Results 331 to 340 of about 280,623 (343)
Alloying effects on deformation induced microstructure evolution in copper. [PDF]
Sci RepPokharel R +15 more
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False positives in gravitational wave campaigns: the electromagnetic perspective. [PDF]
Philos Trans A Math Phys Eng SciOates S.
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A bright burst from FRB 20200120E in a globular cluster of the nearby galaxy M81. [PDF]
Nat CommunZhang SB +11 more
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Self-Diffusion of Ge in Amorphous Ge x Si1-x Films Studied In Situ by Neutron Reflectometry. [PDF]
ACS Mater AuHüger E, Stahn J, Schmidt H.
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Pulsar glitches from quantum vortex networks. [PDF]
Sci RepMarmorini G, Yasui S, Nitta M.
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Determining whether a phosphatic concretion containing a Cretaceous juvenile crocodylian is a coprolite or a non-fecal concretion. [PDF]
Sci RepAllen RC +4 more
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Enhanced diffusion through multivalency.
Soft MatterBartoš L, Lund M, Vácha R.
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Physical Review Letters, 1993
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
D. G. Ravenhall +2 more
openaire +3 more sources
We calculate properties of neutron star matter at subnuclear densities using an improved nuclear Hamiltonian. Nuclei disappear and the matter becomes uniform at a density of about 0.6n(s), where n(s) of about 0.16/cu fm is the saturation density of nuclear matter. As a consequence, the mass of matter in the crusts of neutron stars is only about half as
D. G. Ravenhall +2 more
openaire +3 more sources
Astrophysics and Cosmology, 2016
Radio pulsars are unique laboratories for a wide range of physics and astrophysics. Understanding how they are created, how they evolve and where we find them in the Galaxy, with or without binary companions, is highly constraining of theories of stellar and binary evolution.
openaire +2 more sources
Radio pulsars are unique laboratories for a wide range of physics and astrophysics. Understanding how they are created, how they evolve and where we find them in the Galaxy, with or without binary companions, is highly constraining of theories of stellar and binary evolution.
openaire +2 more sources