Search Results - "Dimmelmeier, H"
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3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state
Published in Physical review letters (29-06-2007)“…We present 2D and 3D simulations of the collapse of rotating stellar iron cores in general relativity employing a nuclear equation of state and an approximate…”
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Generic gravitational-wave signals from the collapse of rotating stellar cores
Published in Physical review letters (22-06-2007)“…We perform general relativistic (GR) simulations of stellar core collapse to a protoneutron star, using a microphysical equation of state (EOS) and an…”
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Axisymmetric modes of rotating relativistic stars in the Cowling approximation
Published in Monthly notices of the Royal Astronomical Society (21-08-2001)“…Axisymmetric pulsations of rotating neutron stars can be excited in several scenarios, such as core collapse, crust- and core-quakes or binary mergers, and…”
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Axisymmetric general relativistic simulations of the accretion-induced collapse of white dwarfs
Published in Physical review. D, Particles, fields, gravitation, and cosmology (15-02-2010)Get full text
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Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation
Published in Monthly notices of the Royal Astronomical Society (01-06-2006)“…We study non-linear axisymmetric pulsations of rotating relativistic stars using a general relativistic hydrodynamics code under the assumption of a…”
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Conclusions on severe accident research priorities
Published in Annals of nuclear energy (01-12-2014)“…•Estimation of research priorities related to severe accident phenomena.•Consideration of new topics, partly linked to the severe accidents at…”
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Gravitational Waves from Relativistic Rotational Core Collapse
Published in The Astrophysical journal (20-10-2001)Get full text
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A new multi-dimensional general relativistic neutrino hydrodynamics code for core-collapse supernovae. I. Method and code tests in spherical symmetry
Published 21-04-2010“…We present a new general relativistic (GR) code for hydrodynamic supernova simulations with neutrino transport in spherical and azimuthal symmetry (1D/2D). The…”
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General relativistic simulations of pasive-magneto-rotational core collapse with microphysics
Published 22-03-2007“…This paper presents results from axisymmetric simulations of magneto-rotational stellar core collapse to neutron stars in general relativity using the passive…”
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Relativistic simulations of the phase-transition-induced collapse of neutron stars
Published 05-05-2009“…Mon.Not.Roy.Astron.Soc.394:52-76,2009 An increase in the central density of a neutron star may trigger a phase transition from hadronic matter to deconfined…”
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Axisymmetric simulations of magnetorotational core collapse: Approximate inclusion of general relativistic effects
Published 08-02-2006“…Astronomy and Astrophysics, Volume 457, Issue 1, October I 2006, pp.209-222 We continue our investigations of the magnetorotational collapse of stellar cores…”
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Axisymmetric General Relativistic Simulations of the Accretion-Induced Collapse of White Dwarfs
Published 14-10-2009“…Phys.Rev.D81:044012,2010 (Abridged.) The accretion-induced collapse (AIC) of a white dwarf (WD) may lead to the formation of a protoneutron star and a…”
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3D Collapse of Rotating Stellar Iron Cores in General Relativity including Deleptonization and a Nuclear Equation of State
Published 29-09-2006“…Phys.Rev.Lett.98:261101,2007 We present results from the first 2D and 3D simulations of the collapse of rotating stellar iron cores in general relativity…”
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Exploring the relativistic regime with Newtonian hydrodynamics: An improved effective gravitational potential for supernova simulations
Published 08-02-2005“…Astron.Astrophys. 445 (2006) 273 We investigate the possibility to approximate relativistic effects in hydrodynamical simulations of stellar core collapse and…”
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CFC+: Improved dynamics and gravitational waveforms from relativistic core collapse simulations
Published 23-12-2004“…Core collapse supernovae are a promising source of detectable gravitational waves. Most of the existing (multidimensional) numerical simulations of core…”
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