Search results for "lcsh:QC170-197"

showing 4 items of 4 documents

Numerical Hydrodynamics and Magnetohydrodynamics in General Relativity.

2008

This article presents a comprehensive overview of numerical hydrodynamics and magneto-hydrodynamics (MHD) in general relativity. Some significant additions have been incorporated with respect to the previous two versions of this review (2000, 2003), most notably the coverage of general-relativistic MHD, a field in which remarkable activity and progress has occurred in the last few years. Correspondingly, the discussion of astrophysical simulations in general-relativistic hydrodynamics is enlarged to account for recent relevant advances, while those dealing with general-relativistic MHD are amply covered in this review for the first time. The basic outline of this article is nevertheless sim…

PhysicsField (physics)Physics and Astronomy (miscellaneous)General relativityNumerical analysisStructure (category theory)Review Articlelcsh:Atomic physics. Constitution and properties of matterlcsh:QC170-197Relativistic hydrodynamicsMagnetohydrodynamicsTheoretical physicsNumerical relativityGravitational fieldNumerical relativityGravitational collapseHydrodynamicsMagnetohydrodynamicsLiving reviews in relativity
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Numerical Hydrodynamics in General Relativity

2003

The current status of numerical solutions for the equations of ideal general relativistic hydrodynamics is reviewed. With respect to an earlier version of the article the present update provides additional information on numerical schemes and extends the discussion of astrophysical simulations in general relativistic hydrodynamics. Different formulations of the equations are presented, with special mention of conservative and hyperbolic formulations well-adapted to advanced numerical methods. A large sample of available numerical schemes is discussed, paying particular attention to solution procedures based on schemes exploiting the characteristic structure of the equations through lineariz…

PhysicsNumerical RelativityField (physics)Physics and Astronomy (miscellaneous)General relativityNumerical analysisAstrophysics (astro-ph)Structure (category theory)FOS: Physical sciencesReview ArticleGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysicslcsh:Atomic physics. Constitution and properties of matterGeneral Relativity and Quantum Cosmologylcsh:QC170-197Neutron starRiemann hypothesissymbols.namesakeClassical mechanicsGravitational fieldGravitational collapsesymbolsLiving Reviews in Relativity
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Numerical Hydrodynamics in Special Relativity

2003

This review is concerned with a discussion of numerical methods for the solution of the equations of special relativistic hydrodynamics (SRHD). Particular emphasis is put on a comprehensive review of the application of high-resolution shock-capturing methods in SRHD. Results obtained with different numerical SRHD methods are compared, and two astrophysical applications of SRHD flows are discussed. An evaluation of the various numerical methods is given and future developments are analyzed.

PhysicsNumerical RelativityPhysics and Astronomy (miscellaneous)Numerical analysisAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstrophysicsReview Articlelcsh:Atomic physics. Constitution and properties of matterAstrophysicsSpecial relativity (alternative formulations)Cosmologylcsh:QC170-197Numerical relativityTheoretical physicsClassical mechanicsLiving Reviews in Relativity
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First results of the experiment to search for 2β decay of 106Cd with the help of 106CdWO4 crystal scintillators

2011

An experiment to search for 2β processes in 106Cd with the help of 106CdWO4 crystal scintillator (mass of 215 g), enriched in 106Cd up to 66 %, is in progress at the Gran Sasso National Laboratories of the INFN (Italy). After 1320 h of data taking, limits on double beta processes in 106Cd have been established on the level of 1019 − 1020 yr, in particular (all the results at 90 % C.L.): T1/2(0ν2ε) > 3.6 · 1020 yr, T1/2(2νεβ+) > 7.2 · 1019 yr, and T1/2(2ν2β+) > 2.5 · 1020 yr. Resonant 0ν2ε processes have been restricted as T1/2(0ν2K) > 1.4 · 1020 yr and T1/2(0νLK) > 3.2 · 1020 yr. A possible resonant enhancement of the 0ν2ε processes is estimated in the framework of the QRPA approach.

double beta decay106CdCdWO4 crystal scintillator.lcsh:Atomic physics. Constitution and properties of matterlcsh:QC170-197
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