Bosnonic dark matter dynamics in neutron star and its imprint on gravitational waves
APA
(2024). Bosnonic dark matter dynamics in neutron star and its imprint on gravitational waves. SciVideos. https://youtu.be/M3PJoOjseZI
MLA
Bosnonic dark matter dynamics in neutron star and its imprint on gravitational waves. SciVideos, Dec. 31, 2024, https://youtu.be/M3PJoOjseZI
BibTex
@misc{ scivideos_ICTS:30710, doi = {}, url = {https://youtu.be/M3PJoOjseZI}, author = {}, keywords = {}, language = {en}, title = {Bosnonic dark matter dynamics in neutron star and its imprint on gravitational waves}, publisher = {}, year = {2024}, month = {dec}, note = {ICTS:30710 see, \url{https://scivideos.org/index.php/icts-tifr/30710}} }
Abstract
Neutron star (NS) can capture dark matter (DM) particles, which can lead to black hole formation destroying the entire star. For bosonic DM, the black hole formation can happen either from a Bose-Einstein condensate (BEC) state or a non-BEC state. The nascent black holes have different initial mass depending on the thermal state of DM particles. As its consequence, the destruction of the host star takes different time for depending on the intial mass of the black hole. This time can be inferred from gravitational wave (GW) signals of a binary system. We show the DM parameter space for BEC formation and discuss its probe via GW detectors.