Author(s): T. S. Wood and R. Hollerbach
Simulations of the magnetic field of a neutron star show that shear stresses induced by the field are strong enough to fracture the star’s crust.
[Phys. Rev. Lett. 114, 191101] Published Tue May 12, 2015
Elu, loodus, teadus ja tehnoloogia
Author(s): T. S. Wood and R. Hollerbach
Simulations of the magnetic field of a neutron star show that shear stresses induced by the field are strong enough to fracture the star’s crust.
[Phys. Rev. Lett. 114, 191101] Published Tue May 12, 2015