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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…

高能物理 - 唯象学 · 物理学 2023-03-10 Eleanor Hall , Thomas Konstandin , Robert McGehee , Hitoshi Murayama

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron…

高能物理 - 唯象学 · 物理学 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

We consider a baryogenesis scenario, where the difference of baryon (B) and lepton (L) number is conserved in such a way that the B-L asymmetry in the standard model sector is compensated by an asymmetry of opposite sign stored in the dark…

高能物理 - 唯象学 · 物理学 2010-11-26 Florian Bauer , Marc-Thomas Eisele , Mathias Garny

We introduce a new mechanism for the simultaneous generation of baryon and dark matter asymmetries through ultraviolet-dominated freeze-in scatterings. The mechanism relies on heavy Majorana neutrinos that connect the visible Standard Model…

高能物理 - 唯象学 · 物理学 2026-03-05 Pouya Asadi , Marianne Moore , David E. Morrissey , Michael Shamma

In standard models of baryogenesis and of dark matter, the mechanisms which generate the densities in both sectors are unrelated to each other. In this paper we explore models which generate the baryon asymmetry through the dark matter…

高能物理 - 唯象学 · 物理学 2010-12-24 Jessie Shelton , Kathryn M. Zurek

We propose a mechanism for cogenesis of baryon and dark matter (DM) in the universe via the Affleck-Dine (AD) route. An AD field which breaks the lepton number symmetry, leads to the generation of lepton asymmetry by virtue of its cosmic…

高能物理 - 唯象学 · 物理学 2023-05-24 Debasish Borah , Suruj Jyoti Das , Nobuchika Okada

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

We propose a new mechanism where asymmetric dark matter (ADM) and the baryon asymmetry are both generated in the same decay chain of a metastable weakly interacting massive particle (WIMP) after its thermal freeze-out. Dark matter and…

高能物理 - 唯象学 · 物理学 2020-12-11 Yanou Cui , Michael Shamma

We discuss aidnogenesis, the generation of a dark matter asymmetry via new sphaleron processes associated to an extra non-abelian gauge symmetry common to both the visible and the dark sectors. Such a theory can naturally produce an…

高能物理 - 唯象学 · 物理学 2011-03-07 Mattias Blennow , Basudeb Dasgupta , Enrique Fernandez-Martinez , Nuria Rius

The main mechanism responsible for Axion-Like-Particle (ALP) production in the early universe is the so-called misalignment mechanism. Three regimes have been investigated in this context: standard misalignment, large misalignment and…

高能物理 - 唯象学 · 物理学 2025-04-02 Cem Eröncel , Ryosuke Sato , Geraldine Servant , Philip Sørensen

We will review the main aspects of a mechanism for the contemporary generation of the baryon and Dark Matter abundances from the out-of-equilibrium decay of a Wimp-like mother particle and briefly discuss a concrete realization in a…

高能物理 - 唯象学 · 物理学 2016-03-23 Giorgio Arcadi

We argue that coherent oscillations of the axion field excited by the misalignment mechanism and non-thermal leptogenesis by the saxion decay can naturally explain the observed abundance of dark matter and baryon asymmetry, thus providing a…

高能物理 - 唯象学 · 物理学 2015-06-12 Kwang Sik Jeong , Fuminobu Takahashi

We explore a mechanism for producing the baryon asymmetry and dark matter in models with multiple hidden sectors that are Standard-Model-like but with varying Higgs mass parameters. If the field responsible for reheating the Standard Model…

高能物理 - 唯象学 · 物理学 2024-04-08 Hassan Easa , Thomas Gregoire , Daniel Stolarski , Catarina Cosme

In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

高能物理 - 唯象学 · 物理学 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

We propose a scenario where dark matter (DM) with a wide mass range from a few keV to PeV can be produced solely from evaporating primordial black holes (PBH), while being consistent with the required free streaming length for structure…

高能物理 - 唯象学 · 物理学 2022-09-07 Basabendu Barman , Debasish Borah , Suruj Jyoti Das , Rishav Roshan

We propose a new mechanism to understand the relation between the baryon and dark matter asymmetries in the universe in theories where the baryon number is a local symmetry. In these scenarios the B-L asymmetry generated through a mechanism…

高能物理 - 唯象学 · 物理学 2014-03-11 Pavel Fileviez Perez , Hiren H. Patel

Motivated by their potential role as dark matter, we study the cosmological evolution of light scalar and vector fields non-minimally coupled to gravity. Our focus is on a situation where the dominant contribution to the energy density…

高能物理 - 唯象学 · 物理学 2020-03-04 Gonzalo Alonso Álvarez , Joerg Jaeckel , Thomas Hugle

We present a unified theory of inflation, neutrino mass, baryogenesis and dark matter where global lepton number symmetry and its breaking play a crucial role. The basic idea is to use a lepton number carrying complex scalar field as the…

高能物理 - 唯象学 · 物理学 2022-03-14 Rabindra N. Mohapatra , Nobuchika Okada

We propose an unified model of dark matter and baryon asymmetry in a lepto-philic world above the electroweak scale. We provide an example where the inflaton decay products subsequently generate a lepton asymmetry and a dark matter…

高能物理 - 唯象学 · 物理学 2009-11-06 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu , Philip Stephens

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