D. Christodoulou, The Formation of Black Holes in General Relativity, EMS Monographs in Mathematics, European Mathematical Society (EMS), Zu¨rich, 2009.D. Christodoulou, "The formation of black holes in general relativity" (Monographs in Mathematics, European Mathematical Soc. Publishing House, ...
Although micro black holes are tiny, they still can be detected.D. People are not sure about the origins of SMBH and micro black holes.)4. Which of the following is the best title for the passage?A. The formation of black holesB. The development of black holesC. The introduction to ...
Several theories have been proposed to describe the formation of black hole seeds in the early Universe and to explain the emergence of very massive black holes observed in the first thousand million years after the Big Bang1,2,3. Models consider different seeding and accretion scenarios4,5,6,...
In this paper, we will explore the formation of black holes, their properties, and their effects on the universe. Introduction:The concept of a black hole was first introduced by John Michell in 1783, but it wasn't until the 20th century that they were accepted as a real astronomical ...
of the black hole, respectively. The formation of black hole shadow is due essentially to the deflection of light in the strong gravity field [7,8,9,10], its image may carry some valuable information of the geometry around the black hole. Consequently, the investigation of the black hole ...
In contrast, we infer a wide range in star formation properties and host morphologies for the sample, from disk-dominated to elliptical galaxies. Nearly one-quarter have highly disturbed morphologies indicative of ongoing mergers. Unlike the BHs, which are apparently experiencing significant growth, ...
The x‐ray spectra of accreting black holes in x‐ray binaries show anultrasoft/ultrahardspectral combination that is distinct amongst the galactic populat... NE White,Paradijs - 《Astrophysical Journal》 被引量: 95发表: 1996年 On the formation of low-mass black holes in massive binary stars...
Formation of a Black Hole in the Dark.We show that the black hole in the x-ray binary Cygnus X-1 was formed in situ and did not receive an energetic trigger from a nearby supernova. The progenitor of the black hole had an initial mass greater than 40 solar masses, and during the ...
Sakharov, "Formation of black holes in first order phase transitions ", hep-ph/980734; M.Yu. Khlopov, R.V. Konoplich, S.G. Rubin, A.S. Sakharov, "First order phase transitions as a source of black holes in the early universe ", Grav.Cosmol. 2 (1999) S1, hep-ph/9912422. S....
In this note we suggest that high-mass black holes; i.e., black holes of several solar masses, can be formed in binaries with low-mass main-sequence companions, provided that the hydrogen envelope of the massive star is removed in common envelope evoluti