12–17 Oct 2015
Saha Institute of Nuclear Physics
Asia/Kolkata timezone

Thermonuclear flame propagation on neutron stars

16 Oct 2015, 11:10
45m
Meghnad Saha Auditorium (Saha Institute of Nuclear Physics)

Meghnad Saha Auditorium

Saha Institute of Nuclear Physics

1/AF Bidhannagar, Salt Lake, Sector-1, Kolkata - 700064, India

Speaker

Prof. Sudip Bhattacharyya (TIFR, Mumbai)

Description

Accreted matter accumulated on a low magnetic field neutron star intermittently burns via thermonuclear runaway processes, and gives rise to bursts observed in X-rays. During the rise of the X-ray intensity, the thermonuclear flame spreads to engulf the entire stellar surface. Such flame propagation in extreme environment, which is relevant for several branches of physics, is an interesting field in its own right, and is important to probe the super-dense degenerate matter at stellar cores. I will discuss the theoretical and observational aspects of flame spreading, its importance, and why ASTROSAT will be very useful to advance our knowledge.

Presentation materials