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Understanding the nature of the Dark Matter (DM) is one of the current challenges in modern astrophysics and cosmology. Knowing the properties of the DM particle would shed light on physics beyond the Standard Model and even provide us with…

Cosmology and Nongalactic Astrophysics · Physics 2018-11-09 Luca Visinelli

Feebly Interacting Massive Particles (FIMPs) are dark matter candidates that never thermalize in the early universe and whose production takes place via decays and/or scatterings of thermal bath particles. If FIMPs interactions with the…

High Energy Physics - Phenomenology · Physics 2021-10-15 Francesco D'Eramo , Alessandro Lenoci

Since 1990's the detection of extremely energetic air showers and precise astronomical measurements have proved that our knowledge about fundamental laws of Nature is far from being complete. These observations have found convincing…

Astrophysics · Physics 2007-05-23 Houri Ziaeepour

It has recently been shown that if the dark matter is in thermal equilibrium with a sector that is highly decoupled from the Standard Model, it can freeze-out with an acceptable relic abundance, even if the dark matter is as heavy as ~1-100…

High Energy Physics - Phenomenology · Physics 2016-12-02 Asher Berlin , Dan Hooper , Gordan Krnjaic

The gravitational interaction is ubiquitous and the effect of gravitational particle production necessarily contributes to the dark matter abundance. A simple candidate of dark matter is a scalar particle, whose only renormalizable…

High Energy Physics - Phenomenology · Physics 2024-11-26 Soichiro Izumine , Kazunori Nakayama

The unitary bound restricts thermal relics to be lighter than $100$ TeV. This work investigates the production of ultraheavy dark matter and WIMPs in the presence of primordial black holes. Firstly, we describe how Hawking evaporation can…

High Energy Physics - Phenomenology · Physics 2024-08-27 Giorgio Arcadi , Manfred Lindner , Jacinto P. Neto , Farinaldo S. Queiroz

The scalar dark matter candidate in a prototypical theory space little Higgs model is investigated. We review all details of the model pertinent to dark matter. We perform a thermal relic density calculation including couplings to the gauge…

High Energy Physics - Phenomenology · Physics 2014-11-17 Andreas Birkedal-Hansen , Jay G. Wacker

We study the post-inflationary dynamics for reheating and freeze-in dark matter in the Higgs-$R^2$ inflation model. Taking the perturbative approach for reheating, we determine the evolution of the temperature for radiation bath produced…

High Energy Physics - Phenomenology · Physics 2022-06-08 Shuntaro Aoki , Hyun Min Lee , Adriana G. Menkara , Kimiko Yamashita

Weakly Interacting Massive Particles (WIMPs) are among the best-motivated dark matter candidates. In the standard scenario where the freeze-out occurs well after the end of inflationary reheating, they are in tension with the severe…

High Energy Physics - Phenomenology · Physics 2022-12-21 Nicolás Bernal , Yong Xu

Weakly interacting massive particles provide a well-motivated framework for dark matter, naturally reproducing the observed relic abundance through thermal freeze-out. A recent claim of an indirect-detection signal from the Galactic halo,…

High Energy Physics - Phenomenology · Physics 2026-04-08 Yasunori Nomura , Tomonori Totani

We show that dark matter could be made of massive gauge bosons whose stability doesn't require to impose by hand any discrete or global symmetry. Stability of gauge bosons can be guaranteed by the custodial symmetry associated to the gauge…

High Energy Physics - Phenomenology · Physics 2010-03-26 Thomas Hambye

One of the simplest extensions of the Standard Model is the Higgs portal extension involving a dark Higgs. Dark sectors that include dark matter candidates, WIMPs, axions, and dark photons, can naturally have this type of interaction, where…

High Energy Physics - Phenomenology · Physics 2025-12-04 Wen Yin

The gravitational production of superheavy dark matter, in the Peebles-Vilenkin quintessential inflation model, is studied in two different scenarios: When the particles, whose decay products reheat the universe after the end of the…

General Relativity and Quantum Cosmology · Physics 2020-04-22 Jaume Haro

We investigate a simple extension of the standard model (SM) in which the dark matter consists of a feebly interacting fermion (FIMP), charged under a new $Z_4$ symmetry, that is produced in the early Universe by the freeze-in mechanism.…

High Energy Physics - Phenomenology · Physics 2023-08-11 Carlos E. Yaguna , Óscar Zapata

Super-weakly interacting massive particles produced in the late decays of weakly interacting massive particles (WIMPs) are generic in large regions of supersymmetric parameter space and other frameworks for physics beyond the standard…

High Energy Physics - Phenomenology · Physics 2013-08-08 Jose A. R. Cembranos , Manoj Kaplinghat

Warm dark matter (WDM) of order keV mass may be able to resolve the disagreement between structure formation in cold dark matter simulations and observations. The detailed properties of WDM will depend upon its energy distribution, in…

High Energy Physics - Phenomenology · Physics 2016-08-31 John McDonald

We investigate the production of dark matter (DM) via a heavy $Z'$ mediator during the post-inflationary reheating epoch. In particular, we study production from three mechanisms which are smoothly connected to one another: WIMP-like…

High Energy Physics - Phenomenology · Physics 2025-12-05 Stephen E. Henrich , Yann Mambrini , Keith A. Olive

Particle creation (or annihilation) mechanisms, described by either quantum field theoretical models, or by the thermodynamics of irreversible processes, play an important role in the evolution of the early Universe, like, for example, in…

General Relativity and Quantum Cosmology · Physics 2022-11-03 T. Harko , K. Asadi , H. Moshafi , H. Sheikhahmadi

Particle production at the end of a first-order electroweak phase transition may be rather generic in theories beyond the standard model. Dark matter may then be abundantly produced by this mechanism if it has a sizable coupling to the…

High Energy Physics - Phenomenology · Physics 2015-06-12 Adam Falkowski , Jose Miguel No

We consider thermal production mechanisms of self-interacting dark matter in models with gauged $Z_3$ symmetry. A complex scalar dark matter is stabilized by the $Z_3$, that is the remnant of a local dark $U(1)_d$. Light dark matter with…

High Energy Physics - Phenomenology · Physics 2017-02-01 Soo-Min Choi , Yoo-Jin Kang , Hyun Min Lee