Skip to content
DraconiticResearch
Search Sources API
190,869 studies31 sourcesUpdated 18 min ago
PreprintCC BY 4.0arXiv

Light and charge yields from nuclear recoils in noble liquids: From sub-keV energies to 1 MeV

Abstract

We present a first-principles study of total quanta and charge recombination in noble liquids, based on a solution of Lindhard's integro-differential equation for atomic motion with electronic straggling and detailed modeling of inter-atomic potentials. We introduce the electronic scaling length ξe as a fundamental parameter related to a physical observable of the system. We study the energy and electric-field dependence of the exciton-to-ion ratio for nuclear recoils based on the Bates-Griffing process and semiclassical atomic interactions. The resulting light and charge yields are expressed through the recombination probability in the Thomas-Imel box model using the calculated parameter ξe and one fitted constant. We compare our model with recent measurements of the electric-field dependence of the box size in LAr and LXe and provide a physical explanation for this behavior. Our model extends to sub-keV energies and provides a consistent description of available data from a few keV to 1 MeV, yielding better overall agreement with existing LAr data than NEST and offering predictions for LXe.

Related

  1. Exothermic nuclear recoils from thermal quasi-pNGB dark matter
    Riasat Sheikh, Takashi Toma, Koji Tsumura
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
  2. Super-Lindhard Ionization from 254 eVnr Nuclear Recoils in Germanium
    A. R. L. Kavner, E. Todd, M. Babicz +11
    arXivPreprintCC BY 4.0Full textApplied physics & instrumentationarXiv
  3. Can Nuclear Recoils and Solar Neutrinos Resolve the Composition of Singlino-Higgsino Dark Matter?
    Jingwei Lian, Jin Min Yang
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  4. Nuclear Recoils from Invisible Neutron-Pair Annihilation and the LZ event
    Junseok Lee, Fuminobu Takahashi, Yu-Dai Tsai
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
  5. High-Energy Nuclear Recoils from Boosted Dark Matter for the LZ 248-keV Event: Beyond the Halo-Dependent High-Velocity Tail
    Haider Alhazmi, Doojin Kim, Kyoungchul Kong +2
    arXivPreprintCC0Full textHigh-energy & particle physicsarXiv
BibTeX
@misc{sarkis2026light,
  title = {{Light and charge yields from nuclear recoils in noble liquids: From sub-keV energies to 1 MeV}},
  author = {Y. Sarkis and Juan Carlos D'Olivo and Alexis Aguilar-Arevalo},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.38718},
  eprint = {2610.38718},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.38718},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Light and charge yields from nuclear recoils in noble liquids: From sub-keV energies to 1 MeV
AU  - Y. Sarkis
AU  - Juan Carlos D'Olivo
AU  - Alexis Aguilar-Arevalo
PY  - 2026
DA  - 2026/10/28
PB  - arXiv
DO  - 10.48550/arxiv.2610.38718
UR  - https://arxiv.org/abs/2610.38718
AB  - We present a first-principles study of total quanta and charge recombination in noble liquids, based on a solution of Lindhard's integro-differential equation for atomic motion with electronic straggling and detailed modeling of inter-atomic potentials. We introduce the electronic scaling length ξ_e as a fundamental parameter related to a physical observable of the system. We study the energy and electric-field dependence of the exciton-to-ion ratio for nuclear recoils based on the Bates-Griffing process and semiclassical atomic interactions. The resulting light and charge yields are expressed through the recombination probability in the Thomas-Imel box model using the calculated parameter ξ_e and one fitted constant. We compare our model with recent measurements of the electric-field dependence of the box size in LAr and LXe and provide a physical explanation for this behavior. Our model extends to sub-keV energies and provides a consistent description of available data from a few keV to 1 MeV, yielding better overall agreement with existing LAr data than NEST and offering predictions for LXe.
ER  -