Astronomy and Astrophysics Seminars

Double Neutron Stars: Merger Times, Systemic Velocity, and Travel Distances

by Dr. Jeff Andrews (Niels Bohr Institute, Copenhagen, Denmark)

Tuesday, March 5, 2019 from to (Asia/Kolkata)
at DAA SEMINAR ROOM ( A269 )
TIFR
Description
The formation and evolution of double neutron star (DNS) populations are traditionally studied using binary population synthesis. In this talk, I argue that the basic characteristics of DNSs can be understood using analytic and semi-analytic techniques. In particular, I will demonstrate how different NS natal kick velocity distributions, pre-SN orbital separations, and progenitor He-star masses affect DNS orbital periods, eccentricities, merger times, systemic velocities, and distances travelled by the system before merging. Comparison with the 17 known Milky Way DNSs in the field provides stringent constraints on these distributions.