Boosted Neutrinos and Relativistic Dark Particles as Messengers from Reheating
arXiv:2007.15006 · doi:10.1088/1475-7516/2021/02/044
Abstract
Usually information from early eras such as reheating is hard to come by. In this paper we argue that, given the right circumstances, right-handed sterile neutrinos decaying to left-handed active ones at relatively late times can carry information from reheating by propagating freely over the thermal history. For not too small mixing angles, suitable right-handed neutrino masses are around (MeV-GeV). We identify the typical spectra and argue that they provide information on the ratio of the inflaton mass to the reheating temperature. This primordial neutrino signal can be strong enough that it can be detected in IceCube. More speculatively, for a reheating temperature and inflaton mass satisfying , and GeV they may even explain the observed PeV events. Also more general relativistic dark particles can play the role of such messengers, potentially not only allowing for the PeV events but also alleviating the -tension .
38pages, 7figures
References in corpus (22)
- Results from a search for dark matter in the complete LUX exposure
- Dark Matter Results from First 98.7-day Data of PandaX-II Experiment
- CMB-S4 Science Book, First Edition
- Theory and Numerics of Gravitational Waves from Preheating after Inflation
- How to find neutral leptons of the nuMSM?
- A Gravitational Wave Background from Reheating after Hybrid Inflation
- Dark Matter Search Results from the PICO-2L CF Bubble Chamber
- Cosmological constraints on exotic injection of electromagnetic energy
- The LUX-ZEPLIN (LZ) Experiment
- Dark Radiation in LARGE Volume Models
- Gravitational perturbations from oscillons and transients after inflation
- The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part II: Properties of the Atmospheric and Astrophysical Neutrino Flux
- Boosted Dark Matter in IceCube and at the Galactic Center
- Boosted Dark Matter Interpretation of the XENON1T Excess
- The Art of Lattice and Gravity Waves from Preheating
- Search for heavy neutral lepton production in decays to positrons
- Dark Matter and the XENON1T electron recoil excess
- Neutrinoful Universe
- Monochromatic neutrinos generated by dark matter and the see-saw mechanism
- Search for new physics in the monophoton final state in proton-proton collisions at sqrt(s) = 13 TeV
- Constraints on electron-scattering interpretation of XENON1T excess
- Gravitational Waves from Axion Monodromy
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- Indirect Detection of eV Dark Matter via Infrared Spectroscopy
- The Spectrum of Dark Radiation as a Probe of Reheating
- An Analytic Approach to Light Dark Matter Propagation
- High Energy Sphalerons for Baryogenesis at Low Temperatures
- Phenomenology of CP-even ALP
- Probing a light dark sector at future lepton colliders via invisible decays of the SM-like and dark Higgs bosons
- Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events
- Precise Capture Rates of Cosmic Neutrinos and Their Implications on Cosmology
- Shining ALP Dark Radiation
- Signatures of afterglows from light dark matter boosted by supernova neutrinos in current and future large underground detectors
- Dark Fluxes from Accreting Black Holes and Direct Detections
- Directional direct detection of light dark matter up-scattered by cosmic rays from direction of the Galactic center
- Hidden Photon and Axion Dark Matter from Symmetry Breaking
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- Investigating the collinear splitting effects of boosted dark matter at neutrino detectors
- On the reactions involving neutrinos and hidden mass particles in hypercolor model
- LHAASO Galactic Plane -rays Strongly Constrain Heavy Dark Matter
- Primordial high energy neutrinos: theoretical/observational constraints and sharp spectral features