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We explore a scenario in which dark matter is a massive bosonic field, arising solely from quantum fluctuations generated during inflation. In this framework, dark matter exhibits primordial isocurvature perturbations with an amplitude of…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-06 Mohammad Ali Gorji , Misao Sasaki , Teruaki Suyama

The existence of Dark Matter (DM) has been well established from various cosmological and astrophysical evidences. However, the particle properties of DM are largely undetermined and attempts to probe its interactions with the Standard…

High Energy Physics - Phenomenology · Physics 2018-12-26 Nicolás Bernal , Arindam Chatterjee , Arnab Paul

Recent cosmological observations indicate the existence of extra light species, i.e., dark radiation. In this paper we show that signatures of the dark radiation are imprinted in the spectrum of inflationary gravitational waves. If the dark…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Ryusuke Jinno , Takeo Moroi , Kazunori Nakayama

We derive a bound on dark photon dark matter scenarios where the dark photon mass is generated through the Higgs mechanism, based on the requirement that symmetry breaking must occur sufficiently early in the universe. We emphasize that…

High Energy Physics - Phenomenology · Physics 2025-02-06 Naoya Kitajima , Shota Nakagawa , Fuminobu Takahashi , Wen Yin

We present a novel perspective on the role of inflation in the production of Dark Matter (DM). Specifically, we explore the DM production during Warm Inflation via ultraviolet Freeze-In (WIFI). We demonstrate that in a Warm Inflation (WI)…

High Energy Physics - Phenomenology · Physics 2024-12-10 Katherine Freese , Gabriele Montefalcone , Barmak Shams Es Haghi

The origin of dark matter in the universe may be weakly interacting scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We present two interesting cases, the case of small…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ram Brustein , Merav Hadad

We propose a new mechanism for generating both luminous and dark matter during cosmic inflation. According to this mechanism, ordinary and dark matter carry common charge which is associated with an anomalous $ U(1)_{X} $ group. Anomaly…

High Energy Physics - Phenomenology · Physics 2015-03-10 Neil D. Barrie , Archil Kobakhidze

Dark matter modeled as a classical scalar field that interacts only with gravity and with itself by a potential that is close to quartic at large field values and approaches a quadratic form when the field is small would be gravitationally…

Astrophysics · Physics 2009-10-31 P. J. E. Peebles

We calculate the rate of production of dark photons from electron-positron pair annihilation in hot and dense matter characteristic of supernova progenitors. Given the non-linear dependence of the emission rate on the dark photon mass and…

High Energy Physics - Phenomenology · Physics 2019-07-24 Ermal Rrapaj , Andre Sieverding , Yong-Zhong Qian

We study the possibility that a keV-MeV mass hidden photon (HP), i.e. a hidden sector U(1) gauge boson, accounts for the observed amount of dark matter. We focus on the case where the HP interacts with the standard model sector only through…

High Energy Physics - Phenomenology · Physics 2010-04-28 Marieke Postma , Javier Redondo

In recent article [PhysRevD.109.055041 (2024)] it has been argued that production of dark photons -- hypothetical massive vectors -- in nuclear reactors via mixing with the visible photons is considerably enhanced (by a factor of 10) due to…

High Energy Physics - Phenomenology · Physics 2025-12-22 S. V. Demidov , D. S. Gorbunov , A. L. Polonski

We discuss a scenario that gravitinos produced non-thermally by an inflaton decay constitute dark matter in the present universe. We find that this scenario is realized for wide ranges of the inflaton mass and the vacuum expectation value.…

High Energy Physics - Phenomenology · Physics 2008-11-26 Fuminobu Takahashi

We present a model where inflation and Dark Matter takes place via a single scalar field phi. Without introducing any new parameters we are able unify inflation and Dark Matter using a scalar field phi that accounts for inflation at an…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 A. de la Macorra

Macroscopic dark matter like nontopological solitons can form either via the fusion and accumulation of free particles or during cosmological phase transitions. Both mechanisms can create dark matter with large masses ranging from TeV to…

High Energy Physics - Phenomenology · Physics 2024-05-16 Nicholas Orlofsky

Dark matter (DM) could couple to particles in the Standard Model (SM) through a light vector mediator. In the limit of small coupling, this portal could be responsible for producing the observed DM abundance through a mechanism known as…

High Energy Physics - Phenomenology · Physics 2019-06-19 Cora Dvorkin , Tongyan Lin , Katelin Schutz

We propose a minimal setup that realises dynamical inflection point inflation, and, using the same field content, generates neutrino masses, a baryon asymmetry of the universe, and dark matter. A dark $SU(2)_D$ gauge sector with a dark…

High Energy Physics - Phenomenology · Physics 2024-02-15 Debasish Borah , Arnab Dasgupta , Daniel Stolarski

We show that warm inflation can be realized within a minimal extension of the Standard Model with three right-handed neutrinos, three complex scalars and a gauged lepton/B-L U(1) symmetry. This simple model can address all the shortcomings…

High Energy Physics - Phenomenology · Physics 2022-01-05 Miguel Levy , João G. Rosa , Luis B. Ventura

We investigate the gravitational particle production from vacuum for a minimally coupled fermionic spectator field during a single-field inflationary phase. We observe that metric perturbations arising from the quantum fluctuations of a…

General Relativity and Quantum Cosmology · Physics 2025-12-04 Alessio Belfiglio , Orlando Luongo

We analyse dark matter (DM) produced somehow in space-time is charged under the hidden $U^{\prime} (1)$ gauge symmetry and interacting with Standard Model (SM) through the scale invariance breaking sector containing dilatons and dark…

High Energy Physics - Phenomenology · Physics 2020-12-11 Gennady Kozlov

We discuss the gravitational creation of superheavy particles $\chi$ in an inflationary scenario with a quartic potential and a non-minimal coupling between the inflaton $\varphi$ and the Ricci curvature: $\xi \varphi^2 R/2$. We show that…

High Energy Physics - Phenomenology · Physics 2020-10-14 E. Babichev , D. Gorbunov , S. Ramazanov , L. Reverberi