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The cosmological evolution of a scalar field is shaped by Hubble damping. Any non-gravitational couplings of the scalar with the primordial thermal bath generically contribute additional damping. Although rarely considered, such thermal…

High Energy Physics - Phenomenology · Physics 2025-12-08 Abhishek Banerjee , Ngan H. Nguyen , Erwin H. Tanin

Early dark energy solutions to the Hubble tension introduce an additional scalar field which is frozen at early times but becomes dynamical around matter-radiation equality. In order to alleviate the tension, the scalar's share of the total…

High Energy Physics - Phenomenology · Physics 2025-04-01 Marc Kamionkowski , Anubhav Mathur

We present a scalar-driven sterile neutrino production model where the interaction with the ultralight scalar field modifies the oscillation production of sterile neutrinos in the early universe. The model effectively suppresses the…

High Energy Physics - Phenomenology · Physics 2023-09-28 Yuxuan He , Jia Liu , Xiaolin Ma , Xiao-Ping Wang

We consider the propagation of a neutrino in a background composed of a scalar particle and a fermion using a simple model for the coupling of the form $\lambda\bar f_R\nu_L\phi$. In the presence of these interactions there can be damping…

High Energy Physics - Phenomenology · Physics 2019-05-22 José F. Nieves , Sarira Sahu

Sterile neutrinos produced through oscillations are a well motivated dark matter candidate, but recent constraints from observations have ruled out most of the parameter space. We analyze the impact of new interactions on the evolution of…

High Energy Physics - Phenomenology · Physics 2018-01-11 Rasmus S. L. Hansen , Stefan Vogl

We study the damping of an oscillating scalar field in a Friedmann-Robertson-Walker spacetime by perturbative processes, taking into account the finite density effects that interactions with the plasma of decay products have on the damping…

High Energy Physics - Phenomenology · Physics 2014-11-18 Marco Drewes

A first principle derivation is given of the neutrino damping rate in real-time thermal field theory. Starting from the discontinuity of the neutrino self energy at the two loop level, the damping rate can be expressed as integrals over…

High Energy Physics - Theory · Physics 2009-11-07 Eduardo S. Tututi , Manuel Torres , Juan Carlos D'Olivo

We calculate the incoherent resonant and non-resonant scattering production of sterile neutrinos in the early universe. We find ranges of sterile neutrino masses, vacuum mixing angles, and initial lepton numbers which allow these species to…

Astrophysics · Physics 2009-11-06 K. Abazajian , G. M. Fuller , M. Patel

We demonstrate that a scalar field is unable to reverse its direction of motion while continuously exchanging energy with another fluid. If the rate of transfer is modulated by the scalar's acceleration, the field can undergo a rapid…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-15 Fergus Simpson , Raul Jimenez , Carlos Pena-Garay , Licia Verde

We investigate observable cosmological aspects of sterile neutrino dark matter produced via the freeze-in mechanism. The study is performed in a framework that admits many cosmologically interesting variations: high temperature production…

High Energy Physics - Phenomenology · Physics 2017-06-15 Samuel B. Roland , Bibhushan Shakya

We describe two new generation mechanisms for Dark Matter composed of sterile neutrinos with ${\cal O}(1)$ keV mass. The model contains a light scalar field which coherently oscillates in the early Universe and modulates the Majorana mass…

High Energy Physics - Phenomenology · Physics 2019-04-23 F. Bezrukov , A. Chudaykin , D. Gorbunov

Within the Minimal Supersymmetric Standard Model (MSSM), LHC bounds suggest that scalar superpartner masses are far above the electroweak scale. Given a high superpartner mass, nonthermal dark matter is a viable alternative to WIMP dark…

High Energy Physics - Phenomenology · Physics 2014-02-05 Richard Easther , Richard Galvez , Ogan Ozsoy , Scott Watson

We consider ultralight scalar dark matter that couples to right-handed neutrinos. Due to the high density of neutrinos in the early universe, the background neutrino density dominates the dynamics of the scalar field, and qualitatively…

High Energy Physics - Phenomenology · Physics 2025-02-05 Ryan Plestid , Sophia Tevosyan

The lightest supersymmetric particle, most likely the neutralino, might account for a large fraction of dark matter in the Universe. We show that the primordial spectrum of density fluctuations in neutralino cold dark matter (CDM) has a…

Astrophysics · Physics 2008-11-26 Stefan Hofmann , Dominik J. Schwarz , Horst Stoecker

Small Recent theories have proposed a variety of massive particles, like the moduli, whose abundance or decay endangers standard cosmological results. To dilute them, thermal inflation has been proposed, with its own massive scalar flaton…

High Energy Physics - Phenomenology · Physics 2016-09-06 Paramita Adhya , D. Rai Chaudhuri

Sterile neutrino dark matter is expected to suppress structure formation at small astrophysical scales. The details of the suppression depend on the sterile neutrino production mechanism in the early universe. In this proceeding, we focus…

Cosmology and Nongalactic Astrophysics · Physics 2017-04-07 Aurel Schneider

We consider the decoherence effects in the propagation of neutrinos in a background composed of a scalar particle and a fermion due to the non-forward neutrino scattering processes. Using a simple model for the coupling of the form $\bar…

High Energy Physics - Phenomenology · Physics 2020-01-16 Jose F. Nieves , Sarira Sahu

We present a detailed study of the production of dark matter in the form of a sterile neutrino via freeze-in from decays of heavy right-handed neutrinos. Our treatment accounts for thermal effects in the effective couplings, generated via…

High Energy Physics - Phenomenology · Physics 2025-10-02 A. Abada , G. Arcadi , M. Lucente , G. Piazza , S. Rosauro-Alcaraz

The LSND and MiniBooNE results as well as the reactor and Gallium anomalies seem to indicate the presence of a sterile neutrino with a mass of $\sim 1$ eV mixed with active neutrinos. Such sterile neutrino can be produced in the early…

High Energy Physics - Phenomenology · Physics 2020-05-01 Yasaman Farzan

Flavor transitions of Neutrinos with a nonstandard interaction are studied. A scalar field is conformally coupled to matter and neutrinos. This interaction alters the neutrino effective mass and its wavefunction leading to a damping factor,…

High Energy Physics - Phenomenology · Physics 2021-05-25 H. Mohseni Sadjadi , H. Yazdani Ahmadabadi
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