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We show that in the presence of a chemical potential, black hole evaporation generates baryon number. If the inflaton or Ricci scalar is derivatively coupled to the B-L current, the expansion of the universe acts as a chemical potential and…

高能物理 - 唯象学 · 物理学 2015-01-06 Anson Hook

We revisit baryogenesis from the asymmetric evaporation of light primordial black holes, focusing on scenarios where gravitational effects induce a matter antimatter asymmetry. In particular, we consider a higher-dimension operator coupling…

高能物理 - 唯象学 · 物理学 2025-08-29 Joaquim Iguaz Juan , Yuber F. Perez-Gonzalez , Jessica Turner

We investigate the consistency of a scenario in which the baryon asymmetry, dark matters, as well as the cosmic density perturbation are generated simultaneously through the evaporation of primordial black holes (PBHs). This scenario can…

宇宙学与河外天体物理 · 物理学 2014-05-07 Tomohiro Fujita , Keisuke Harigaya , Masahiro Kawasaki , Ryo Matsuda

We reconsider the possibility that the observed baryon asymmetry was generated by the evaporation of primordial black holes that dominated the early universe. We present a simple derivation showing that the baryon asymmetry is insensitive…

高能物理 - 理论 · 物理学 2007-05-23 Daniel Baumann , Paul J. Steinhardt , Neil Turok

We examine the extent to which primordial black holes (PBHs) can constitute the observed dark matter while also giving rise to the measured matter-antimatter asymmetry and account for the observed baryon abundance through asymmetric Hawking…

宇宙学与河外天体物理 · 物理学 2021-04-14 Alexis Boudon , Benjamin Bose , Hyat Huang , Lucas Lombriser

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 discuss the hypothesis that the cosmological baryon asymmetry and entropy were produced in the early Universe by the primordial black hole (PBHs) evaporation.

天体物理学 · 物理学 2007-05-23 A. D. Dolgov , P. D. Naselsky , I. D. Novikov

We explore a purely gravitational origin of observed baryon asymmetry and dark matter (DM) abundance from asymmetric Hawking radiation of light primordial black holes (PBH) in presence of a non-zero chemical potential, originating from the…

高能物理 - 唯象学 · 物理学 2025-01-28 Basabendu Barman , Kousik Loho , Óscar Zapata

The evaporation of primordial black holes with a mass in the $1\ {\rm gram}\lesssim M_{\rm PBH}\lesssim$1000 kg range can lead to the production of dark matter particles of almost any mass in the range $0.1\ {\rm MeV}\lesssim m_{\rm…

宇宙学与河外天体物理 · 物理学 2019-05-06 Logan Morrison , Stefano Profumo , Yan Yu

We investigate a cogenesis scenario for composite asymmetric dark matter framework: a dark sector has a similar strong dynamics to quantum chromodynamics in the standard model, and the dark-sector counterpart of baryons is the dark matter…

高能物理 - 唯象学 · 物理学 2025-11-21 Takumi Kuwahara , Yoshiki Uchida

We propose a novel mechanism to generate a suitable baryon asymmetry from dark (hidden) sector. This is a Baryogenesis through a reverse pathway of the "asymmetric dark matter" scenario. In the mechanism, the asymmetry of dark matter is…

高能物理 - 唯象学 · 物理学 2011-09-12 N. Haba , S. Matsumoto

We find that the Hawking radiation of black holes can create the baryon number in the Higgs phase vacuum of the extended standard model with 2-Higgs doublets. We propose new scenarios of baryogenesis based on the black holes, and one of our…

高能物理 - 唯象学 · 物理学 2007-05-23 Yukinori Nagatani

The process of baryogenesis through the evaporation of black holes formed at the end of inflation phase is considered. The increase of black hole mass due to accretion from the surrounding radiation after the reheating is taken into…

天体物理学 · 物理学 2015-06-24 E. V. Bugaev , M. G. Elbakidze , K. V. Konishchev

The origin of the baryon asymmetry of the Universe (BAU) and the nature of dark matter are two of the most challenging problems in cosmology. We propose a scenario in which the gravitational collapse of large inhomogeneities at the…

宇宙学与河外天体物理 · 物理学 2019-04-26 Juan García-Bellido , Bernard Carr , Sebastien Clesse

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 propose a new scenario of the baryogenesis from primordial black holes (PBH). Assuming presence of microscopic baryon (or lepton) number violation and a CP violating operator such as $\partial_\alpha F(\mathcal{R_{....}} ) J^\alpha$,…

高能物理 - 唯象学 · 物理学 2017-04-27 Yuta Hamada , Satoshi Iso

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

If primordial black holes (PBHs) contribute more than 10 percent of the dark matter (DM) density, their energy density today is of the same order as that of the baryons. Such a cosmic coincidence might hint at a mutual origin for the…

宇宙学与河外天体物理 · 物理学 2022-01-28 Yi-Peng Wu , Elena Pinetti , Joseph Silk

We investigate the possibility that dark matter and the baryon asymmetry of the Universe are generated by the same mechanism, following an idea initially proposed by V.A. Kuzmin and recently discussed by R. Kitano and I. Low. In our model,…

高能物理 - 唯象学 · 物理学 2009-11-11 Nicolas Cosme , Laura Lopez Honorez , Michel H. G. Tytgat

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
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