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We show that a mini-thermal inflation occurs naturally in a class of gauge mediation models of supersymmetry (SUSY) breaking, provided that the reheating temperature T_R of the primary inflation is much higher than the SUSY-breaking scale,…

高能物理 - 唯象学 · 物理学 2009-11-10 M. Fujii , M. Ibe , T. Yanagida

Standard thermal freeze-out scenarios with QCD-scale interaction rates predict a $uuddss$ sexaquark relic abundance many orders of magnitude below the observed dark matter density, representing a key challenge for sexaquark dark matter…

高能物理 - 唯象学 · 物理学 2026-05-05 Marianne Moore , Stefano Profumo

We study the possibility of realising cosmic inflation, dark matter (DM), baryon asymmetry of the universe (BAU) and light neutrino masses in non-supersymmetric minimal gauged $B-L$ extension of the standard model with three right handed…

高能物理 - 唯象学 · 物理学 2021-03-17 Debasish Borah , Suruj Jyoti Das , Abhijit Kumar Saha

In the first stages of inflationary reheating, the temperature of the radiation produced by inflaton decays is typically higher than the commonly defined reheating temperature $T_{RH} \sim (\Gamma_\phi M_P)^{1/2}$ where $\Gamma_\phi$ is the…

高能物理 - 唯象学 · 物理学 2017-11-22 Marcos A. G. Garcia , Yann Mambrini , Keith A. Olive , Marco Peloso

We unify inflation and dark matter via a single scalar field phi. One of the main difficulties for this unification is that between inflation and dark matter one needs a successful reheating process and a long lasting period of radiation.…

宇宙学与河外天体物理 · 物理学 2009-11-30 A. de la Macorra , F. Briscese

There are a lot of works within a class of classically scale invariant model, which is motivated by solving the gauge hierarchy problem. In this context, the Higgs mass vanishes at the UV scale due to the classically scale invariance, and…

高能物理 - 唯象学 · 物理学 2016-02-16 Naoyuki Haba , Hiroyuki Ishida , Ryo Takahashi , Yuya Yamaguchi

We consider gauge unification in nonminimal models with extra spacetime dimensions above the TeV scale. We study the possibility that only a a subset of the supersymmetric standard model gauge and Higgs fields live in the higher dimensional…

高能物理 - 唯象学 · 物理学 2009-10-31 Christopher D. Carone

What is commonly called the reheat temperature, $T_{RH}$, is not the maximum temperature obtained after inflation. The maximum temperature is, in fact, much larger than $T_{RH}$. As an application of this we consider the production of…

高能物理 - 唯象学 · 物理学 2016-08-25 Daniel J. H. Chung , Edward W. Kolb , Antonio Riotto

Mechanisms for the generation of the matter-antimatter asymmetry and dark matter strongly depend on the reheating temperature T_R, the maximal temperature reached in the early universe. Forthcoming results from the LHC, low energy…

高能物理 - 唯象学 · 物理学 2012-12-17 Wilfried Buchmuller

We analyze a recently proposed extension of the Standard Model based on the SU(4) x SU(2)_L x U(1)_X gauge group, in which baryon number is interpreted as the fourth color and dark matter emerges as a neutral partner of the ordinary quarks…

高能物理 - 唯象学 · 物理学 2016-04-13 Bartosz Fornal , Tim M. P. Tait

Minimal dark matter is an attractive candidate for dark matter because it is stabilized without the need to impose additional symmetries. It is known that the $SU(2)_L$ quintuplet fermion can serve as a minimal dark matter candidate, with…

高能物理 - 唯象学 · 物理学 2025-03-26 Takashi Toma

We discuss the production of dark matter with mass of order $10$-$100$ TeV and $\mathcal{O}(1)$ couplings to the standard model, a scenario we refer to as the `mesotuned WIMP'. Given the lack of new physics observed at the LHC, indicating…

高能物理 - 唯象学 · 物理学 2023-06-01 Michael Nee

The dynamics of cosmic reheating, that is, on how the energy stored in the inflaton is transferred to the standard model (SM) thermal bath, is largely unknown. In this work, we show that the phenomenology of the nonbaryonic dark matter (DM)…

高能物理 - 唯象学 · 物理学 2025-03-14 Nicolás Bernal , Kuldeep Deka , Marta Losada

In the absence of low energy supersymmetry, we show that (a) the dark matter particle alone at the TeV scale can improve gauge coupling unification, raising the unification scale up to the lower bound imposed by proton decay, and (b) the…

高能物理 - 唯象学 · 物理学 2010-04-20 Michele Frigerio , Thomas Hambye

SO(10) grand unification accommodates intermediate gauge symmetries with which gauge coupling unification can be realized without supersymmetry. In this paper, we discuss the possibility that a new massive gauge boson associated with an…

高能物理 - 唯象学 · 物理学 2016-03-23 Jason L. Evans , Natsumi Nagata , Keith A. Olive , Jiaming Zheng

We investigate a new bound on the low reheating temperature in a scenario where the Universe experiences early matter-domination before reheating after which the standard big bang cosmology begins. In many models of dark matter (DM), the…

宇宙学与河外天体物理 · 物理学 2017-08-30 Ki-Young Choi , Tomo Takahashi

We propose a simple non-supersymmetric grand unified theory (GUT) based on the gauge group $SO(10) \times U(1)_\psi$. The model includes 3 generations of fermions in ${\bf 16}$ ($+1$), ${\bf 10}$ ($-2$) and ${\bf 1}$ ($+4$) representations.…

高能物理 - 唯象学 · 物理学 2019-07-01 Nobuchika Okada , Digesh Raut , Qaisar Shafi

Supersymmetric models with t-b-\tau Yukawa unification at M_{GUT} qualitatively predict a sparticle mass spectrum including first and second generation scalars at the 3--15 TeV scale, third generation scalars at the (few) TeV scale and…

高能物理 - 唯象学 · 物理学 2010-04-21 Howard Baer , Markus Haider , Sabine Kraml , Sezen Sekmen , Heaya Summy

We propose a new thermal freeze-out mechanism for ultra-heavy dark matter. Dark matter coannihilates with a lighter unstable species, leading to an annihilation rate that is exponentially enhanced relative to standard WIMPs. This scenario…

高能物理 - 唯象学 · 物理学 2017-09-27 Asher Berlin

The discovery of nongravitational interactions between dark matter and the Standard Model would be an important step in unraveling the nature of dark matter. If such an interaction exists, it would have profound implications on how dark…

高能物理 - 唯象学 · 物理学 2019-07-11 Hongwan Liu