“Dark Matter” Science-Research, October 2021, Week 2 — summary from Astrophysics Data System, Arxiv and DOAJ

Astrophysics Data System — summary generated by Brevi Assistant

The most exact model to define gravitational interaction is the popular theory of General Relativity. An in-depth picture of the communication of massive black holes and scalar dark matter frameworks is given. We mimic the gravitational characteristics of an enormous item interacting with Ultralight/ Fuzzy Dark Matter, non-relativistic quantum matter defined by the Schrodinger-Poisson formula. We broadly confirm easy price quotes of dynamical rubbing timescales for a black hole at the center of a halo yet see that a large moving factor mass delights meaningful breathing modes in a ULDM soliton. Dark matter detectors employing a Spherical Proportional Counter have demonstrated a single-electron discovery limit and are forecasted to have tiny history rates. We locate that DarkSphere has the potential to improve existing exclusion limitations on DM masses over 4 MeV by as much as 5 orders of magnitude. String theory has been asserted to generate natural unclear dark matter candidates in the type of ultralight axions. We discover that obtaining a significant contribution to the observed dark matter wealth without adjusting the axion initial imbalance angle is not a generic function of 4D string models since it needs a mild offense of the S f≲M_P bound, where S is the instanton activity and f the axion degeneration constant. We review the formation and dissipation of primitive black holes and their feasible contribution to dark matter. Planck-mass relics of PBH dissipations or stupendously big black holes bigger than 10¹² M_⊙ might additionally be an intriguing dark element. The evidence of gravitational wave was first indirectly validated by the orbital duration loss of Hulse-Taylor double star, which agrees well with Einstein’s general relativistic prediction. These light fragments can be promising prospects of fuzzy dark matter which can be penetrated from the above accuracy measurements.

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Arxiv — summary generated by Brevi Assistant

We explore the opportunity of having a fermionic dark matter prospect within U’ models for CE ν NS experiments in light of the newest COHERENT data and the existing and future dark matter straight discovery experiments. We do a complementary investigation utilizing CE ν NS experiments and dark matter straight discovery searches to discover dark matter along with Z^’ boson specification space. We attribute discrepancies between the muon and electron magnetic minutes from the academic predictions to the visibility of an added U^’ supersymmetric model. Dark matter detectors using a Spherical Proportional Counter have shown a single-electron discovery limit and are projected to have tiny history rates. String theory has been claimed to provide surge to all-natural unclear dark matter candidates in the type of ultralight axions. We locate that obtaining a significant contribution to the observed dark matter abundance without tuning the axion first imbalance angle is not a common attribute of 4D string models since it calls for a moderate infraction of the S f≲M_P bound, where S is the instanton action and f the axion decay constant. The evidence of gravitational wave was first indirectly verified by the orbital duration loss of Hulse-Taylor double star, which agrees well with Einstein’s general relativistic prediction. These light fragments can be appealing candidates of fuzzy dark matter which can be probed from the above precision dimensions. We create a supersymmetric variation of gravity with mimetic dark matter. It is then revealed that the system including the supergravity multiplet, the chiral multiplet and the Lagrange multiplier multiplet can break supersymmetry automatically causing a model of a graviton, large gravitino and 2 scalar areas standing for mimetic dark matter.

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DOAJ — summary generated by Brevi Assistant

We examine an intriguing possibility that a solitary field is accountable for both the rising cost of living and dark matter, focusing on the very little set- up where the rising cost of living is driven by a scalar coupling to curvature. On the other hand, thermalized dark matter is sensible, yet the unitarity bound forces the inflaton mass into a narrow window near half the Higgs mass. Abstract The Starobinsky rising cost of living model is among the most basic rising cost of living models that follows the cosmic microwave history monitorings. In the very little configuration, we reveal that it is tough to describe the observed dark matter abundance without conflicting empirical restraints on the cold and the self-interaction of dark matter. We examine the influence of optimum zeros of the Dirac mass matrix on neutrino phenomenology and dark matter within the framework of an inverted seesaw ISS. We extensively research the impact of various appearances of Dirac mass matrix on clean and sterile neutrino dark matter phenomenology. Abstract Very just recently, a Fermilab report of muon g − 2 revealed a 4.2 σ inconsistency in between it and the basic model forecast. In this situation, the singlino-dominated DM and singlet-dominated Higgs bosons can form a remote DM market with χ ~1 0 χ ~1 0 ∼χ_1⁰∼χ_1⁰ → h s A s in charge of the gauged DM relic wealth when m χ ~1 0 m_∼χ_1⁰ ≳ 150 GeV and the Yukawa combining κ is around 0.2 Abstract this paper provides a search for dark matter in the context of a two-Higgs-doublet model along with an extra pseudoscalar arbitrator, a, which decays right into the dark-matter bits. Abstract Pseudo Nambu-Goldstone bosons are attractive dark matter candidates, since they couple to the Standard Model predominantly through acquired interactions. In particular, we show that DM direct detection experiments have come to be conscious of many pNGB DM realisations once loop-induced communications are considered.

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