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The shear modulus of neutron star matter in the free-neutron state

✍ Scribed by P. B. Jones


Publisher
Springer Netherlands
Year
1975
Tongue
English
Weight
444 KB
Volume
38
Category
Article
ISSN
0004-640X

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We address a recent claim that the stability of neutron stars implies a lower bound on the mass of the neutrino. We argue that the result obtained by some previous authors is due to an improper summation of an infraredsensitive series and that a non-perturbative "resummation" of the series yields a