Wednesday Colloquia
Do fast-spinning neutron stars emit elusive continuous gravitational waves?
by Prof. Sudip Bhattacharyya (DAA, TIFR)
Wednesday, April 11, 2018
from
to
(Asia/Kolkata)
at Lecture Theatre ( AG-66 )
at Lecture Theatre ( AG-66 )
TIFR
Description |
A neutron star, which has a sun's worth of material crammed into a sphere of the size of a city, is useful to study some extreme aspects of nature. A fast-spinning neutron star, known as a millisecond pulsar, can typically spin several hundred times in a second. A non-symmetric distortion of such a pulsar, which is not along its spin axis, can generate continuous gravitational waves. Such continuous waves, which have not been detected so far, could provide a wealth of information about neutron stars, and be an excellent tool to probe fundamental aspects of gravitational physics. I will discuss how observations of millisecond pulsars in the traditional electromagnetic wave bands, combined with theoretical calculations, can indicate gravitational wave emission from these pulsars. |