New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Boukhtouchen, Yilda, Bramante, Joseph, Buchanan, Andrew, Hayes, Alexander, Leybourne, Matthew, McIntosh, Jennika, Ray, Anupam, Shugar, Aaron
Format: Preprint
Publié: 2026
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866914623801786368
author Boukhtouchen, Yilda
Bramante, Joseph
Buchanan, Andrew
Hayes, Alexander
Leybourne, Matthew
McIntosh, Jennika
Ray, Anupam
Shugar, Aaron
author_facet Boukhtouchen, Yilda
Bramante, Joseph
Buchanan, Andrew
Hayes, Alexander
Leybourne, Matthew
McIntosh, Jennika
Ray, Anupam
Shugar, Aaron
contents Muscovite mica is a translucent, layered silicate mineral whose basal cleavage, low radiogenic background, gigayear exposures, and demonstrated track retention over geological timescales make it a compelling target for rare particle searches. In this work, we develop a new framework for detecting heavy composite dark matter using muscovite mica as a paleodetector. We model melt track formation by heavy composite dark matter transiting through mica using a Sedov-Taylor thermal spike formalism, and validate the sub-micron regime with SRIM/TRIM simulations of nuclear recoil cascades, which also calibrate the phonon efficiency governing local energy deposition. We demonstrate a novel readout method using rapid X-ray fluorescence mapping with a copper backing contrast technique, capable of identifying micron-scale damage features in cleaved mica sheets over macroscopic scan areas, and calibrate the minimum detectable track size using laser-ablated defect regions. We present projected sensitivities for opaque and diffuse composite dark matter, including a sub-melt hole-channel detection mode for large composites substantially attenuated by overburden. We also revisit prior dark matter exclusions from etched mica searches, identifying shortcomings that compromise the robustness of these constraints.
format Preprint
id arxiv_https___arxiv_org_abs_2606_02579
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica
Boukhtouchen, Yilda
Bramante, Joseph
Buchanan, Andrew
Hayes, Alexander
Leybourne, Matthew
McIntosh, Jennika
Ray, Anupam
Shugar, Aaron
High Energy Physics - Phenomenology
High Energy Physics - Experiment
Muscovite mica is a translucent, layered silicate mineral whose basal cleavage, low radiogenic background, gigayear exposures, and demonstrated track retention over geological timescales make it a compelling target for rare particle searches. In this work, we develop a new framework for detecting heavy composite dark matter using muscovite mica as a paleodetector. We model melt track formation by heavy composite dark matter transiting through mica using a Sedov-Taylor thermal spike formalism, and validate the sub-micron regime with SRIM/TRIM simulations of nuclear recoil cascades, which also calibrate the phonon efficiency governing local energy deposition. We demonstrate a novel readout method using rapid X-ray fluorescence mapping with a copper backing contrast technique, capable of identifying micron-scale damage features in cleaved mica sheets over macroscopic scan areas, and calibrate the minimum detectable track size using laser-ablated defect regions. We present projected sensitivities for opaque and diffuse composite dark matter, including a sub-melt hole-channel detection mode for large composites substantially attenuated by overburden. We also revisit prior dark matter exclusions from etched mica searches, identifying shortcomings that compromise the robustness of these constraints.
title New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica
topic High Energy Physics - Phenomenology
High Energy Physics - Experiment
url https://arxiv.org/abs/2606.02579