Calibrated Quantification of the Dark-Exciton Reservoir via a k-Space-Folding Probe

Fuente: arXiv
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Autores principales: Dai, Guangyu, Zhang, Xinyu, Gu, Zhaoqi, Zhang, Junyuan, Dou, Lin, Yu, Jiaxin, Gu, Fuxing
Formato: Preprint
Publicado: 2026
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author Dai, Guangyu
Zhang, Xinyu
Gu, Zhaoqi
Zhang, Junyuan
Dou, Lin
Yu, Jiaxin
Gu, Fuxing
author_facet Dai, Guangyu
Zhang, Xinyu
Gu, Zhaoqi
Zhang, Junyuan
Dou, Lin
Yu, Jiaxin
Gu, Fuxing
contents Spin-forbidden dark excitons in monolayer transition metal dichalcogenides constitute a dominant hidden reservoir that governs exciton dynamics and many-body interactions. Yet determining the population distribution within this reservoir remains challenging because detected brightness conflates radiative-rate modification with collection efficiency, obscuring the link between intensity and population. Here we make this inverse problem well posed by calibrating the position- and orientation-resolved detection response. Combining microsphere-enabled k-space folding with Green-tensor quasinormal-mode calibration, we decouple radiative-rate modification from collection efficiency. We extract a room-temperature dark-to-bright population ratio ND/NB = 4.3, consistent with a near-thermalized manifold under continuous-wave excitation. This calibrated population metric provides a quantitative thermodynamic benchmark for the dark reservoir and interaction-driven 2D exciton phases.
format Preprint
id arxiv_https___arxiv_org_abs_2602_01324
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Calibrated Quantification of the Dark-Exciton Reservoir via a k-Space-Folding Probe
Dai, Guangyu
Zhang, Xinyu
Gu, Zhaoqi
Zhang, Junyuan
Dou, Lin
Yu, Jiaxin
Gu, Fuxing
Optics
Spin-forbidden dark excitons in monolayer transition metal dichalcogenides constitute a dominant hidden reservoir that governs exciton dynamics and many-body interactions. Yet determining the population distribution within this reservoir remains challenging because detected brightness conflates radiative-rate modification with collection efficiency, obscuring the link between intensity and population. Here we make this inverse problem well posed by calibrating the position- and orientation-resolved detection response. Combining microsphere-enabled k-space folding with Green-tensor quasinormal-mode calibration, we decouple radiative-rate modification from collection efficiency. We extract a room-temperature dark-to-bright population ratio ND/NB = 4.3, consistent with a near-thermalized manifold under continuous-wave excitation. This calibrated population metric provides a quantitative thermodynamic benchmark for the dark reservoir and interaction-driven 2D exciton phases.
title Calibrated Quantification of the Dark-Exciton Reservoir via a k-Space-Folding Probe
topic Optics
url https://arxiv.org/abs/2602.01324