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We explore GxG unified theories with the visible and the hidden or dark sectors paired under a Z2 symmetry. Developing a system of 'asymmetric symmetry breaking' we motivate such models on the basis of their ability to generate dark baryons…

High Energy Physics - Phenomenology · Physics 2015-07-08 Stephen J. Lonsdale , Raymond R. Volkas

We investigate a theory of $SU(9)$ dark grand unification, where dark matter consists of asymmetric dark baryons from the $Sp(4)_D$ dark QCD sector. By unifying the dark color gauge group with the Standard Model gauge group, the asymmetry…

High Energy Physics - Phenomenology · Physics 2026-02-03 Yi Chung

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

Motivated by the observed ratio of dark matter to baryon mass densities, $\rho_D/\rho_B \simeq 5$, we propose a theory of dark-color unification. In this theory, the dark to visible baryon masses are fixed by the ratio of dark to visible…

High Energy Physics - Phenomenology · Physics 2022-05-18 Clara Murgui , Kathryn M. Zurek

Some models of asymmetric dark matter commonly employ a gauge group structure of the form $G_{V}\times{}G_{D}$ where $G_{V}$ is the visible gauge group containing the Standard Model and $G_{D}$ is the gauge group responsible for…

High Energy Physics - Phenomenology · Physics 2017-05-08 Benjamin D. Callen

Motivated by the collisionless cold dark matter small scale structure problem, we propose an asymmetric dark matter model where dark matter particle interact with each other via a massive dark gauge boson. This model easily avoid the strong…

High Energy Physics - Phenomenology · Physics 2023-05-31 Zien Chen , Kairui Ye , Mengchao Zhang

We propose a scenario that explains the comparable abundances of dark matter (DM) and baryons without any coincidence in the corresponding particle masses. Here, DM corresponds to heavy "dark baryons" in a hidden MSSM-like dark sector,…

High Energy Physics - Phenomenology · Physics 2022-11-21 João G. Rosa , Duarte M. C. Silva

The similar cosmological abundances observed for visible and dark matter suggest a common origin for both. By viewing the dark matter density as a dark-sector asymmetry, mirroring the situation in the visible sector, we show that the…

High Energy Physics - Phenomenology · Physics 2012-03-01 Kalliopi Petraki , Mark Trodden , Raymond R. Volkas

We introduce a model for matters-genesis in which both the baryonic and dark matter asymmetries originate from a first-order phase transition in a dark sector with an $SU(3)\times SU(2)\times U(1)$ gauge group and minimal matter content. In…

High Energy Physics - Phenomenology · Physics 2023-03-10 Eleanor Hall , Thomas Konstandin , Robert McGehee , Hitoshi Murayama

Asymmetric dark matter (ADM) is motivated by the similar cosmological mass densities measured for ordinary and dark matter. We present a comprehensive theory for ADM that addresses the mass density similarity, going beyond the usual ADM…

High Energy Physics - Phenomenology · Physics 2018-05-23 Stephen J. Lonsdale , Raymond R. Volkas

We consider the production of asymmetric dark matter during hidden sector baryogenesis. We consider a particular supersymmetric model where the dark matter candidate has a number density approximately equal to the baryon number density,…

High Energy Physics - Phenomenology · Physics 2011-10-03 Bhaskar Dutta , Jason Kumar

Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

High Energy Physics - Phenomenology · Physics 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

D3-brane probes of E-type Yukawa points lead to strongly coupled nearly conformal sectors nearby the Standard Model (visible sector) which are motivated by F-theory GUTs. Realistic visible sector brane configurations induce a seesaw mass…

High Energy Physics - Theory · Physics 2015-03-19 Jonathan J. Heckman , Soo-Jong Rey

About 80\% of the mass of the present Universe is made up of the unknown (dark matter), while the rest is made up of ordinary matter. It is a very intriguing question why the {\it mass} densities of dark matter and ordinary matter (mainly…

High Energy Physics - Phenomenology · Physics 2019-10-23 Masahiro Ibe , Ayuki Kamada , Shin Kobayashi , Takumi Kuwahara , Wakutaka Nakano

We propose a theory in which the Standard Model gauge symmetry is extended by a new $SU(2)_\ell$ group acting nontrivially on the lepton sector which is spontaneously broken at the TeV scale. Under this $SU(2)_\ell$ the ordinary leptons…

High Energy Physics - Phenomenology · Physics 2017-08-09 Bartosz Fornal , Yuri Shirman , Tim M. P. Tait , Jennifer Rittenhouse West

I suggest a new extension of the standard model of particle physics, which introduces a dark sector with the $SU(2)_{D}\otimes U(1)_{D'}$ symmetry besides the SM sector. The new particles of the model all inhabit in the dark sector. The…

High Energy Physics - Phenomenology · Physics 2019-06-26 Wei-Min Yang

We argue that the striking similarity between the cosmic abundances of baryons and dark matter, despite their very different astrophysical behavior, strongly motivates the scenario in which dark matter resides within a rich dark sector…

High Energy Physics - Phenomenology · Physics 2024-06-13 Arushi Bodas , Manuel A. Buen-Abad , Anson Hook , Raman Sundrum

In gauge-mediated theories supersymmetry breaking originates in a strongly interacting sector and is communicated to the ordinary sparticles via SU(3)$\times$SU(2)$\times$U(1) carrying ``messenger'' particles. Stable baryons of the strongly…

High Energy Physics - Phenomenology · Physics 2009-10-28 S. Dimopoulos , G. F. Giudice , A. Pomarol

The asymmetric dark matter (ADM) paradigm is motivated by the apparent coincidence between the cosmological mass densities of visible and dark matter, $\Omega_\mathrm{DM} \simeq 5\Omega_\mathrm{VM}$. However, most ADM models only relate the…

High Energy Physics - Phenomenology · Physics 2023-02-15 Alexander C. Ritter , Raymond R. Volkas

The cosmological origin of both dark and baryonic matter can be explained through a unified mechanism called hylogenesis where baryon and antibaryon number are divided between the visible sector and a GeV-scale hidden sector, while the…

High Energy Physics - Phenomenology · Physics 2012-12-04 Nikita Blinov , David E. Morrissey , Kris Sigurdson , Sean Tulin
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