in the black hole;Information model of a black hole;Characteristics of the emission and absorption of usual substance by a black hole describes the information model of a black hole;The information paradox;A simple explanation of the information paradox by the information model of a black hole.do...
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,...
The novel perspective advanced here is that if BH entropy counts the number of accessible physical states in a quantum black hole, then the paradox can be seen as an instance of the fundamental problem of statistical mechanics. We suggest a specific analogy to the increase of the entropy in ...
the two black holes have a joint mass that is 28billiontimes larger than that ofthe sun, making this the most massive black hole binary ever seen. Not only that, but the binary components of this system are the closest in a supermassive black hole pair, separated by just 24 light-years....
Based on a new explanation I read Where? Please give a specific reference. Somoth Ergai said: It seems like it should take an infinite amount of time to enter a black hole, even from the perspective of the object entering it. This is wrong. The proper time for an ...
In Sect. 3, we will start by considering the five-dimensional case where the rotating stealth black hole will be constructed on the Myers– Perry spacetime with equal angular momenta. We will also see that the scalar field leaves the metric invariant under a constant disformal transformation. ...
Black Hole boasts at how simple it was to save Bomby's life. The same two contestants are then knocked off accidentally by Dora when she runs up the stairs, and Black Hole once again launches Bomby back up. Later, when Pie (who was killed by Flower in her rush to win) is ...
This provides a simple explanation of the result that the rate of pair creation of non-extreme black holes is enhanced by precisely the black hole entropy. Finally, we discuss black hole $annihilation$, and argue that Planck scale remnants are not sufficient to preserve unitarity in quantum ...
byUniversity of California - Berkeley A supernova (bright spot at lower left) and its host galaxy (upper center), as they would appear if gravitationally lensed by an intervening black hole (center). The gravitational field of the black hole distorts and magnifies the image and makes both th...
But the black holes were born into a gas-depleted cavity and, with little gas to feed on, they grew very slowly. “During the 200 million years of our simulation, a 100 solar-mass black hole grew by less than one percent of its mass,” Alvarez said.” ...