Pith. sign in

REVIEW 17 cited by

Freezing-in hadrophilic dark matter at low reheating temperatures

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2210.15653 v2 pith:LWFUIFTY submitted 2022-10-27 hep-ph

Freezing-in hadrophilic dark matter at low reheating temperatures

classification hep-ph
keywords darkmatterreheatingcrosshadrophilicdetectiondirectexperiments
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

If the reheating temperature at the end of inflation is low, of order 10 MeV, then dark matter produced through ultraviolet freeze-in has a large direct detection cross section. We study such a scenario in which dark matter is hadrophilic. This leads to dark matter-nucleon scattering cross sections of interest for near-future experiments for dark matter masses in the range of 100 keV-100 MeV. We explore how these predictions vary if reheating is non-instantaneous.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 17 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Leptogenesis and Low Reheating Temperatures

    hep-ph 2026-07 conditional novelty 7.0

    Standard non-thermal leptogenesis works at arbitrarily low reheating temperatures above the BBN bound when the inflaton potential has a quartic minimum (k≥4), because the inflaton's evolving mass kinematically shuts o...

  2. Kaon Portal to Freeze-in Dark Matter

    hep-ph 2026-05 unverdicted novelty 7.0

    Freeze-in dark matter produced by kaons in low-reheating cosmologies requires larger couplings at lower reheating temperatures, directly linking the relic density to observable rates in rare kaon decay experiments.

  3. Dark matter energy exchange in stars orbiting supermassive black holes

    hep-ph 2026-07 conditional novelty 6.0

    Orbit-averaged elastic DM scattering in S4714 reaches stellar luminosity at σ_χp ∼ 10^{-36} cm² (MeV–GeV) and σ_χe ∼ 5×10^{-38} cm² (sub-MeV) for a spiked profile.

  4. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 6.0

    MobileEgo Anywhere releases an open mobile app, processing pipeline, and 200-hour dataset for long-horizon egocentric data collection on commodity hardware to support vision-language-action model training.

  5. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 conditional novelty 6.0

    Kaon-driven freeze-in of light dark matter at low reheating temperatures requires couplings large enough that NA62, KOTO, and KOTO II can probe the same operator.

  6. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 6.0

    MobileEgo Anywhere supplies an open mobile app, 200-hour long-form egocentric dataset, and processing pipeline that enables collection of persistent-state egocentric trajectories on commodity hardware for VLA and foun...

  7. Dark matter energy exchange in stars orbiting supermassive black holes

    hep-ph 2026-07 unverdicted novelty 5.0

    Orbit-averaged DM energy exchange for S4714 reaches stellar luminosity at σ_χp ~ 10^{-36} cm² (MeV-GeV) and σ_χe ~ 5×10^{-38} cm² (sub-MeV) for spiked DM profiles.

  8. Probing Inelastic Dark Matter via Cosmic-Ray Upscattering in NGC 1068

    hep-ph 2026-06 unverdicted novelty 5.0

    Constraints on sub-GeV inelastic dark matter are derived from cosmic-ray cooling in NGC 1068 by including elastic and deep inelastic scattering in a vector-portal model.

  9. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 5.0

    MobileEgo Anywhere provides an open infrastructure and 200-hour dataset for collecting long-horizon egocentric trajectories on commodity phones to support VLA model training.

  10. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 5.0

    An open framework with a free smartphone app, STERA pipeline, and 200-hour dataset enables hour-plus egocentric data collection on commodity hardware and demonstrates utility by lowering VLA action-prediction error af...

  11. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 5.0

    MobileEgo Anywhere releases an open-source smartphone app, 200-hour egocentric dataset with persistent tracking, and pipeline to enable long-horizon data collection for VLA and foundation model research on commodity hardware.

  12. New benchmarks for direct detection of freeze-in dark matter in vector portal models

    hep-ph 2026-03 unverdicted novelty 5.0

    Freeze-in at low reheating temperatures allows MeV-scale dark matter in vector portal models to be probed by future direct detection experiments in nuclear recoils for 50-500 MeV masses and via enhanced solar neutrino...

  13. Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production

    hep-ph 2025-11 unverdicted novelty 5.0

    A dark U(1)_D model with dark Higgs inflation and low reheating allows dark photon dark matter to achieve the observed relic density for a wider range of couplings, with inflation predictions matching Planck, BICEP/Ke...

  14. MobileEgo Anywhere: Open Infrastructure for long horizon egocentric data on commodity hardware

    cs.CV 2026-05 unverdicted novelty 4.0

    MobileEgo Anywhere releases a 200-hour long-form egocentric dataset with persistent state tracking plus the STERA open infrastructure and processing pipeline to convert commodity mobile captures into training-ready fo...

  15. Thermal effects on Dark Matter production during cosmic reheating

    hep-ph 2026-04 unverdicted novelty 4.0

    Thermal corrections to reheating and freeze-in DM production rates are generally small in the computable regime but can be large in constructed counter-examples.

  16. Seasons of Dark Matter Freeze-In Shaped by the Weather of the Early Universe

    hep-ph 2025-11 unverdicted novelty 4.0

    Variations in pre-nucleosynthesis cosmology produce distinct seasons in the phase-space distribution of freeze-in dark matter, directly affecting its warmness and mass bounds.

  17. Neutron stars as thermometers for reheating induced dipole dark matter

    hep-ph 2026-07 unverdicted novelty 3.0

    Dipole dark matter produced by freeze-out or freeze-in, including entropy dilution from reheating, can be probed via neutron star heating due to momentum-dependent electromagnetic interactions.