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Related papers: Self-interacting Spin-2 Dark Matter

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We consider a fermionic dark matter candidate interacting via a scalar mediator coupled with the Standard Model through a Higgs portal. We consider general setting including both scalar and pseudoscalar interactions between the scalar and…

High Energy Physics - Phenomenology · Physics 2017-04-12 Kimmo Kainulainen , Kimmo Tuominen , Ville Vaskonen

We generalize models invoking a spin-2 particle as a mediator between the dark sector and the Standard Model. We show that a massive spin-2 messenger can efficiently play the role of a portal between the two sectors. The dark matter is then…

High Energy Physics - Phenomenology · Physics 2018-06-20 Nicolas Bernal , Maira Dutra , Yann Mambrini , Keith A. Olive , Marco Peloso , Mathias Pierre

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether…

High Energy Physics - Phenomenology · Physics 2018-05-09 Andres Olivares-Del Campo , Celine Boehm , Sergio Palomares-Ruiz , Silvia Pascoli

The small-scale structure problems of the universe can be solved by self-interacting dark matter that becomes strongly interacting at low energies. A particularly predictive model is resonant short-range self-interactions, with a…

High Energy Physics - Phenomenology · Physics 2019-05-14 Eric Braaten , Daekyoung Kang , Ranjan Laha

A promising proposal for resolving the cusp-core anomaly in the density profile of dwarf galaxies is to allow dark matter to interact with itself through a light mediator of mass much less than a GeV. The theoretical challenge is to have a…

High Energy Physics - Phenomenology · Physics 2017-02-22 Ernest Ma

If dark matter has a large self-interaction scattering cross section, then interactions among dark-matter particles will drive galaxy and cluster halos to become spherical in their centers. Work in the past has used this effect to rule out…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 Annika H. G. Peter , Miguel Rocha , James S. Bullock , Manoj Kaplinghat

Self-interacting dark matter resolves the issue of cuspy profiles that appear in non-interacting cold dark matter simluations; it may additionally resolve the so-called "too big to fail" problem in structure formation. Asymmetric dark…

High Energy Physics - Phenomenology · Physics 2013-07-05 Lauren Pearce , Alexander Kusenko

We develop an effective field theory of a generic massive particle of any spin and, as an example, apply this to study higher-spin dark matter (DM). Our formalism does not introduce unphysical degrees of freedom, thus avoiding the potential…

High Energy Physics - Phenomenology · Physics 2021-01-04 Juan Carlos Criado , Niko Koivunen , Martti Raidal , Hardi Veermäe

We present an effective non-relativistic theory of self-interacting dark matter. We classify the long range interactions and discuss how they can be generated from quantum field theories. Generic dark sectors can generate singular…

High Energy Physics - Phenomenology · Physics 2013-10-30 Brando Bellazzini , Mathieu Cliche , Philip Tanedo

A bevy of light dark matter direct detection experiments have been proposed, targeting spin-independent dark matter scattering. In order to be exhaustive, non-standard signatures that have been investigated in the WIMP window including…

High Energy Physics - Phenomenology · Physics 2019-05-14 Harikrishnan Ramani , Graham Woolley

We investigate the possibilities of searching for a self-conjugate polarizable particle in the self-interactions of light. We first observe that polarizability can arise either from the exchange of mediator states or as a consequence of the…

High Energy Physics - Phenomenology · Physics 2017-05-24 Sylvain Fichet

We review theories of dark matter (DM) beyond the collisionless paradigm, known as self-interacting dark matter (SIDM), and their observable implications for astrophysical structure in the Universe. Self-interactions are motivated, in part,…

High Energy Physics - Phenomenology · Physics 2018-03-14 Sean Tulin , Hai-Bo Yu

The recent WMAP data have confirmed that exotic dark matter together with the vacuum energy (cosmological constant) dominate in the flat Universe. The nature of the dark matter constituents cannot be determined till they are directly…

High Energy Physics - Phenomenology · Physics 2010-01-21 J. D. Vergados

Dark matter may play an important role in galaxy formation through its non-trivial properties. For example, self-interacting dark matter may contribute to the formation of the widely observed core structures in galaxies. However, galaxy…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-08 Noriaki Kitazawa

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

We initiate a systematic study of the self-interactions of a massive spin-2 "graviton" consistent with up to $\mathcal{N}=4$ supersymmetry. Using a recently developed massive on-shell superspace formalism, we construct the most general set…

High Energy Physics - Theory · Physics 2024-03-05 Laura Engelbrecht , Callum R. T. Jones , Shruti Paranjape

Self-interacting dark matter (SIDM) arises generically in scenarios for physics beyond the Standard Model that have dark sectors with light mediators or strong dynamics. The self-interactions allow energy and momentum transport through…

As has been previously proposed, a minimal modification of the standard $SU(3)\times SU(2)\times U(1)$ theory provides a viable dark matter candidate. Such a particle, a scalar gauge singlet, is naturally self-interacting---making it of…

High Energy Physics - Phenomenology · Physics 2009-11-07 Daniel E. Holz , Anthony Zee

We constrain theories of a massive spin-2 particle coupled to a massless spin-2 particle by demanding the absence of a time advance in eikonal scattering. This is an $S$-matrix consideration that leads to model-independent constraints on…

High Energy Physics - Theory · Physics 2018-07-17 James Bonifacio , Kurt Hinterbichler , Austin Joyce , Rachel A. Rosen

In this paper we (re)consider the problem of electromagnetic interactions for massless spin 2 particles and show that in $(A)dS$ spaces with non-zero cosmological constant it is indeed possible (at least in linear approximation) to switch…

High Energy Physics - Theory · Physics 2009-02-10 Yu. M. Zinoviev
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