Effective field theory and scalar triplet dark matter
We discuss an extension of the standard model with a real scalar triplet, T, including non-renormalizable operators (NROs) up to d = 6. If T is odd under a Z 2 symmetry, the neutral component of T is a good candidate for the dark matter (DM) of the ...
Carolina Arbeláez +4 more
doaj +4 more sources
Constraints on the mass and self-coupling of ultra-light scalar field dark matter using observational limits on galactic central mass [PDF]
It is well known that Ultra-Light Dark Matter (ULDM), usually scalar fields of mass m ∼ 10-22 eV, can solve some of the outstanding problems of the Cold Dark Matter (CDM) paradigm. Such a scalar field could have non-negligible self-coupling λ.
S. Chakrabarti +3 more
semanticscholar +1 more source
Scalar field dark matter and dark energy: a hybrid model for the dark sector [PDF]
Diverse cosmological and astrophysical observations strongly hint at the presence of dark matter and dark energy in the Universe. One of the main goals of Cosmology is to explain the nature of these two components.
C. van de Bruck +2 more
semanticscholar +1 more source
Core-envelope haloes in scalar field dark matter with repulsive self-interaction: fluid dynamics beyond the de Broglie wavelength [PDF]
Scalar Field Dark Matter (SFDM) comprised of ultralight bosons has attracted great interest as an alternative to standard, collisionless Cold Dark Matter (CDM) because of its novel structure-formation dynamics, described by the coupled Schrödinger ...
Taha Dawoodbhoy +2 more
semanticscholar +1 more source
Constraints on Scalar Field Dark Matter from Colocated Michelson Interferometers. [PDF]
Low-mass (sub-eV) scalar field dark matter may induce apparent oscillations of fundamental constants, resulting in corresponding oscillations of the size and the index of refraction of solids.
L. Aiello +6 more
semanticscholar +1 more source
Quasinormal modes, Hawking radiation and absorption of the massless scalar field for Bardeen black hole surrounded by perfect fluid dark matter [PDF]
We study the quasinormal modes, Hawking radiation and absorption cross-section of the Bardeen black hole surrounded by perfect fluid dark matter for a massless scalar field. Our results show that the oscillation frequency of quasinormal modes is enhanced
Qi Sun, Qian Li, Yu Zhang, Qi-Quan Li
semanticscholar +1 more source
Core-halo mass relation in scalar field dark matter models and its consequences for the formation of supermassive black holes [PDF]
Scalar-field dark matter (SFDM) halos exhibit a core-envelope structure with soliton-like cores and CDM-like envelopes. Simulations without self-interaction (free-field case) report a core-halo mass relation $M_c\propto M_{h}^{\beta}$, with either $\beta=
Luis E. Padilla +4 more
semanticscholar +1 more source
Analytical treatment of small scales matter power spectrum in coupled scalar field (CSF) cosmology [PDF]
In this paper, we reconstruct matter power spectrum of a cosmological model in which coupled scalar field acts as dark energy. The coupled scalar field (CSF) dark energy we propose here is a generalized model of quintessence, k-essence or phantom coupled
Mulki Fargiza A. M., Wulandari Hesti
doaj +1 more source
In recent years, the scalar field dark matter (SFDM), also called ultralight bosonic dark matter, has received considerable attention due to the number of problems it might help to solve.
Jordi Solís-López +4 more
semanticscholar +1 more source
Radiative interactions between new non-Abelian gauge sector and the standard model
We discuss one loop generation of the term connecting gauge fields from a local hidden SU(2)H and the standard model U(1)Y introducing an SU(2)H doublet fermion with non-zero hypercharge and a scalar field in adjoint representation.
Takaaki Nomura, Hiroshi Okada
doaj +1 more source

