Magnetically deformed neutron stars and gravitational waves emission

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.

Publication Details

Journal: Electronic Theses and Dissertations Repository (University of Pisa)
Published: 2025-07-12
Primary Topic: Geochemistry and Geologic Mapping
Type: article
Field-Weighted Citation Impact: 0.00

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article

Magnetically deformed neutron stars and gravitational waves emission

Jul 12, 2025

Electronic Theses and Dissertations Repository (University of Pisa)

Geochemistry and Geologic Mapping

article

Magnetically deformed neutron stars and gravitational waves emission

July 12, 2025article en

Abstract

Electronic Theses and Dissertations Repository (University of Pisa)

Openalex Percentile: Top 41%

Geochemistry and Geologic Mapping

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Magnetically deformed neutron stars and gravitational waves emission · Electronic Theses and Dissertations Repository (University of Pisa) (2025) | TGRS Research Map | TGRS