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Core-collapse supernovae are the terminal explosions of massive stars. After successive phases of nuclear fusion proceeding up to silicon burning, these stars form an iron core that is supported by electron degeneracy pressure. The core…

High Energy Astrophysical Phenomena · Physics 2026-05-27 B. Mueller , B. Sykes

The shape of the neutrino pulse from the supernova SN1987a provides one of the most stringent constraints on the size of large, compact, "gravity-only" extra dimensions. Previously, calculations have been carried out for a newly-born…

Nuclear Theory · Physics 2009-11-07 Daniel Arndt

We derive supernova (SN) bounds on muon-philic bosons, taking advantage of the recent emergence of muonic SN models. Our main innovations are to consider scalars $\phi$ in addition to pseudoscalars $a$ and to include systematically the…

High Energy Physics - Phenomenology · Physics 2026-04-06 Andrea Caputo , Georg Raffelt , Edoardo Vitagliano

Recent observations suggest that gamma ray bursts (GRBs) and their afterglows are produced by highly relativistic jets emitted in core collapse supernova explosions (SNe). The result of the event, probably, is not just a compact object plus…

Astrophysics · Physics 2009-11-06 Arnon Dar

Observations from the last decade have indicated the existence of a general class of superluminous supernovae (SLSNe), in which the peak luminosity exceeds 10^{44} erg/s. Here we focus on a subclass of these events, where the light curve is…

Solar and Stellar Astrophysics · Physics 2015-06-05 Sivan Ginzburg , Shmuel Balberg

Heavy sterile neutrinos with masses ${\mathcal O}(100)$ MeV mixing with active neutrinos can be produced in the core of a collapsing supernova (SN). In order to avoid an excessive energy loss, shortening the observed duration of the SN…

High Energy Physics - Phenomenology · Physics 2020-01-07 Leonardo Mastrototaro , Alessandro Mirizzi , Pasquale Dario Serpico , Arman Esmaili

We present new constraints on sub-GeV dark matter and dark photons from the electron beam-dump experiment E137 conducted at SLAC in 1980-1982. Dark matter interacting with electrons (e.g., via a dark photon) could have been produced in the…

High Energy Physics - Phenomenology · Physics 2015-10-09 Brian Batell , Rouven Essig , Ze'ev Surujon

A supernova event in our own galaxy will result in a large number of neutrinos detected on Earth within the time-frame of a few seconds. These neutrinos will have been produced thermally with, in principle, three distinct temperatures for…

High Energy Physics - Phenomenology · Physics 2016-05-04 Jonathan H. Davis

We calculate the production of ultra-light axion-like particles (ALPs) in a nearby supernova progenitor. Once produced, ALPs escape from the star and a part of them is converted into photons during propagation in the Galactic magnetic…

High Energy Physics - Phenomenology · Physics 2022-02-02 Kanji Mori , Tomoya Takiwaki , Kei Kotake

We investigate in this paper the core-collapse supernova explosion mechanism in both one and two dimensions. We verify the usefulness of neutrino-driven overturn (``convection'') between the shock and the neutrinosphere in igniting the…

Astrophysics · Physics 2009-10-28 Adam Burrows , John Hayes , Bruce Fryxell

The EDGES Collaboration has recently reported the detection of a stronger-than-expected absorption feature in the global 21-cm spectrum, centered at a frequency corresponding to a redshift of z ~ 17. This observation has been interpreted as…

High Energy Physics - Phenomenology · Physics 2018-07-11 Asher Berlin , Dan Hooper , Gordan Krnjaic , Samuel D. McDermott

We analyze the confining effect of cloud collapse on an expanding supernova shockfront. We solve the differential equation for the forces on the shockfront due to ram pressure, supernova energy, and gravity. We find that the expansion of…

Astrophysics · Physics 2009-11-11 M. M. Kasliwal , R. V. E. Lovelace , J. R. Houck

The interaction of a supernova with a circumstellar medium (CSM) can dramatically increase the emitted luminosity by converting kinetic energy to thermal energy. In 'superluminous' supernovae (SLSNe) of Type IIn -- named for narrow hydrogen…

Constraints on couplings of several Beyond Standard Model Physics scenarios, mediated by massive intermediate particles including (1) Extra Z-prime, (2) New Light Spin-1 Boson, and (3) Charged Higgs Boson, are placed via neutrino-electron…

High Energy Physics - Phenomenology · Physics 2018-03-28 B. Sevda , A. Şen , M. Demirci , M. Deniz , M. Agartioglu , A. Ajjaq , S. Kerman , L. Singh , A. Sonay , H. T. Wong , M. Zeyrek

We derive a simple approximate model describing the early, hours to days, UV/optical supernova emission, which is produced by the expansion of the outer <~0.01 solar mass part of the shock-heated envelope, and precedes the optical emission…

High Energy Astrophysical Phenomena · Physics 2015-03-13 Itay Rabinak , Eli Waxman

Dark photon is a new gauge boson beyond the Standard Model as a kind of dark matter (DM) candidate. Dark photon dark matter (DPDM) interacts with electromagnetic fields via kinetic mixing, implicating an approach to give a constraint with…

High Energy Astrophysical Phenomena · Physics 2024-07-24 Tian-Ci Liu , Ming-Xuan Lu , Xiao-Song Hu

In light of the latest IceCube data, we discuss the implications of the cosmic ray energy input from hypernovae and supernovae into the Universe, and their propagation in the hosting galaxy and galaxy clusters or groups. The magnetic…

High Energy Astrophysical Phenomena · Physics 2015-06-09 Nicholas Senno , Peter Mészáros , Kohta Murase , Philipp Baerwald , Martin J. Rees

We show how the spectrum of the minimal anomaly-mediated supersymmetry breaking model can be constrained from the condition that the electroweak symmetry breaking minimum of the scalar potential is the deepest point in the field space.…

High Energy Physics - Phenomenology · Physics 2009-11-07 Amitava Datta , Anirban Kundu , Abhijit Samanta

We revisit the limit on very light axion-like particles (ALPs) from the absence of gamma rays coincidental with the neutrino burst from SN1987A. We use updated supernova simulations, modern models for the magnetic field inside the Galaxy,…

High Energy Astrophysical Phenomena · Physics 2014-10-17 Alexandre Payez