# Black Hole Evaporation Driven by Non-Thermal Squeezing Through SNS and CSNS Dynamics

Source: [Black Hole Evaporation Driven by Non-Thermal Squeezing Through SNS and CSNS Dynamics](<https://www.sota2.com/research/paper/694cc4ee53fdd5c36173a703>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-12-26T05:00:05.119Z

Authors: Dhwani Gangal, K. K. Venkataratnam

Published: 2025-12-24T07:19:09.000Z

## Abstract

In this work, we present a comprehensive semiclassical analysis of black hole radiation in a spatially flat FRW Universe for two fundamental nonclassical states: the Squeezed Number State (SNS) and the Coherent Squeezed Number State (CSNS). Unlike thermally modified earlier studies, SNS and CSNS constitute fully non-thermal, number-state-dependent quantum configurations. By embedding these states within the framework of semiclassical theory of gravity, we derive state-resolved expressions for the Hawking temperature, entropy variation, and corresponding mass loss of an evaporating black hole. The influence of the squeezing parameter $\\rho$ and number state parameter $n$ on Hawking emission is examined through a series of analytical results supported by twelve detailed plots. The analysis reveals that the Hawking temperature exhibits monotonic growth with increasing $\\rho$ and $n$, thereby elevating the effective temperature experienced at the black hole horizon. The entropy variations $\\Delta \\mathbb{S}\_{\\mathrm{SNS}}$ and $\\Delta \\mathbb{S}\_{\\mathrm{CSNS}}$ show strong nonlinear enhancement, especially at moderate and large squeezing values. Overall, the study extends earlier thermal squeezed-state approaches to a fully number-state-resolved framework, highlighting the sensitivity of Hawking emission to nonclassical quantum configurations. These findings contribute a new perspective on gravitational particle creation in cosmological settings.

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## Original sources and implementation

[Original paper](<https://arxiv.org/abs/2512.21014>)

[PDF](<https://arxiv.org/pdf/2512.21014.pdf>)