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Based on tentative evidence for a peak in the Fermi gamma-ray spectrum originating from near the center of the galaxy, it has been suggested that dark matter of mass ~130 GeV is annihilating directly into photons with a cross section ~24…

High Energy Physics - Phenomenology · Physics 2013-05-30 James M. Cline

Asymmetric Dark Matter (ADM) models relate the dark matter density to the baryon asymmetry, so that a natural mass scale for ADM is around a few GeV. In existing models of ADM, this mass scale is unexplained; here we generate this GeV scale…

High Energy Physics - Phenomenology · Physics 2014-11-21 Timothy Cohen , Daniel J. Phalen , Aaron Pierce , Kathryn M. Zurek

We present updated constraints on dark matter models with momentum-dependent or velocity-dependent interactions with nuclei, based on direct detection and solar physics. We improve our previous treatment of energy transport in the solar…

High Energy Physics - Phenomenology · Physics 2016-11-15 Aaron C. Vincent , Pat Scott , Aldo Serenelli

The DAMIC-M collaboration recently reported impressive bounds on sub-GeV dark matter, robustly testing both thermal and non-thermal models for the very first time. In this work we derive novel bounds from the recent PandaX-4T ionization…

High Energy Physics - Phenomenology · Physics 2025-07-23 Andrew Cheek , Pablo Figueroa , Gonzalo Herrera , Ian M. Shoemaker

Searching for dark matter (DM) at colliders is one of the biggest challenges in high-energy physics today. Significant efforts have been made to detect DM within the mass range of 1-10,000 GeV at the Large Hadron Collider and other…

High Energy Physics - Experiment · Physics 2025-11-17 Tamas Almos Vami

Diverse astrophysical observations suggest the existence of cold dark matter that interacts only gravitationally with radiation and ordinary baryonic matter. Any nonzero coupling between dark matter and baryons would provide a significant…

Annihilation of light dark matter of $m_{\rm DM} \approx (10-40)$ GeV into the Standard Model fermions has been suggested as a possible origin of the gamma-ray excess at GeV energies in the Fermi-LAT data. In this paper, we examine possible…

High Energy Physics - Phenomenology · Physics 2015-06-19 Kyoungchul Kong , Jong-Chul Park

The scenario of isospin-violating dark matter (IVDM) with destructive interference between DM-proton and DM-neutron scatterings provides a potential possibility to reconcile the experimental results of DAMA, CoGeNT and XENON. We explore the…

High Energy Physics - Phenomenology · Physics 2016-02-24 Yu-Feng Zhou

Current multi-ton detectors put stringent constraints on the GeV-scale galactic dark matter, pushing the allowed cross-section almost towards the neutrino fog, yet remain mostly insensitive to the light dark matter. Cosmic rays can…

High Energy Physics - Phenomenology · Physics 2026-01-26 Sk Jeesun , Anirban Majumdar

In this work we complete a model independent analysis of dark matter constraining its mass and interaction strengths with data from astro- and particle physics experiments. We use the effective field theory framework to describe…

High Energy Physics - Phenomenology · Physics 2015-06-19 Csaba Balázs , Tong Li , Jayden L. Newstead

The forest of Lyman-$\alpha$ absorption lines detected in the spectra of distant quasars encodes information on the nature and properties of dark matter and the thermodynamics of diffuse baryonic material. Its main observable -- the 1D flux…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-19 Bruno Villasenor , Brant Robertson , Piero Madau , Evan Schneider

Direct detection experiments relying on nuclear recoil signatures lose sensitivity to sub-GeV dark matter for typical galactic velocities. This sensitivity is recovered if there exists another source of flux with higher momenta. Such an…

High Energy Physics - Phenomenology · Physics 2020-03-03 James Alvey , Miguel Campos , Malcolm Fairbairn , Tevong You

We examine cosmological, astrophysical and collider constraints on thermal dark matter (DM) with mass mX in the range 1 MeV to 10 GeV. Cosmic microwave background (CMB) observations, which severely constrain light symmetric DM, can be…

High Energy Physics - Phenomenology · Physics 2012-12-12 Tongyan Lin , Hai-Bo Yu , Kathryn M. Zurek

We propose a method that allows to place an upper limit on the dark matter elastic scattering cross section with nucleons which is independent of the velocity distribution. Our approach combines null results from direct detection…

High Energy Physics - Phenomenology · Physics 2015-09-30 Francesc Ferrer , Alejandro Ibarra , Sebastian Wild

Deep inelastic scattering of $e^{\pm}$ off protons is sensitive to contributions from "dark photon" exchange. Using HERA data fit to HERA's parton distribution functions, we obtain the model-independent bound $\epsilon \lesssim 0.02$ on the…

High Energy Physics - Phenomenology · Physics 2021-01-13 Graham D. Kribs , David McKeen , Nirmal Raj

We report on constraints on the lifetime of decaying gravitino dark matter in models with bilinear R-parity violation derived from observations of cosmic-ray antiprotons with the PAMELA experiment. Performing a scan over a viable set of…

High Energy Physics - Phenomenology · Physics 2015-03-30 Michael Grefe , Timur Delahaye

I consider constraints from observations on a cutoff scale in clustering due to free streaming of the dark matter in a warm dark matter cosmological model with a cosmological constant. The limits are derived in the framework of a sterile…

Astrophysics · Physics 2007-05-23 Kevork Abazajian

A search for dark matter produced in association with a dark Higgs boson decaying into a bottom quark-antiquark pair has been performed using proton-proton collision data at a center-of-mass energy of 13 TeV. The search uses data collected…

High Energy Physics - Experiment · Physics 2026-04-24 CMS Collaboration

New results after 0.69 kg yr of measurement with an enriched 76Ge detector of the Heidelberg--Moscow experiment with an active mass of 2.758 kg are presented. An energy threshold of 9 keV and a background level of 0.042 counts/(kg d keV) in…

We generalize the recently proposed continuum dark matter model to the case where the dark matter consists of a spin-$1/2$ or spin-$1$ gapped continuum. We construct simple continuum analogs of weakly interacting massive particles…

High Energy Physics - Phenomenology · Physics 2023-02-22 Csaba Csaki , Ameen Ismail , Seung J. Lee