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Tuesday, 15 January 2013

Rapid rotation o neutron star

Neutron stars spin very fast, lets fid in what time it completes on revolution.

Formula P_{ns} = P_c(\frac{R_{ns}}{R_c})^2

P_{ns} = period of neutron star

P_c = period of core

R_{ns} = radius of neutron star

R_c = Radius of core


Ans::


Cross-section of neutron star. Densities are in terms of ρ0 the saturation nuclear matter density, where nucleons begin to touch.


                                  














So the radius of the core will be taken as 3Km and radius of neutron star is 17Km, period of core is say 0.000007seconds

$ P_{ns} = 0.0007(\frac{17}{3})^2 = 0.000335sec$

now 
R_c = 0.7Km, R_{ns} = 20Km, P_c=3.6e-6sec

so

$ P_{ns} = 3.6e-6(\frac{20}{0.7})^2 = 0.0029sec$

Now I exagerate:

$R_{ns} = 15.5Km, R_c = 0.06Km, P_c = 0.000000006sec$

so:

P_{ns} = 0.000000006(\frac{15.5}{0.06})^2 = 0.0004sec

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