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Bosonic Dark Matter in White Dwarfs by 202521004 is a document available to read on EtoBox.
This document explores the potential presence of a gravitationally coupled bosonic scalar field in white dwarfs (WDs) to explain discrepancies in mass measurements obtained through electromagnetic and gravitational redshift methods. The authors propose a mixed configuration of a white dwarf and a bosonic star, suggesting that a scalar field component could account for observed mass biases of 5-15%. The study provides a theoretical framework and preliminary constraints on the mass of the scalar field, along
- Author
- 202521004
- Language
- EN