Motivated by these theoretical considerations, we present…

High Energy Physics - Phenomenology · Physics 2025-12-10 Xun-Jie Xu , Boting Zhou

In this Letter, we motivate the fact that couplings between a scalar field and the Standard Model with strengths $10^{-6}(m_\phi/{\rm eV})^{-1/4}$ relative to gravity yield the total measured cosmological dark matter abundance over a broad…

High Energy Physics - Phenomenology · Physics 2025-09-19 David Cyncynates , Olivier Simon

Dynamical extra dimensions break the conformal invariance of Maxwell's equations in four dimensions. A higher dimensional background with $n$ contracting extra dimensions and four expanding dimensions is matched to an effectively four…

High Energy Physics - Phenomenology · Physics 2010-04-05 Kerstin E. Kunze

Dark photon dark matter that has a kinetic mixing with the Standard Model photon can resonantly convert in environments where its mass $m_{A'}$ coincides with the plasma frequency. We show that such conversion in neutron stars or accreting…

High Energy Physics - Phenomenology · Physics 2023-09-14 Edward Hardy , Ningqiang Song

Damping of an electromagnetic wave in a strong magnetic field is analyzed in the kinematic region near the threshold of electron-positron pair production. Damping of the electromagnetic field is shown to be noticeably nonexponential in this…

High Energy Physics - Phenomenology · Physics 2010-11-15 N. V. Mikheev , M. V. Chistyakov

Aims. We investigate the cosmological evolution of large- and small-scale magnetic fields in galaxies in the light of present models of formation and evolution of galaxies. Methods. We use the dynamo theory to derive the timescales of…

Astrophysics · Physics 2009-11-13 Tigran G. Arshakian , Rainer Beck , Marita Krause , Dmitry Sokoloff
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