Constraints on Bose-Einstein condensate stars as neutron stars models from new observational data
Adriel Ernesto Rodr\'iguez Concepci\'on, Gretel Quintero Angulo

TL;DR
This paper assesses Bose-Einstein condensate stars as neutron star models using recent observational data, constraining particle interaction parameters and evaluating their compatibility with observed neutron star properties.
Contribution
It introduces constraints on the scattering length of bosons in BECS models based on recent neutron star observations, supporting their viability as neutron star representations.
Findings
Scattering length for BECS compatible with GW170817 data is 4-10 fm.
Stars similar to XMMU J173203.3-344518 are modeled at a~3.1-4 fm.
Heat capacity exceeds neutron star bounds for a>2-5 fm.
Abstract
We evaluate the feasibility of Bose-Einstein condensate stars (BECS) as models for the interior of neutron stars. BECS are compact objects composed of bosons, formed through the spin-parallel pairing of neutrons. Here, we utilize the astronomical data from GW170817, XMMU J173203.3-344518 (the lightest neutron star known), and a novel lower limit on neutron star core heat capacity to scrutinize the compatibility of BECS with these recent observations of neutron stars. Our specific focus is to constrain the values of the scattering length , a parameter determining the strength of particle interactions in the model. Our analysis suggests that if the stars involved in GW170817 were BECSs, the scattering length of their constituent bosons should fall within the to fm range. Additionally, at a scattering length of fm, stars with mass and radius characteristics akin…
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