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Estimate the non-relativistic degeneracy pressure at the center of a 1.4 Msun neutron star (p=1.5x1018 kg/m³) and compare with the estimated pressure at the center of Sirius B. Use Z/A=1 in the n-formula, since this represents now the neutron number density which is approximately 1.

Estimate the non-relativistic degeneracy pressure at the center of a 1.4 Msun neutron star (p=1.5x1018 kg/m³) and compare with the estimated pressure at the center of Sirius B. Use Z/A=1 in the n-formula, since this represents now the neutron number density which is approximately 1.

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Estimate the non-relativistic degeneracy pressure at the center of a 1.4 Msun neutron star (p=1.5x1018 kg/m³) and compare with the estimated pressure at the center of Sirius B. Use Z/A=1 in the n-formula, since this represents now the neutron number density which is approximately 1.
Transcribed Image Text:Estimate the non-relativistic degeneracy pressure at the center of a 1.4 Msun neutron star (p=1.5x1018 kg/m³) and compare with the estimated pressure at the center of Sirius B. Use Z/A=1 in the n-formula, since this represents now the neutron number density which is approximately 1.
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