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We propose a new mechanism to simultaneously explain the observed dark matter abundance and the baryon asymmetry of the Universe. The mechanism is based on the Filtered Dark Matter scenario, where dark matter particles acquire a large mass…

高能物理 - 唯象学 · 物理学 2022-08-24 Michael J. Baker , Moritz Breitbach , Joachim Kopp , Lukas Mittnacht , Yotam Soreq

Primordial nucleosynthesis, or Big-Bang Nucleosynthesis (BBN), is one of the three evidences for the Big-Bang model, together with the expansion of the Universe and the Cosmic Microwave Background. There is a good global agreement over a…

核实验 · 物理学 2017-01-18 Alain Coc

Ultralight scalar dark matter can interact with all massive Standard Model particles through a universal coupling. Such a coupling modifies the Standard Model particle masses and affects the dynamics of Big Bang Nucleosynthesis. We model…

高能物理 - 唯象学 · 物理学 2020-12-16 Sergey Sibiryakov , Philip Sørensen , Tien-Tien Yu

The existence of Dark Matter (DM) is a well established fact since many decades, thanks to the observation of the effects of its gravitational interaction with the ordinary matter in the Universe. However, our knowledge of the Dark Matter…

高能物理 - 唯象学 · 物理学 2020-09-08 Alessandra Filippi , Marzio De Napoli

We perform calculations of dark photon production and decay in the early universe for ranges of dark photon masses and vacuum coupling with standard model photons. Simultaneously and self-consistently with dark photon production and decay,…

宇宙学与河外天体物理 · 物理学 2021-01-05 Jung-Tsung Li , George M. Fuller , Evan Grohs

Scenarios with gravitino dark matter face potential cosmological problems induced by the presence of the Next-to-Lightest Supersymmetric Particle (NLSP) at the time of Big Bang Nucleosynthesis (BBN). A very simple, albeit radical, solution…

高能物理 - 唯象学 · 物理学 2007-10-16 Alejandro Ibarra

We describe the model-independent mechanism by which dark matter and dark matter structures heavier than $\sim 8\times 10^{11}$ GeV form binary pairs in the early Universe that spin down and merge both in the present and throughout the…

高能物理 - 唯象学 · 物理学 2023-08-29 Melissa D. Diamond , David E. Kaplan , Surjeet Rajendran

Any neutral boson such as a dark photon or dark Higgs that is part of a non-standard sector of particles can mix with its standard model counterpart. When very weakly mixed with the Standard Model, these particles are produced in the early…

高能物理 - 唯象学 · 物理学 2016-11-23 Joshua Berger , Karsten Jedamzik , Devin G. E. Walker

A simple way of explaining dark matter without modifying known Standard Model physics is to require the existence of a hidden (dark) sector, which interacts with the visible one predominantly via gravity. We consider a hidden sector…

高能物理 - 唯象学 · 物理学 2020-03-04 R. Foot , S. Vagnozzi

The high densities in the early Universe provide a unique laboratory to constrain couplings between feebly interacting particles, such as dark matter and neutrinos. In this article, we study how Big Bang Nucleosynthesis can constrain models…

高能物理 - 唯象学 · 物理学 2025-09-30 Toni Bertólez-Martínez , Justo López-Sarrión , Jordi Salvado

A light ($m_{\nu d} \lesssim $ MeV) dark fermion mixing with the Standard Model neutrinos can naturally equilibrate with the neutrinos via oscillations and scattering. In the presence of dark sector interactions, production of dark fermions…

宇宙学与河外天体物理 · 物理学 2024-02-02 Daniel Aloni , Melissa Joseph , Martin Schmaltz , Neal Weiner

Big bang nucleosynthesis (BBN), an epoch of primordial nuclear transformations in the expanding Universe, has left an observable imprint in the abundances of light elements. Precision observations of such abundances, combined with…

高能物理 - 唯象学 · 物理学 2011-04-14 Maxim Pospelov , Josef Pradler

The observational relation between the density of baryon and dark matter in the Universe, $\Omega_{\rm DM}/\Omega_B\simeq 5$, is one of the most difficult problems to solve in modern cosmology. We discuss a scenario that explains this…

高能物理 - 唯象学 · 物理学 2013-05-30 Kohei Kamada , Masahide Yamaguchi

We perform a consistent analysis of the alternative left-right symmetric model emerging from $E_6$ grand unification. We include a large set of theoretical and experimental constraints, with a particular emphasis on dark matter observables…

高能物理 - 唯象学 · 物理学 2020-04-28 Mariana Frank , Benjamin Fuks , Özer Özdal

The standard model (SM) of particle physics is for the last three decades a very successful description of the properties and interactions of all known elementary particles. Currently, it is again probed with the first collisions at the…

高能物理 - 唯象学 · 物理学 2011-04-18 Florian Staub

Motivated by inflation, the theory of big-bang nucleosynthesis and the quest for a deeper understanding of the fundamental forces and particles, a very successful paradigm for the development of structure in the Universe has evolved. It…

天体物理学 · 物理学 2009-10-28 Scott Dodelson , Evalyn Gates , Michael S. Turner

The possible role of supersymmetry in our understanding of big bang baryogenesis and cosmological dark matter is explored. The discussion will be limited to the out-of equilibrium decay scenario in SUSY GUTs, the decay of scalar…

高能物理 - 唯象学 · 物理学 2016-09-01 Keith A. Olive

Primordial nucleosynthesis, or big bang nucleosynthesis (BBN), is one of the three evidences for the big bang model, together with the expansion of the universe and the cosmic microwave background. There is a good global agreement over a…

宇宙学与河外天体物理 · 物理学 2017-09-20 Alain Coc , Elisabeth Vangioni

We review some recent determinations of the amount of dark matter on galactic, cluster, and large scales, noting some puzzles and their possible resolutions. We discuss the interpretation of big bang nucleosynthesis for dark matter, and…

天体物理学 · 物理学 2007-05-23 Kim Griest

The Big Bang Nucleosynthesis (BBN) model is a cornerstone for the understanding of the evolution of the early universe, making seminal predictions that are in outstanding agreement with the present observation of light element abundances in…

核理论 · 物理学 2023-02-15 Carlos A. Bertulani , Francis W. Hall , Benjamin I. Santoyo