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The persistent absence of signals in traditional dark matter searches has intensified interest in scenarios beyond the canonical weakly interacting massive particle paradigm. In this work, we investigate the collider phenomenology of feebly…

High Energy Physics - Phenomenology · Physics 2026-04-06 Junzhe Liu , Alfredo Gurrola

We explore the phenomenology of having a second epoch of dark matter annihilation into dark radiation long after the standard thermal freeze-out. Such a hidden reannihilation process could affect visible sectors only gravitationally. As a…

Cosmology and Nongalactic Astrophysics · Physics 2018-06-20 Tobias Binder , Michael Gustafsson , Ayuki Kamada , Stefan Marinus Rodrigues Sandner , Max Wiesner

Theoretical models of self-interacting dark matter represent a promising answer to a series of open problems within the so-called collisionless cold dark matter (CCDM) paradigm. In case of asymmetric dark matter, self-interactions might…

High Energy Astrophysical Phenomena · Physics 2017-08-02 Andrea Maselli , Pantelis Pnigouras , Niklas Gønlund Nielsen , Chris Kouvaris , Kostas D. Kokkotas

The weakly interacting massive particles (WIMPs) have been the most popular particle dark matter (DM) candidate for the last several decades, and it is well known that WIMP can be probed via the direct, indirect and collider experiments.…

High Energy Physics - Phenomenology · Physics 2022-03-21 Jia Liu , Xiao-Ping Wang , Ke-Pan Xie

The interacting dark matter (IDM) scenario allows for the acceleration of the Universe without Dark Energy. We constrain the IDM model by using the newly revised observational data including $H(z)$ data and Union2 SNe Ia via the Markov…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Shuo Cao , Zong-Hong Zhu , Nan Liang

The B-L extension of the Standard Model requires the existence of right-handed neutrinos and naturally realizes the seesaw mechanism of neutrino mass generation. We study the possibility of explaining the dark matter in this model with an…

High Energy Physics - Phenomenology · Physics 2015-12-23 Werner Rodejohann , Carlos E. Yaguna

We revisit the annihilation of dark matter to neutrinos in the Sun near the WW and tt kinematic thresholds. We investigate the potential importance of annihilation to WW* in a minimal dark matter model in which a Majorana singlet is mixed…

High Energy Physics - Phenomenology · Physics 2013-05-30 John Kearney , Aaron Pierce

We propose a new signature for weakly interacting massive particle (WIMP) dark matter, a spectral feature in the diffuse extragalactic gamma-ray radiation. This feature, a sudden drop of the gamma-ray intensity at an energy corresponding to…

Astrophysics · Physics 2010-04-06 Lars Bergstrom , Joakim Edsjo , Piero Ullio

We analyse dark matter in most general form of effective field theory approach. To examine the interactions between weakly interacting massive particles(WIMPs) and Standard Model (SM) particles, we use the six-dimensional EFT mediated by…

High Energy Physics - Phenomenology · Physics 2023-05-05 Ayşe Elçiboğa Kuday , Ferhat Özok , Erdinç Ulaş Saka

Hints of direct dark matter detection coming from the DAMA, CoGeNT experiments point toward light dark matter with isospin-violating and possibly inelastic couplings. However an array of astrophysical constraints are rapidly closing the…

High Energy Physics - Phenomenology · Physics 2015-05-30 James M. Cline , Andrew R. Frey

Inspired by the excess of gamma rays from the Galactic Center, we confront a number of simplified dark matter models with experimental data. Assuming a single dark matter particle coupled to standard matter via a spin-0 mediator, we compare…

High Energy Physics - Phenomenology · Physics 2014-10-01 Csaba Balázs , Tong Li

Extra dimensions can be very useful tools when constructing new physics models. Previously, we began investigating toy models for the 5-D analog of the kinetic mixing/vector portal scenario where the interactions of bulk dark matter with…

High Energy Physics - Phenomenology · Physics 2018-11-14 Thomas G. Rizzo

The bulk matter Randall-Sundrum (RS) model is a setup where Standard Model (SM) matter and gauge fields reside in the bulk of 5D warped spacetime while the Higgs field is confined on the IR brane. The wavefunctions of the 1st and 2nd…

High Energy Physics - Phenomenology · Physics 2015-05-30 Toshifumi Yamada

The detection of gravitational waves from merging binaries has ushered in the era of gravitational wave interferometer astronomy. Besides these strong, transient, calamitous events, much weaker signals can be detected if the oscillations…

Cosmology and Nongalactic Astrophysics · Physics 2021-04-26 Juan Manuel Armaleo , Diana López Nacir , Federico R. Urban

We propose an electroweakly interacting spin-1 dark matter (DM) model. The electroweak gauge symmetry, SU(2)$_L\times$U(1)$_Y$, is extended into SU(2)$_0\times$SU(2)$_1 \times $SU(2)$_2 \times$U(1)$_Y$. A discrete symmetry exchanging…

High Energy Physics - Phenomenology · Physics 2020-08-26 Tomohiro Abe , Motoko Fujiwara , Junji Hisano , Kohei Matsushita

To date, no observational confirmation of dark matter particles has been found. In this paper, we put forward an alternative approach to inferring evidence for dark matter through modified gravity, without invoking fundamental dark matter…

General Relativity and Quantum Cosmology · Physics 2025-05-28 Kimet Jusufi , Abdelrahman Yasser , Emmanuele Battista , Nader Inan

Monochromatic photons could be produced in the annihilation or decay of dark matter particles. At high energies, the search for such line features in the cosmic gamma-ray spectrum is essentially background free because plausible…

High Energy Physics - Phenomenology · Physics 2015-05-27 Gilles Vertongen , Christoph Weniger

We discuss the weak gravitational field created by isolated matter sources in the Randall-Sundrum brane-world. In the case of two branes of opposite tension, linearized Brans-Dicke (BD) gravity is recovered on either wall, with different BD…

High Energy Physics - Theory · Physics 2010-02-18 Jaume Garriga , Takahiro Tanaka

The presence of dark matter (DM) is suggested by a wealth of astrophysical and cosmological measurements. However, its underlying nature is yet unknown. Among the most promising candidates are weakly interacting massive particles (WIMPs):…

High Energy Astrophysical Phenomena · Physics 2021-08-25 A. Montanari , E. Moulin , D. Malyshev

We investigate indirect neutrino signals from annihilations of Kaluza-Klein dark matter in the Sun. Especially, we examine a five- as well as a six-dimensional model, and allow for the possibility that boundary localized terms could affect…

High Energy Physics - Phenomenology · Physics 2015-05-14 Mattias Blennow , Henrik Melbeus , Tommy Ohlsson
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