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Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

High Energy Physics - Phenomenology · Physics 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

Active-sterile neutrino mixing is strongly constrained for m_s > 100 keV to avoid excessive energy losses from supernova cores. For smaller m_s, matter effects suppress the effective mixing angle except for a resonant range of energies…

High Energy Physics - Phenomenology · Physics 2011-06-07 Georg G. Raffelt , Shun Zhou

We propose a novel mechanism with two component dark matter models. The subdominant dark matter can thermalize the dominant one in galaxies, and leads to core density profiles. Using ultralight dark photons and $\mathrm{GeV}$-$\mathrm{TeV}$…

High Energy Physics - Phenomenology · Physics 2019-12-18 Jia Liu , Xiao-Ping Wang , Wei Xue

Dark matter pair production at high energy colliders may leave observable signatures in the energy and momentum spectra of the objects recoiling against the dark matter. We use LEP data on mono-photon events with large missing energy to…

High Energy Physics - Phenomenology · Physics 2011-08-09 Patrick J. Fox , Roni Harnik , Joachim Kopp , Yuhsin Tsai

Context: Dark photons (Dph) appear in theories beyond the Standard Model of particles (SM). Under certain conditions, it is possible to have a mixing between SM photons and Dphs that should be observed as anomalies in the spectrum of…

High Energy Astrophysical Phenomena · Physics 2025-12-03 Arlette Melo , Sergio Hernández , Rubén Alfaro

We study an effective theory beyond the standard model (SM) where either of two additional gauge singlets, a Majorana fermion and a real scalar, constitutes all or some fraction of dark matter. In particular, we focus on the masses of the…

High Energy Physics - Phenomenology · Physics 2019-05-22 Wen Yin

We report direct-detection constraints on light dark matter particles interacting with electrons. The results are based on a method that exploits the extremely low levels of leakage current of the DAMIC detector at SNOLAB of…

A model of dark sector where $O({\rm few~GeV})$ mass dark matter particles $\chi$ couple to a lighter dark force mediator $V$, $m_V \ll m_\chi$, is motivated by the recently discovered mismatch between simulated and observed shapes of…

High Energy Physics - Phenomenology · Physics 2024-08-30 Haipeng An , Bertrand Echenard , Maxim Pospelov , Yue Zhang

We investigate the power of low-energy, high-luminosity electron--positron colliders to probe hidden sectors with a mass below ~10 GeV that couple to Standard Model particles through a light mediator. Such sectors provide well-motivated…

High Energy Physics - Phenomenology · Physics 2015-02-24 Rouven Essig , Jeremy Mardon , Michele Papucci , Tomer Volansky , Yi-Ming Zhong

Ultralight dark photon dark matter features distinctive cosmological and astrophysical signatures and is also supported by a burgeoning direct-detection program searching for its kinetic mixing with the ordinary photon over a wide mass…

High Energy Physics - Phenomenology · Physics 2025-08-20 David Cyncynates , Zachary J. Weiner

GeV-scale dark matter is an increasingly attractive target for direct detection, indirect detection, and collider searches. Especially for masses in the MeV to GeV range, indirect detection is expected to give a leading constraint. In that…

High Energy Physics - Phenomenology · Physics 2021-02-16 Peter Reimitz

Dark matter particles can be captured by the sun with rates that depend on the dark matter mass and the DM-nucleon cross section. However, for masses below $\sim 3.3$ GeV, the captured dark matter particles evaporate, leading to an…

High Energy Physics - Phenomenology · Physics 2015-10-07 Chris Kouvaris

If sub-GeV Dark matter(DM) annihilates to the charged particles such as $e^+ e^-$, $\mu^+ \mu^-$, or $\pi^+ \pi^-$, it generates an additional source of electrons and positrons in the cosmic ray (CR) population within our Milky Way. During…

High Energy Astrophysical Phenomena · Physics 2025-12-10 Guansen Wang , Bing-Yu Su , Lei Zu , Lei Feng

We study a minimal model of pseudo-Dirac dark matter, interacting through transition electric and magnetic dipole moments. Motivated by the fact that xenon experiments can detect electrons down to $\sim$\,keV recoil energies, we consider…

High Energy Physics - Phenomenology · Physics 2023-05-24 Shiuli Chatterjee , Ranjan Laha

For active-sterile mixing to be responsible for the full relic abundance of dark matter additional new physics is needed beyond the keV-scale sterile neutrino itself. The extra ingredient we consider here is the presence of…

High Energy Physics - Phenomenology · Physics 2019-08-06 Lucas Johns , George M. Fuller

One of the interesting portals linking a dark sector and the standard model (SM) is the kinetic mixing between the SM $U(1)_Y$ field with a new dark photon $A'$ from a $U(1)_{A'}$ gauge interaction. Stringent limits have been obtained for…

High Energy Physics - Phenomenology · Physics 2017-09-13 Min He , Xiao-Gang He , Cheng-Kai Huang

In a broad class of consistent models, MeV to few-GeV dark matter interacts with ordinary matter through weakly coupled GeV-scale mediators. We show that a suitable meter-scale (or smaller) detector situated downstream of an electron…

High Energy Physics - Phenomenology · Physics 2014-02-05 Eder Izaguirre , Gordan Krnjaic , Philip Schuster , Natalia Toro

We study the direct detection prospects for a representative set of simplified models of sub-GeV dark matter (DM), accounting for existing terrestrial, astrophysical and cosmological constraints. We focus on dark matter lighter than an MeV,…

High Energy Physics - Phenomenology · Physics 2018-01-03 Simon Knapen , Tongyan Lin , Kathryn M. Zurek

We use 7 years of electron and positron Fermi-LAT data to search for a possible excess in the direction of the Sun in the energy range from 42 GeV to 2 TeV. In the absence of a positive signal we derive flux upper limits which we use to…

High Energy Astrophysical Phenomena · Physics 2020-01-15 A. Cuoco , P. De La Torre Luque , F. Gargano , M. Gustafsson , F. Loparco , M. N. Mazziotta , D. Serini

We revisit SN1987A constraints on light, hidden sector gauge bosons ("dark photons") that are coupled to the standard model through kinetic mixing with the photon. These constraints are realized because excessive bremsstrahlung radiation of…

High Energy Physics - Phenomenology · Physics 2017-09-06 Cameron Mahoney , Adam K. Leibovich , Andrew R. Zentner
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