[HTML][HTML] Feebly-interacting particles: FIPs 2022 workshop report
C Antel, M Battaglieri, J Beacham, C Boehm… - The European Physical …, 2023 - Springer
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
The first three seconds: a review of possible expansion histories of the early universe
R Allahverdi, MA Amin, A Berlin, N Bernal… - arXiv preprint arXiv …, 2020 - arxiv.org
It is commonly assumed that the energy density of the Universe was dominated by radiation
between reheating after inflation and the onset of matter domination 54,000 years later …
between reheating after inflation and the onset of matter domination 54,000 years later …
in the Standard Model at NLO is 3.043
The effective number of relativistic neutrino species is a fundamental probe of the early
Universe, and its measurement represents a key constraint on many scenarios beyond the …
Universe, and its measurement represents a key constraint on many scenarios beyond the …
Precision early universe thermodynamics made simple: Neff and neutrino decoupling in the Standard Model and beyond
ME Abenza - Journal of Cosmology and Astroparticle Physics, 2020 - iopscience.iop.org
Precision measurements of the number of effective relativistic neutrino species and the
primordial element abundances require accurate theoretical predictions for early Universe …
primordial element abundances require accurate theoretical predictions for early Universe …
Cosmological constraints on dark matter interactions with ordinary matter
Dark matter interactions with electrons or protons during the early Universe leave imprints
on the cosmic microwave background and the matter power spectrum, and can be probed …
on the cosmic microwave background and the matter power spectrum, and can be probed …
Maximizing direct detection with highly interactive particle relic dark matter
We estimate the maximum direct detection cross section for sub-GeV dark matter (DM)
scattering off nucleons. For DM masses in the range 10 keV–100 MeV, cross sections …
scattering off nucleons. For DM masses in the range 10 keV–100 MeV, cross sections …
Report of the topical group on particle dark matter for snowmass 2021
J Cooley, T Lin, WH Lippincott, TR Slatyer… - arXiv preprint arXiv …, 2022 - arxiv.org
This report summarizes the findings of the CF1 Topical Subgroup to Snowmass 2021, which
was focused on particle dark matter. One of the most important scientific goals of the next …
was focused on particle dark matter. One of the most important scientific goals of the next …
Dark matter annihilation to neutrinos
CA Argüelles, A Diaz, A Kheirandish… - Reviews of Modern …, 2021 - APS
The annihilation of dark matter into neutrinos over a range of dark matter masses from MeV/c
2 to ZeV/c 2 is reviewed. Thermally produced models of dark matter are expected to self …
2 to ZeV/c 2 is reviewed. Thermally produced models of dark matter are expected to self …
Strong constraints on decay and annihilation of dark matter from heating of gas-rich dwarf galaxies
Gas-rich dwarf galaxies located outside the virial radius of their host are relatively pristine
systems and have ultralow gas cooling rates. This makes them very sensitive to heat …
systems and have ultralow gas cooling rates. This makes them very sensitive to heat …
An extended analysis of heavy neutral leptons during big bang nucleosynthesis
Abstract Heavy Neutral Leptons (HNLs) are strongly motivated by theory due to their
capability of simultaneously explaining the observed phenomena of dark matter, neutrino …
capability of simultaneously explaining the observed phenomena of dark matter, neutrino …