Detecting bosonic dark matter with neutron stars

Author(s)

Maity, Tarak Nath ^{[1, 2]} ; Queiroz, Farinaldo S. ^{[3, 4, 5]}

Affiliation

^[1] Inst Phys, Sachivalaya Marg, Bhubaneswar 751005 - India

^[2] Indian Inst Sci, Ctr High Energy Phys, Bangalore 560012, Karnataka - India

^[3] Univ Fed Rio Grande do Norte, Int Inst Phys, Campus Univ, BR-59078970 Natal, RN - Brazil

^[4] Univ Fed Rio Grande do Norte, Dept Fis, BR-59078970 Natal, RN - Brazil

^[5] Millennium Inst Subat Phys High Energy Frontier S, Fernandez Concha 700, Santiago - Chile

• Document type: Journal article
• Source: Physical Review D; v. 104, n. 8 OCT 14 2021.
• Web of Science Citations: 0

Abstract

What if the dark matter-nucleon scattering cross section is too small to be detected by direct detection experiments? It is well known in the literature that some interactions lead to dark matter-nucleon scattering cross sections that can be velocity and momentum suppressed. We show that in the case of bosonic dark matter, neutron star spectroscopy offers a possible detection. Firstly, we discuss the case of scalar dark matter with scalar, pseudoscalar, and vector mediators. Later, we do this exercise for vector dark matter. We show that, depending on the nature of dark matter and the interaction involved, neutron stars can improve the sensitivity on the dark matter-nucleon scattering cross section by orders of magnitude, representing a major step forward in the dark matter siege. (AU)

• FAPESP's process: 16/01343-7 - ICTP South American Institute for Fundamental Research: a regional center for theoretical physics
• Grantee: Nathan Jacob Berkovits
• Support Opportunities: Special Projects