activity
19992002
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astro-ph2002

A Hall--Drift Induced Magnetic Field Instability

M. Rheinhardt, U. Geppert

In the presence of a strong magnetic field and under conditions as realized in the crust and the superfluid core of neutron stars the Hall--drift dominates the field evolution. We…

astro-ph2001

Neutron star cooling in transiently accreting low mass binaries: a new tool for probing nuclear matter

Andrea Possenti, Monica Colpi, Dany Page +1

We explore, using an exact cooling code, the thermal evolution of a neutron star undergoing episodes of intense accretion, alternated by long periods of quiescence (e.g. Soft X-Ray…

astro-ph1999

Turbulent dynamo action in the high-conductivity limit: a hidden dynamo

K. -H. Raedler, U. Geppert

The paper deals with a simple spherical mean-field dynamo model of -type in the case of high electrical conductivity. A spherically symmetric distribution of turbulent motions…

astro-ph1999

Recycling NSs to ultrashort periods: a statistical analysis of their evolution in the "magnetic moment vs period" plane

Andrea Possenti, Monica Colpi, Ulrich Geppert +2

We investigate the statistical evolution of magnetic neutron stars recycled in Low Mass Binary (LMB) systems, simulating synthetic populations. Irrespective to the details of the p…

astro-ph1999

Magneto-rotational and thermal evolution of magnetars with crustal magnetic fields

U. Geppert, D. Page, M. Colpi +1

Soft Gamma-ray Repeaters (SGRs) and Anomalous X-ray Pulsars (AXPs) are interpreted as young highly magnetized neutron stars (NSs). Their X-ray luminosity in quiescence, exceeding 1…