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Questions related from Bharat Kumar
For non-relativistic limit, we should expect that our usual intuition regarding the accelerating charges would hold, and a falling charge should radiate with an acceleration. On the other hand,...
10 July 2016 4,464 29 View
In the degenerate interiors of neutron stars, the equation of state is usually just density (and composition) dependent. You can express the pressure as a polytropic law of the form P∝ρα, where ρ...
15 December 2015 4,064 8 View
We know that the equilibrium condition for neutron star. But I do not know in the case of hyperon star. Is it same or not?
26 November 2015 3,390 1 View
The astrophysical rapid proton capture and rapid neutron capture processes, which are responsible for the generation of many heavy elements, operate veryclose to the drip lines; hence, the...
25 June 2015 3,758 1 View
The phenomena of the deformation was first suggested by Pauli that the hyperfine structure of atomic and molecular energy levels comes from the electromagnetic interaction with nonspherical atomic...
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