Work

Magnetically deformed neutron stars and gravitational waves emission

Year: 2025

Type: dissertation

Abstract: The thesis presents a theoretical model that predicts the deformation of neutron stars under the effects of the magnetic field and accretion. A realistic equation of state is considered for the interior of the star. The observational prospects of the model are also studied, in particular for what concerns the possibility of detection of continuous gravitational waves from rotating deformed neutron stars.

Source: Electronic Theses and Dissertations Repository (University of Pisa)

Author: BRUSCO, TOMMASO

Language: English

Topic: Pulsars and Gravitational Waves Research

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

OpenAlex ID: W7081697970

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