Constraints for the X17 boson from compacts objects observations
A. Kanakis-Pegios, V. Petousis, M. Veselsky, Jozef Leja, Ch.C., Moustakidis

TL;DR
This paper explores constraints on the hypothetical X17 boson using neutron star and quark star observations, focusing on its coupling and in-medium effects, to understand its impact on stellar properties within physical limits.
Contribution
It provides new bounds on the X17 boson's coupling and in-medium effects based on astrophysical observations and causality constraints, considering various equations of state.
Findings
X17's effects are mainly constrained by causality limits.
Interaction coupling and in-medium effects significantly influence stellar properties.
Effects are more pronounced in quark stars.
Abstract
We investigate the hypothetical X17 boson on neutron stars and Quark Stars (QSs) using various hadronic Equation of States (EoSs) with phenomenological or microscopic origin. Our aim is to set realistic constraints on its coupling constant and the mass scaling, with respect to causality and various possible upper mass limits and the dimensionless tidal deformability . In particular, we pay special attention on two main phenomenological parameters of the X17, the one is related to the coupling constant that it has with hadrons or quarks and the other with the in-medium effects through the regulator . Both are very crucial concerning the contribution on the total energy density and pressure. In the case of considering the X17 as a carrier of nuclear force in Relativistic Mean Field (RMF) theory, an admixture into vector boson segment was constrained…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · High-pressure geophysics and materials
