| Full text | |
| Author(s): |
Lourenco, O.
;
Lenzi, C. H.
;
Frederico, T.
;
Dutra, M.
Total Authors: 4
|
| Document type: | Journal article |
| Source: | PHYSICAL REVIEW D; v. 106, n. 4, p. 9-pg., 2022-08-08. |
| Abstract | |
In this work, we study the outcomes related to dimensionless tidal deformability (A) obtained through a relativistic mean-field (RMF) hadronic model including short-range correlations (SRCs) and dark matter (DM) content [Phys. Rev. D 105, 023008 (2022)]. As a dark particle candidate, we use the lightest neutralino interacting with nucleons through the Higgs boson exchange. In particular, we test the model against the constraints regarding the observation of gravitational waves from the binary neutron star merger event GW170817 provided by the LIGO/Virgo Collaboration (LVC). We show that A decreases as the dark particle Fermi momentum (k(F)(Dm) ) increases. This feature favors the RMF-SRC-DM model used here to satisfy the limits of lambda(1.4) = 190(-120)(+390)(lambda of a 1.4 M-? neutron star), and (sic) = 300(-230)(+420) given by the LVC. We also show that as k(F)(Dm) increases, lambda(1) and lambda 2, namely, the tidal deformabilities of the binary system, are also moved in the direction of the GW170817 observational data. Finally, we verify that the inclusion of DM in the system does not destroy the I-Love relation (correlation between A and the dimensionless moment of inertia, I over bar ). The observational data for I(over bar)(?) equivalent to I(over bar)(M-? ) = 11.10(-2.28)(+3.68), with M-? = 1.338 M(? )is obtained by the RMF-SRC-DM model. (AU) | |
| FAPESP's process: | 20/05238-9 - Different approaches in the strongly interacting matter study |
| Grantee: | Odilon Lourenço da Silva Filho |
| Support Opportunities: | Regular Research Grants |
| FAPESP's process: | 17/05660-0 - Theoretical studies of the structure and reactions of exotic nuclei and many-body systems |
| Grantee: | Brett Vern Carlson |
| Support Opportunities: | Research Projects - Thematic Grants |