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Cosmological production of scalar, non-minimally coupled dark matter depends on the specifics of the inflationary model under consideration. We analyze both Starobinsky inflation and a quadratic potential, solve the full background…

General Relativity and Quantum Cosmology · Physics 2026-02-24 Jose A. R. Cembranos , Luis J. Garay , Álvaro Parra-López , Javier Ortega del Río

Z' gauge bosons arise in many particle physics models as mediators between the dark and visible sectors. We exploit dark matter complementarity and derive stringent and robust collider, direct and indirect constraints, as well as limits…

High Energy Physics - Phenomenology · Physics 2015-10-14 Alexandre Alves , Asher Berlin , Stefano Profumo , Farinaldo S. Queiroz

An appealing framework for dark matter is provided by light hidden sectors, below the electroweak scale, feebly coupled to the Standard Model via light mediators. We consider a minimal, predictive model where both the dark matter and the…

High Energy Physics - Phenomenology · Physics 2025-10-31 Ana Luisa Foguel , Renata Zukanovich Funchal , Michele Frigerio

A supercooled phase transition in a nearly conformal dark sector can provide a natural setting for darkogenesis via its out-of-equilibrium dynamics, where a particle-antiparticle number asymmetry in the dark sector can be reprocessed into…

High Energy Physics - Phenomenology · Physics 2025-10-21 Sudhakantha Girmohanta , Yuichiro Nakai , Zhihao Zhang

We study Dark Matter production during first order phase transitions from bubble-plasma collisions. We focus on scenarios where the Dark Matter sector is secluded and its interaction with the visible sector (including the Standard Model)…

High Energy Physics - Phenomenology · Physics 2024-06-19 Aleksandr Azatov , Xander Nagels , Miguel Vanvlasselaer , Wen Yin

We construct exact t Hooft-Polyakov monopole solutions in a non-Hermitian field theory with local non-Abelian SU(2) gauge symmetry and a modified antilinear CPT symmetry. The solutions are obtained in a fourfold Bogomolny-Prasad-Sommerfield…

High Energy Physics - Theory · Physics 2020-08-28 Andreas Fring , Takanobu Taira

Thermal relics lighter than an MeV contribute to the energy density of the universe at the time of nucleosynthesis and recombination. Constraints on extra radiation degrees of freedom typically exclude even the simplest of such dark…

High Energy Physics - Phenomenology · Physics 2019-05-29 Asher Berlin , Nikita Blinov

We combine complementary datasets to constrain dark energy. Using standard Big Bang Nucleosynthesis and the observed abundances of primordial nuclides to put constraints on $\Omega_Q$ at temperatures near $T \sim 1MeV$, we find the strong…

Astrophysics · Physics 2015-06-24 Rachel Bean , Steen H. Hansen , Alessandro Melchiorri

It has recently been shown that a subdominant hidden sector of atomic dark matter in the early universe provides a novel avenue towards resolving the Hubble ($H_0$) tension while maintaining good agreement with Cosmic Microwave Background…

High Energy Physics - Phenomenology · Physics 2022-05-12 Nikita Blinov , Gordan Krnjaic , Shirley Weishi Li

We explore the possibility that the dark matter is a condensate of a very light vector boson. Such a condensate could be produced during inflation, provided the vector mass arises via the Steuckelberg mechanism. We derive bounds on the…

High Energy Physics - Phenomenology · Physics 2012-10-17 Ann E. Nelson , Jakub Scholtz

Scalar dark matter (DM), and axions in particular, have an irreducible abundance of particles produced by freeze-in due to portal interactions with the Standard Model plasma in the early Universe. In addition, vacuum misalignment and other…

High Energy Physics - Phenomenology · Physics 2024-06-05 Wen-Yuan Ai , Ankit Beniwal , Angelo Maggi , David J. E. Marsh

I will begin by reviewing the evidence for Dark Matter in the Universe, as well as the candidates for dark matter. At most 20% of the dark matter in galaxies can be in the form of MACHOs (Massive Compact Halo Objects); the remainder appears…

Astrophysics · Physics 2008-11-26 Katherine Freese

In an earlier paper I proposed a highly symmetric semi-classical initial condition to describe the universe in the period leading up to the electroweak transition and completely determine all cosmology after that. Nothing beyond the…

Cosmology and Nongalactic Astrophysics · Physics 2022-03-25 Daniel Friedan

We propose a new scenario where dark matter belongs to a secluded sector coupled to the Standard Model through energy--momentum tensors. Our model is motivated by constructions where gravity {\it emerges} from a hidden sector, the graviton…

High Energy Physics - Phenomenology · Physics 2021-01-29 Pascal Anastasopoulos , Kunio Kaneta , Yann Mambrini , Mathias Pierre

Freeze-in of multi-component dark sectors is governed not only by the interaction with the thermal plasma, but also by their internal dynamics. Full thermalisation within the dark sector is not guaranteed, raising the question of impact of…

High Energy Physics - Phenomenology · Physics 2026-04-17 Shiuli Chatterjee , Andrzej Hryczuk

We study static magnetic monopoles in the context of varying alpha theories and show that there is a group of models for which the t'Hooft-Polyakov solution is still valid. Nevertheless, in general static magnetic monopole solutions in…

High Energy Physics - Phenomenology · Physics 2014-11-18 J. Menezes , P. P. Avelino , C. Santos

We show that dark matter emerging from late decays (z < 1000) produces a linear power spectrum identical to that of Cold Dark Matter (CDM) on all observationally relavant scales (> 0.1 Mpc), and simultaneously generates observable…

Astrophysics · Physics 2008-11-26 Louis E. Strigari , Manoj Kaplinghat , James S. Bullock

In a previous paper \cite{Khlopov:2007ic}, we showed how the minimal walking technicolor model (WTC) can provide a composite dark matter candidate, by forming bound states between a -2 electrically charged techniparticle and a $^4He^{++}$.…

Astrophysics · Physics 2008-11-26 Maxim Yu. Khlopov , Chris Kouvaris

A multi-component weakly-interacting dark matter scenario is analyzed, where the candidate dark matter states arise from the $SU(2)_{D}\to Z_{3}^{D}\times Z_{2}^{\text{acc}}$ symmetry breaking triggered by a VEV-developing scalar in the…

High Energy Physics - Phenomenology · Physics 2025-05-16 Carlos Alvarado , Alfredo Aranda , Cesar Bonilla , Carlos Ramos Portalatino

Dirac monopoles have been widely studied and searched, though never found. A way out of this impasse is the idea that monopoles are not seen freely because they are confined by their strong magnetic forces forming a monopole-antimonopole…

High Energy Physics - Phenomenology · Physics 2011-07-20 Luis N. Epele , Huner Fanchiotti , Carlos A. Garcia-Canal , Vasiliki A. Mitsou , Vicente Vento