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We study the case of a pseudo-scalar dark matter candidate which emerges from a complex scalar singlet, charged under a global U(1) symmetry, which is broken both explicitly and spontaneously. The pseudo-scalar is naturally stabilized by…

High Energy Physics - Phenomenology · Physics 2021-12-23 Leonardo Coito , Carlos Faubel , Juan Herrero-Garcia , Arcadi Santamaria

Dark matter (DM) could be a pseudo-Dirac thermal relic with a small mass splitting that is coupled off-diagonally to a kinetically mixed dark photon. This model, particularly in the sub-GeV mass range, is a key benchmark for accelerator…

High Energy Physics - Phenomenology · Physics 2023-08-07 Nirmalya Brahma , Saniya Heeba , Katelin Schutz

Motivated by the recently reported excess in electron recoil events by the XENON1T collaboration, we propose an inelastic fermion dark matter (DM) scenario within the framework of a gauged $L_{\mu}-L_{\tau}$ extension of the standard model…

High Energy Physics - Phenomenology · Physics 2020-12-30 Debasish Borah , Satyabrata Mahapatra , Dibyendu Nanda , Narendra Sahu

We test the plausibility that a Majorana fermion dark matter candidate with a scalar mediator explains the gamma ray excess from the Galactic center. Assuming that the mediator couples to all third generation fermions we calculate…

High Energy Physics - Phenomenology · Physics 2015-12-23 Csaba Balázs , Tong Li , Chris Savage , Martin White

Cosmic-ray (CR) physics has been a prolific field of research for over a century. The open problems related to CR acceleration, transport and modulation are deeply connected with the indirect searches for particle dark matter (DM). In…

High Energy Astrophysical Phenomena · Physics 2016-01-12 Daniele Gaggero

The existence of dark matter (DM) and the origin of the baryon asymmetry are persistent indications that the SM is incomplete. More recently, the ATLAS and CMS experiments have observed an excess of diphoton events with invariant mass of…

High Energy Physics - Phenomenology · Physics 2016-06-08 Mads T. Frandsen , Ian M. Shoemaker

We study sterile neutrino dark matter (DM) in a classically conformal U(1)' extension of the Standard Model with three right-handed neutrinos and a Majoron-like singlet scalar that generate the observed pattern of active neutrino masses and…

High Energy Physics - Phenomenology · Physics 2026-02-13 João Gonçalves , Danny Marfatia , António P. Morais , Vinícius Oliveira , Roman Pasechnik

Although Planck data supports the standard \Lambda CDM model, it still allows for the presence of Dark Radiation corresponding up to about half an extra standard neutrino species. We propose a scenario for obtaining a fractional "effective…

High Energy Physics - Phenomenology · Physics 2015-06-15 Pasquale Di Bari , Stephen F. King , Alexander Merle

The nature of Dark Matter remains one of the outstanding questions of modern astrophysics. The success of the Cold Dark Matter cosmological model argues strongly in favor of a major component of the dark matter being in the form of…

Astrophysics · Physics 2007-05-23 M. Casse , P. Fayet , S. Schanne , B. Cordier , J. Paul

The 21-cm signal from the epoch of cosmic dawn prior to reionization consists of a promising observable to gain new insights into the dark matter (DM) sector. In this paper, we investigate its potential to constrain mixed (cold + non-cold)…

Cosmology and Nongalactic Astrophysics · Physics 2022-05-04 Sambit K. Giri , Aurel Schneider

We propose a gauged $U(1)_{B-L}$ version of the light Dirac neutrino portal dark matter. The $U(1)_{B-L}$ symmetry provides a UV completion by naturally accommodating three right handed neutrinos from anomaly cancellation requirements…

High Energy Physics - Phenomenology · Physics 2024-04-10 Nayan Das , Debasish Borah

The Lambda Cold Dark Matter (LCDM) paradigm makes specific predictions for the abundance, structure, substructure and clustering of dark matter halos, the sites of galaxy formation. These predictions can be directly tested, in the low-mass…

Astrophysics of Galaxies · Physics 2019-11-06 Julio F. Navarro

If dark matter (DM) particles are lighter than a few MeV/$c^2$ and can scatter off electrons, their interaction within the solar interior results in a considerable hardening of the spectrum of galactic dark matter received on Earth. For a…

High Energy Physics - Phenomenology · Physics 2018-11-19 Haipeng An , Maxim Pospelov , Josef Pradler , Adam Ritz

One of the open questions in modern cosmology is the small scale crisis of the cold dark matter paradigm. Increasing attention has recently been devoted to self-interacting dark matter models as a possible answer. However, solving the…

Cosmology and Nongalactic Astrophysics · Physics 2017-11-15 Maria Archidiacono , Sebastian Bohr , Steen Hannestad , Jonas Helboe Jørgensen , Julien Lesgourgues

Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies between collisionless cold DM and galactic structure observations. However, $\gamma$-ray searches and the CMB strongly constrain such…

High Energy Physics - Phenomenology · Physics 2018-06-27 Iason Baldes , Marco Cirelli , Paolo Panci , Kalliopi Petraki , Filippo Sala , Marco Taoso

This paper aims to put constraints on the parameters of the Scalar Field Dark Matter (SFDM) model, when dark matter is described by a free real scalar field filling the whole Universe, plus a cosmological constant term. By using a…

Cosmology and Nongalactic Astrophysics · Physics 2022-01-05 A. A. Escobal , J. F. Jesus , S. H. Pereira

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 extend recently proposed mimetic dark matter (DM) and dust of dark energy (DE) models to a U(1)-charged gauged scalar field. This extension yields a mass to the photon via the Higgs mechanism. The square of this photon mass is…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-01 Alexander Vikman

An $SU(2)_N$ extension ($N$ stands for neutral) of the Standard Model (SM) is proposed with an additional $U(1)=S^{'}$ global symmetry, which stabilizes the lightest of the vector boson ($X,\bar{X}$) as dark matter (DM) through unbroken…

High Energy Physics - Phenomenology · Physics 2018-09-26 Basabendu Barman , Subhaditya Bhattacharya , Mohammadreza Zakeri

We review theories of Asymmetric Dark Matter (ADM), their cosmological implications and detection. While there are many models of ADM in the literature, our review of existing models will center on highlighting the few common features and…

High Energy Physics - Phenomenology · Physics 2015-06-16 Kathryn M. Zurek