Zobrazeno 1 - 10
of 724
pro vyhledávání: '"MILLER, J. C."'
This paper presents a novel extension of the edge-based compartmental model for epidemics with arbitrary distributions of transmission and recovery times. Using the message passing approach we also derive a new pairwise-like model for epidemics with
Externí odkaz:
http://arxiv.org/abs/1611.04030
Autor:
Karino, S., Miller, J. C.
Periodic pulsations have been found in emission from the ultra-luminous X-ray source (ULX) M82 X-2, strongly suggesting that the emitter is a rotating neutron star rather than a black hole. However, the radiation mechanisms and accretion mode involve
Externí odkaz:
http://arxiv.org/abs/1605.05723
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
MNRAS 435, 2633-2649 (2013)
Millisecond pulsars are rather weakly-magnetized neutron stars which are thought to have been spun up by disc accretion, with magnetic linkage between the star and the disc playing a key role. Their spin history depends sensitively on details of the
Externí odkaz:
http://arxiv.org/abs/1310.7012
Astrophysical plasmas in accretion discs are usually treated in the framework of fluid or MHD approaches but there are some situations where these treatments become inadequate and one needs to revert to the more fundamental underlying kinetic theory.
Externí odkaz:
http://arxiv.org/abs/1201.1838
The physical mechanism responsible for driving accretion flows in astrophysical accretion disks is commonly thought to be related to the development of plasma instabilities and turbulence. A key question is therefore the determination of consistent e
Externí odkaz:
http://arxiv.org/abs/1201.1839
Autor:
Naso, L., Miller, J. C.
Publikováno v:
A&A 531, A163 (2011)
Millisecond pulsars are believed to be old pulsars spun up by a surrounding accretion disc. Magnetic fields are thought to play a leading role in this, both by determining the location of the inner edge of the disc and by exerting an additional torqu
Externí odkaz:
http://arxiv.org/abs/1012.3194
Publikováno v:
Mon.Not.Roy.Astron.Soc. 404:L35-L39,2010
We present results for neutron star models constructed with a new equation of state for nuclear matter at zero temperature. The ground state is computed using the Auxiliary Field Diffusion Monte Carlo (AFDMC) technique, with nucleons interacting via
Externí odkaz:
http://arxiv.org/abs/0909.3487
Autor:
Naso, L., Miller, J. C.
Publikováno v:
Astron.Astrophys. 521: A31,2010
We report results from calculations investigating stationary magnetic field configurations in accretion discs around magnetised neutron stars. Our strategy is to start with a very simple model and then progressively improve it providing complementary
Externí odkaz:
http://arxiv.org/abs/0906.5082