Constructing neutron stars with a gravitational Higgs mechanism

In scalar-tensor theories, spontaneous scalarization is a phase transition that can occur in ultradense environments such as neutron stars. The scalar field develops a non-trivial configuration once the stars exceeds a compactness threshold. We recently pointed out that, if the scalar exhibits some...

Full description

Bibliographic Details
Main Authors: Franchini, Nicola, Coates, Andrew, Sotiriou, Thomas P.
Format: Article
Language:English
Published: American Physical Society 2018
Online Access:https://eprints.nottingham.ac.uk/51107/
_version_ 1848798418154029056
author Franchini, Nicola
Coates, Andrew
Sotiriou, Thomas P.
author_facet Franchini, Nicola
Coates, Andrew
Sotiriou, Thomas P.
author_sort Franchini, Nicola
building Nottingham Research Data Repository
collection Online Access
description In scalar-tensor theories, spontaneous scalarization is a phase transition that can occur in ultradense environments such as neutron stars. The scalar field develops a non-trivial configuration once the stars exceeds a compactness threshold. We recently pointed out that, if the scalar exhibits some additional coupling to matter, it could give rise to significantly different microphysics in these environments. In this work we study, at the non-perturbative level, a toy model in which the photon is given a large mass when spontaneous scalarization occurs. Our results demonstrate clearly the effectiveness of spontaneous scalarization as a Higgs-like mechanism in neutron stars.
first_indexed 2025-11-14T20:19:27Z
format Article
id nottingham-51107
institution University of Nottingham Malaysia Campus
institution_category Local University
language English
last_indexed 2025-11-14T20:19:27Z
publishDate 2018
publisher American Physical Society
recordtype eprints
repository_type Digital Repository
spelling nottingham-511072018-04-13T18:11:36Z https://eprints.nottingham.ac.uk/51107/ Constructing neutron stars with a gravitational Higgs mechanism Franchini, Nicola Coates, Andrew Sotiriou, Thomas P. In scalar-tensor theories, spontaneous scalarization is a phase transition that can occur in ultradense environments such as neutron stars. The scalar field develops a non-trivial configuration once the stars exceeds a compactness threshold. We recently pointed out that, if the scalar exhibits some additional coupling to matter, it could give rise to significantly different microphysics in these environments. In this work we study, at the non-perturbative level, a toy model in which the photon is given a large mass when spontaneous scalarization occurs. Our results demonstrate clearly the effectiveness of spontaneous scalarization as a Higgs-like mechanism in neutron stars. American Physical Society 2018-03-15 Article PeerReviewed application/pdf en https://eprints.nottingham.ac.uk/51107/1/1708.02113%20%281%29.pdf Franchini, Nicola, Coates, Andrew and Sotiriou, Thomas P. (2018) Constructing neutron stars with a gravitational Higgs mechanism. Physical Review D, 97 (6). 064013. ISSN 2470-0010 https://doi.org/10.1103/PhysRevD.97.064013 doi:10.1103/PhysRevD.97.064013 doi:10.1103/PhysRevD.97.064013
spellingShingle Franchini, Nicola
Coates, Andrew
Sotiriou, Thomas P.
Constructing neutron stars with a gravitational Higgs mechanism
title Constructing neutron stars with a gravitational Higgs mechanism
title_full Constructing neutron stars with a gravitational Higgs mechanism
title_fullStr Constructing neutron stars with a gravitational Higgs mechanism
title_full_unstemmed Constructing neutron stars with a gravitational Higgs mechanism
title_short Constructing neutron stars with a gravitational Higgs mechanism
title_sort constructing neutron stars with a gravitational higgs mechanism
url https://eprints.nottingham.ac.uk/51107/
https://eprints.nottingham.ac.uk/51107/
https://eprints.nottingham.ac.uk/51107/