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Relativistic radiative transfer in relativistic plane-parallel flows: Behavior of the Eddington factor

机译:相对论平面平行流中的相对论辐射传递:爱丁顿因子的行为

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Relativisticradiativetransferinarelativisticplanea€“parallelflowwhichisacceleratedfromitsbase,likeanaccretiondiskwind,isnumericallyexaminedunderafullyspecial-relativistictreatment.Wefirstderiverelativisticformalsolutions.Wetheniterativelysolvetherelativistictransferequationforseveralcasessuchasradiativeequilibriumorlocalthermodynamicequilibrium,andobtainspecificintensitiesintheinertialandcomovingframes,aswellasmomentquantitiesandtheEddingtonfactor.Momentquantitiesareratherdifferentineachcase,butthebehavioroftheEddingtonfactorfortheplanea€“parallelcaseisquitesimilarinallcases.TheEddingtonfactorgenerallydependsontheflowvelocityvaswellastheopticaldepth??.Inthecaseofrelativisticplanea€“parallelflows,inanopticallythinregimeof??a‰21,itisslightlylargerthan1/3atveryslowspeed,itbecomessmallerthan1/3atmildlyrelativisticspeed,anditagainincreasesuptounityinthehighlyrelativisticcase.Athighlyrelativisticspeed,ontheotherhand,itbecomeslargerthan1/3eveninanopticallythickregime.WefindtheEddingtonapproximationisfairlygood,exceptfor??a‰21orv/ca‰30.9,althoughthemomentformalismundertheEddingtonapproximationhassomedefectsat$$v/c=1/sqrt{3}$$.
机译:Relativisticradiativetransferinarelativisticplanea€ “parallelflowwhichisacceleratedfromitsbase,likeanaccretiondiskwind,isnumericallyexaminedunderafullyspecial relativistictreatment.Wefirstderiverelativisticformalsolutions.Wetheniterativelysolvetherelativistictransferequationforseveralcasessuchasradiativeequilibriumorlocalthermodynamicequilibrium,andobtainspecificintensitiesintheinertialandcomovingframes,aswellasmomentquantitiesandtheEddingtonfactor.Momentquantitiesareratherdifferentineachcase,butthebehavioroftheEddingtonfactorfortheplanea€” parallelcaseisquitesimilarinallcases.TheEddingtonfactorgenerallydependsontheflowvelocityvaswellastheopticaldepth ??。Inthecaseofrelativisticplanea€“parallelflows,inanopticallythinregimeof ?? 21‰,itisslightlylargerthan1 / 3atveryslowspeed,itbecomessmallerthan1 / 3atmildlyrelativisticspeed,在相对论速度很高的情况下,在光学相对较厚的情况下,它变得大于1 /3。我们发现爱丁顿方法除了?? 21orv / ca≥30.9以外,此方法的效果还不错,尽管在eddington近似下的矩形式主义在$$ v / c = 1 / sqrt {3} $$时有一些缺陷。

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