Bhatia Hazarika Limit

It is a limit based on Chandrasekhar Limit which is 1.4 times the solar mass for a star to have gravitational collapse for stars such as white dwarfs but the things changes when neutron star escape to form up to twice 2.8 times solar mass it is known as Bhatia Hazarika limit, to become a bigger neutron star or a black hole due to gravitational collapse at the limit when it reaches to 2.8 times solar mass.
The formula is
M <sub> star</sub> = 2 M<sub> sun </sub>
As the velocity of the neutron star along with the rotation increases it may or may not have gravitational collapse, if there is a collapse it converts into black hole after attaining 2.8 times solar mass of Bhatia Hazarika Limit
This formulation is described again theoretically and mathematically, Neutron star smash breaks universe showing 2.8 times solar mass shown in a lecture at Niels Bohr Institute of University of Copenhagen.
A new discovery has been made by LIGO for GW190425 which have 2.8 times solar mass
A book Seeing God through Science exploring the science narrates to strengthen shows that gravitational collapse occurs at 2.8 solar mass. The complex life of Star cluster also shows 2.8 solar mass for neutron star, NASA, the book "The Hundred Greatest Stars", the book "Extreme stars". All exclaimed about the gravitational collapse at 2.8 times of solar mass.
References
Category :Astronomy

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