Fundamental physics from black holes, neutron stars and gamma-ray bursts
Remo Ruffini
TL;DR
This paper explores how gamma-ray bursts and supernovae provide new insights into neutron stars, white dwarfs, and fundamental physics, expanding our understanding of astrophysical phenomena and theoretical frameworks.
Contribution
It introduces novel perspectives on the role of GRBs and SNe in studying compact objects and fundamental physics.
Findings
GRBs offer new observational data on neutron stars.
Supernovae reveal insights into white dwarf physics.
Theoretical models are extended to incorporate these phenomena.
Abstract
Gamma-ray bursts (GRBs) and supernovae (SNe) bring new perspectives to the study of neutron stars and white dwarfs, as well as opening new branches of theoretical physics and astrophysics.
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