Zobrazeno 1 - 9
of 9
pro vyhledávání: '"E. P. T. Liang"'
Autor:
M. P. Haugan, E. P. T. Liang
Publikováno v:
General Relativity and Gravitation. 11:223-226
We investigate the stability of the nakedness of the Weyl singularities against matter perturbations by considering the effects of infalling test matter on the convergence of outgoing null rays. We show that the additional convergence induced by infa
Autor:
E. P. T. Liang
Publikováno v:
Journal of Mathematical Physics. 13:386-393
We consider irrotational perfect fluid solutions of the Einstein equations with an equation of state p = γρ. We define ``velocity‐dominated'' singularities of these solutions, a notion previously introduced for dust models. We demonstrate explici
Autor:
E. P. T. Liang
Publikováno v:
General Relativity and Gravitation. 10:1051-1053
Autor:
E. P. T. Liang
Publikováno v:
AIP Conference Proceedings.
This paper reviews the spectral and temporal constraints on the emission mechanisms of the initial burst and subsequent pulses of the March 5, 1979 γ‐transient. Interpretation of the hard tail above 300 keV as due to inverse comptonization, when c
Autor:
E. P. T. Liang
Publikováno v:
The Astrophysical Journal. 216:206
Shock damping of nonlinear adiabatic fluctuations and entropy production are studied in the context of simple waves in a radiation-dominated Friedmann model. Assuming a power-law spectrum of clumpiness at recombination, we derive the primeval spectru
Autor:
E. P. T. Liang
Publikováno v:
The Astrophysical Journal. 231:L111
Within the framework of unsaturated Compton disk accretion onto a supermassive black hole as a model for power-law active-galactic-nuclei X-ray sources (as opposed to the synchro-Compton model), the hot-inner-disk model of Shapiro, Lightman, and Eard
Autor:
E. P. T. Liang, K. A. Thompson
Publikováno v:
The Astrophysical Journal. 240:271
Autor:
E. P. T. Liang
Publikováno v:
The Astrophysical Journal. 230:325
Autor:
Richard H. Price, E. P. T. Liang
Publikováno v:
The Astrophysical Journal. 218:247
It is plausible that an accretion disk pumps energy into an outer tenuous layer of its atmosphere to form a high-tmeperature corona analogous to the solar corona. General features of such a corona, not specific to any model, are discussed, and order-