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The hypothetical massive dark photon ($\gamma'$) which has kinetic mixing with the SM photon can decay electromagnetically to $e^+e^-$ pairs if its mass $m$ exceeds $2m_e$ and otherwise into three SM photons. These decays yield cosmological…

高能物理 - 唯象学 · 物理学 2014-11-21 Demos Kazanas , Rabindra N. Mohapatra , Shmuel Nussinov , Vigdor L. Teplitz , Yongchao Zhang

Dark photons, hypothetical feebly interacting massive vector bosons, appear in many extensions of the Standard Model. This study investigates their production and subsequent decay during supernova explosions. We demonstrate that the decay…

高能物理 - 唯象学 · 物理学 2024-05-01 Vsevolod Syvolap , Oleg Ruchayskiy

We revisit constraints on dark photons with masses below ~ 100 MeV from the observations of Supernova 1987A. If dark photons are produced in sufficient quantity, they reduce the amount of energy emitted in the form of neutrinos, in conflict…

高能物理 - 唯象学 · 物理学 2019-06-04 Jae Hyeok Chang , Rouven Essig , Samuel D. McDermott

We consider indirect detection signals of atomic dark matter, with a massive dark photon which mixes kinetically with hypercharge. In significant regions of parameter space, dark matter remains at least partially ionized today, and dark…

高能物理 - 唯象学 · 物理学 2015-04-29 Lauren Pearce , Kalliopi Petraki , Alexander Kusenko

Dark matter direct detection experiments have poor sensitivity to a galactic population of dark matter with mass below the GeV scale. However, such dark matter can be produced copiously in supernovae. Since this thermally-produced…

高能物理 - 唯象学 · 物理学 2019-10-17 William DeRocco , Peter W. Graham , Daniel Kasen , Gustavo Marques-Tavares , Surjeet Rajendran

A number of signals involving charged cosmic rays and high-energy photons have been interpreted as being due to annihilating dark matter. This article provides an overview of the experimental evidence and discusses in particular detections…

天体物理学 · 物理学 2007-05-23 U. Schwanke

We investigate cosmological and astrophysical constraints on dark photons with masses $\sim 10^{-1}$-$10^3$ MeV. These dark photons can be copiously produced either in the early universe or during core-collapse supernovae, potentially…

高能物理 - 唯象学 · 物理学 2025-11-21 Andrea Caputo , Jaeyoung Park , Seokhoon Yun

In this letter we begin the study of visible dark sector signals coming from binary neutron star mergers. We focus on dark photons emitted in the 10 ms - 1 s after the merger, and show how they can lead to bright transient gamma-ray…

高能物理 - 唯象学 · 物理学 2022-10-19 Melissa D. Diamond , Gustavo Marques-Tavares

The dark photon is a new gauge boson whose existence has been conjectured. It is dark because it arises from a symmetry of a hypothetical dark sector comprising particles completely neutral under the Standard Model interactions. Dark though…

高能物理 - 唯象学 · 物理学 2021-03-02 Marco Fabbrichesi , Emidio Gabrielli , Gaia Lanfranchi

Ultralight dark photons are compelling dark matter candidates, but their allowed kinetic mixing with the Standard Model photon is severely constrained by requiring that the dark photons do not collapse into a cosmic string network in the…

高能物理 - 唯象学 · 物理学 2025-08-20 David Cyncynates , Zachary J. Weiner

Feebly interacting particles with masses with O(10-100) MeV can be copiously produced by core-collapse supernovae (SNe). In this paper we consider the case of MeV-ish sterile neutrinos and dark photons mixed with ordinary neutrinos and…

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…

高能物理 - 唯象学 · 物理学 2025-12-10 Xun-Jie Xu , Boting Zhou

High energy gamma-rays and neutrinos can be produced both by the annihilation and by the possible slow decay of dark matter particles. We discuss the fluxes and spectra of such secondaries produced by dark matter particles in the universe…

天体物理学 · 物理学 2009-10-28 F. W. Stecker

"Dark Photons", light new vector particles V kinetically mixed with the photon, are a frequently considered extension of the Standard Model. For masses below 10 keV they are emitted from the solar interior. In the limit of small mass m_V…

高能物理 - 唯象学 · 物理学 2013-09-26 Haipeng An , Maxim Pospelov , Josef Pradler

The existence of a new, photon-like, massive particle, the gamma' or dark photon, is postulated in several extensions of the Standard Model. These models are often advocated to explain some recent puzzling astrophysical observations, as…

高能物理 - 实验 · 物理学 2014-02-03 Fabio Bossi

We discuss the possibility that the recent detection of 511 keV gamma rays from the galactic bulge, as observed by INTEGRAL, can be naturally explained by the supermassive very dense droplets (strangelets) of dark matter. These droplets are…

高能物理 - 唯象学 · 物理学 2009-11-10 David H. Oaknin , Ariel R. Zhitnitsky

It is entirely possible that our Universe is filled with dark radiation, such as SM neutrinos or new physics states, that are sourced by the decay of dark matter with cosmologically long lifetime. If non-thermal neutrinos produced such way…

高能物理 - 唯象学 · 物理学 2018-12-24 Josef Pradler

Dark matter annihilation into photons in our galaxy would constitute an exciting indirect signal of its existence, as underscored by tentative evidence for 130 GeV dark matter in Fermi/LAT data. Models that give a large annihilation cross…

高能物理 - 唯象学 · 物理学 2013-11-11 James M. Cline , Grace Dupuis , Zuowei Liu

Considerable efforts have been dedicated to discovering a dark photon via the decay of the Higgs boson to a photon and an invisible particle. A subject that is still mostly unexplored is which properties of the dark photon could be measured…

高能物理 - 唯象学 · 物理学 2022-05-11 Hugues Beauchesne , Cheng-Wei Chiang

Dark matter particles need not be completely stable, and in fact they may be decaying now. We consider this possibility in the frameworks of universal extra dimensions and supersymmetry with very late decays of WIMPs to Kaluza-Klein…

天体物理学 · 物理学 2009-06-23 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari
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