Bhatia Hazarika Limit
In astrophysics, the Chandrasekhar Limit is the maximum mass of a stable white dwarf star, defined as 1.4 times the mass of the sun, before gravitational collapse occurs. However, when a neutron star escapes to become 2.8 times its solar mass, it reaches what is called its Bhatia Hazarika limit,[1] to become a bigger neutron star or a black hole due to gravitational collapse.[2] It was observed in gravitational wave of GW170817 to have a 2.82 time solar mass. The formula is:
M star = 2 3/2 M sun
As the velocity of the neutron star, along with the rotation increases, gravitational collapse may or may not occur. If it does collapse it converts into a black hole after exceeding the Bhatia Hazarika Limit of 2.8 times solar mass. The formula is described again theoretically and mathematically,[3][4][5] A neutron star smash breaks universe showing 2.8 times solar mass shown in a lecture at Niels Bohr Institute of University of Copenhagen.[6]
A new discovery has been made by LIGO for GW190425 which have 2.8 times solar mass [7] A book Seeing God through Science exploring the science narrates that gravitational collapse occurs at 2.8 solar mass.[8] The complex life of Star cluster also shows 2.8 solar mass for neutron star,[9][10] NASA,[11] the book "The Hundred Greatest Stars",[12] the book "Extreme stars".[13] All exclaimed about the gravitational collapse at 2.8 times of solar mass.
References[edit]
- ↑ https://iopscience.iop.org/article/10.1088/0031-8949/53/1/011
- ↑ https://www.forbes.com/sites/startswithabang/2018/06/13/the-surprising-reason-why-neutron-stars-dont-all-collapse-to-form-black-holes/
- ↑ https://sites.ualberta.ca/~pogosyan/teaching/ASTRO_122/lect19/lecture19.html
- ↑ http://www.aoc.nrao.edu/~smyers/courses/astro12/solution6.html
- ↑ https://www.quora.com/What-would-be-the-effects-of-a-neutron-star-if-one-was-heading-towards-our-solar-system
- ↑ https://www.nbi.ku.dk/english/news/news17/neutron-star-smash-shakes-universe/
- ↑ https://theprint.in/science/scientists-at-ligo-detect-heaviest-binary-neutron-star-merger-ever-known/345640/
- ↑ https://books.google.co.in/books?id=uSSsDwAAQBAJ&pg=PA58&lpg=PA58&dq=neutron+star+with+2.8+times+of+sun&source=bl&ots=voH5rk0jH5&sig=ACfU3U160WBgfCaZs5S0QdX4Xug_L_0Ixw&hl=en&sa=X&ved=2ahUKEwjKpK6suorpAhUmIbcAHWcrDw8Q6AEwEnoECAQQAQ#v=onepage&q=neutron%20star%20with%202.8%20times%20of%20sun&f=false
- ↑ https://books.google.co.in/books?id=nihACQAAQBAJ&pg=PA185&lpg=PA185&dq=neutron+star+with+2.8+times+of+sun&source=bl&ots=qKrlDdLauO&sig=ACfU3U1Jk_s2WEC2keiyrjRho0zuGyP2TQ&hl=en&sa=X&ved=2ahUKEwjKpK6suorpAhUmIbcAHWcrDw8Q6AEwE3oECAMQAQ#v=onepage&q=neutron%20star%20with%202.8%20times%20of%20sun&f=false
- ↑ https://books.google.co.in/books?id=vFqbAgAAQBAJ&pg=PT93&lpg=PT93&dq=neutron+star+with+2.8+times+of+sun&source=bl&ots=AV_3W93il1&sig=ACfU3U0W79uBlCDpakii34Vf-QIrFzcINg&hl=en&sa=X&ved=2ahUKEwiwxNrevorpAhX-73MBHRrKBwA4ChDoATACegQICBAB#v=onepage&q=neutron%20star%20with%202.8%20times%20of%20sun&f=false
- ↑ https://svs.gsfc.nasa.gov/10543
- ↑ https://books.google.co.in/books?id=jmoQBwAAQBAJ&pg=PA33&lpg=PA33&dq=neutron+star+with+2.8+times+of+sun&source=bl&ots=FyAKCZovIY&sig=ACfU3U2d61hDwS2Wk4Ov2wqH-yqD3fftlA&hl=en&sa=X&ved=2ahUKEwiwxNrevorpAhX-73MBHRrKBwA4ChDoATAGegQICRAB#v=onepage&q=neutron%20star%20with%202.8%20times%20of%20sun&f=false
- ↑ https://books.google.co.in/books?id=3kcjvYLh8xIC&pg=PA152&lpg=PA152&dq=neutron+star+with+2.8+times+of+sun&source=bl&ots=q10OzQizIx&sig=ACfU3U2o6V-26xP9ZrY_CBtnEHRNEMLVlg&hl=en&sa=X&ved=2ahUKEwjn3o75xIrpAhXs6nMBHerXBUg4FBDoATABegQIBRAB#v=onepage&q=neutron%20star%20with%202.8%20times%20of%20sun&f=false
This article "Bhatia Hazarika Limit" is from Wikipedia. The list of its authors can be seen in its historical and/or the page Edithistory:Bhatia Hazarika Limit. Articles copied from Draft Namespace on Wikipedia could be seen on the Draft Namespace of Wikipedia and not main one.
