All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Probing supernova neutrino boosted dark matter with collective excitations

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A90263%2F25%3A00384533" target="_blank" >RIV/68407700:90263/25:00384533 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1103/xhl3-v17n" target="_blank" >https://doi.org/10.1103/xhl3-v17n</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/xhl3-v17n" target="_blank" >10.1103/xhl3-v17n</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Probing supernova neutrino boosted dark matter with collective excitations

  • Original language description

    We explore the supernova neutrino-boosted dark matter (SN nu BDM) and its direct detection. During core-collapse supernova, an abundance of neutrinos are emitted. These supernova neutrinos can transfer their kinetic energy to the light dark matter via their interactions, and thus are detected in the neutrino and dark matter experiments. Because of the exponential suppression of the high-energy neutrino flux, the kinetic energy carried by a large portion of SN nu BDM falls within the MeV range. We consider a simplified model where dark matter interacts with both electrons and neutrinos through a light mediator. In this case, the enhancement in the scattering rate from the light mediator combined with the excitation of the plasmon resonance in silicon significantly enhances the sensitivity in experiments using low-threshold detectors, such as skipper CCDs, in contrast to conventional neutrino and dark matter direct-detection experiments. We calculate the total scattering rate induced by SN nu BDM and derive exclusion limits from Super-K, XENON1T, SENSEI, and DAMIC-M.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

  • Continuities

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Physical Review D

  • ISSN

    2470-0010

  • e-ISSN

    2470-0029

  • Volume of the periodical

    112

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    13

  • Pages from-to

    "015014-1"-"015014-13"

  • UT code for WoS article

    001543997000006

  • EID of the result in the Scopus database