Speaker
Dr
Filippo Anzuini
(Monash University)
Description
The expectation value of the axion field in neutron stars becomes large due to finite density corrections. By comparing our magneto-thermal simulations with available neutron star data, we find new observable effects to constrain the axion parameter space.
Primary author
Dr
Filippo Anzuini
(Monash University)
Co-authors
Prof.
José A. Pons
(Universitat d'Alacant)
Mr
Antonio Gómez-Bañón
(Universitat d'Alacant)
Prof.
Paul D. Lasky
(Monash University)
Dr
Federico Bianchini
(Stanford University)
Prof.
Andrew Melatos
(The University of Melbourne)
