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Low-scale supersymmetry breaking in string motivated theories implies the presence of O(100) TeV scale moduli, which generically lead to a significant modification of the history of the universe prior to Big Bang Nucleosynthesis. Such an…

高能物理 - 唯象学 · 物理学 2015-05-30 Gordon Kane , Jing Shao , Scott Watson , Hai-Bo Yu

We study a cogenesis mechanism in which the observed baryon asymmetry of the universe and the dark matter abundance can be produced simultaneously at low reheating temperature without violating baryon number in the fundamental vertex. In…

高能物理 - 唯象学 · 物理学 2016-04-20 Mansi Dhuria , Chandan Hati , Utpal Sarkar

We propose a minimal gauged $U(1)_{B-L}$ extension of the minimal supersymmetric Standard Model (MSSM) which resolves the cosmological moduli problem via thermal inflation, and realizes late-time Affleck-Dine leptogensis so as to generate…

高能物理 - 唯象学 · 物理学 2023-11-14 Kwang Sik Jeong , Wan-il Park

The generic expectation in string/supergravity models is that there are multiple moduli fields with masses of the order of the supersymmetry breaking scale. We study the cosmology that arises as a result of vacuum misalignment of these…

高能物理 - 理论 · 物理学 2020-01-23 Bobby S. Acharya , Mansi Dhuria , Diptimoy Ghosh , Anshuman Maharana , Francesco Muia

Cosmology and particle physics are deeply interrelated. Among the common problems are dark energy, dark matter and baryon asymmetry of the Universe. We discuss these problems in general terms, and concentrate on several particular…

广义相对论与量子宇宙学 · 物理学 2018-05-01 V. A. Rubakov

Cosmological moduli generically come to dominate the energy density of the early universe, and thereby trigger an early matter dominated era. Such non-standard cosmological histories are expected to have profound effects on the evolution…

高能物理 - 唯象学 · 物理学 2025-06-13 Robert Wiley Deal , Leia Barrowes , John T. Giblin, , Kuver Sinha , Scott Watson , Fred C. Adams

Recent developments in string theory have led to "realistic" string compactifications which lead to moduli stabilization while generating a hierarchy between the Electroweak and Planck scales at the same time. However, this seems to suggest…

高能物理 - 唯象学 · 物理学 2009-09-16 Piyush Kumar

The supersymmetrized DFSZ axion model is especially compelling in that it contains 1. the SUSY solution to the gauge hierarchy problem, 2. the Peccei-Quinn (PQ) solution to the strong CP problem and 3. the Kim-Nilles solution to the SUSY mu…

高能物理 - 唯象学 · 物理学 2023-07-05 Howard Baer , Vernon Barger , Robert Wiley Deal

${\rm B - L}$ cosmic strings form in a wide class of theories beyond the Standard Model which contain a ${\rm U}(1)_{{\rm B - L}}$ gauge symmetry. They can form at the end of hybrid inflation and explain, together with inflation, the Cosmic…

高能物理 - 唯象学 · 物理学 2007-05-23 R. Jeannerot

Late-decaying string moduli dilute the baryon asymmetry of the universe created in any previous era. The reheat temperature for such moduli is below a GeV, thus motivating baryogenesis at very low temperatures. We present an extension of…

高能物理 - 唯象学 · 物理学 2014-11-21 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

We critically review the role of cosmological moduli in determining the post-inflationary history of the universe. Moduli are ubiquitous in string and M-theory constructions of beyond the Standard Model physics, where they parametrize the…

高能物理 - 理论 · 物理学 2015-08-06 Gordon Kane , Kuver Sinha , Scott Watson

We investigate the possibility that both the baryon asymmetry of the universe and the observed cold dark matter density are generated by decays of a heavy scalar field which dominates the universe before nucleosynthesis. Since baryons and…

高能物理 - 唯象学 · 物理学 2008-11-26 Ryuichiro Kitano , Hitoshi Murayama , Michael Ratz

Light moduli fields, gravitationally coupled scalar fields with no classical potential and which are expected to emerge as remnants from string theory compactification, are dangerous to cosmology in that 1. their late-time decays may…

高能物理 - 唯象学 · 物理学 2021-12-24 Howard Baer , Vernon Barger , Robert Wiley Deal

Composite dark matter is a natural setting for implementing inelastic dark matter - the O(100 keV) mass splitting arises from spin-spin interactions of constituent fermions. In models where the constituents are charged under an axial U(1)…

高能物理 - 唯象学 · 物理学 2014-11-20 Daniele S. M. Alves , Siavosh R. Behbahani , Philip Schuster , Jay G. Wacker

We put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a $\mathrm{U}(1)$ scalar field coupled to dark matter. High dark matter densities cause the $\mathrm{U}(1)$ symmetry to break…

高能物理 - 唯象学 · 物理学 2017-11-22 Jeremy Sakstein , Mark Trodden

Many models of supersymmetry breaking involve particles with weak scale mass and Planck mass suppressed couplings. Coherent production of such particles in the early universe destroys the successful predictions of nucleosynthesis. We show…

高能物理 - 唯象学 · 物理学 2009-09-15 Lisa Randall , Scott Thomas

We study in detail the conditions to generate the baryon asymmetry of the universe from the annihilation of dark matter. This scenario requires a low energy mechanism for thermal baryogenesis, hence we first discuss some of these mechanisms…

高能物理 - 唯象学 · 物理学 2015-06-16 Nicolas Bernal , Stefano Colucci , Francois-Xavier Josse-Michaux , J. Racker , Lorenzo Ubaldi

Despite their tremendous successes, modern-day cosmology and particle physics harbor a variety of unresolved mysteries. Two of the biggest are the origin of the baryon asymmetry of the Universe and the existence and nature of dark matter.…

宇宙学与河外天体物理 · 物理学 2023-01-26 Moritz Breitbach

We propose a simple and flexible mechanism by which sterile neutrinos with masses below the electroweak scale can simultaneously account for the observed baryon asymmetry of the Universe and the dark matter abundance. Crucially, neutrinos…

高能物理 - 唯象学 · 物理学 2026-03-23 G. Arcadi , J. P. Garcés , M. Lindner

A model of inhomogeneous baryogenesis based on the Affleck and Dine mechanism is described. A simple coupling of the scalar baryon field to the inflaton allows for formation of astronomically significant bubbles with a large baryon (or…

高能物理 - 唯象学 · 物理学 2008-11-26 A. D. Dolgov , M. Kawasaki , N. Kevlishvili
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