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As the 2.7K temperature of the CMB continues to cool, more massive black holes will evaporate. So that addresses black holes.
If Hawking's theory of black hole radiation is correct, then black holes are expected to shrink and evaporate over time because they lose mass by the emission of photons and other particles.[32] The temperature of this thermal spectrum (Hawking temperature) is proportional to the surface gravity of the black hole, which, for a Schwarzschild black hole, is inversely proportional to the mass. Hence, large black holes emit less radiation than small black holes.[86]
A stellar black hole of 1 M☉ has a Hawking temperature of about 100 nanokelvins. This is far less than the 2.7 K temperature of the cosmic microwave background radiation. Stellar-mass or larger black holes receive more mass from the cosmic microwave background than they emit through Hawking radiation and thus will grow instead of shrink. To have a Hawking temperature larger than 2.7 K (and be able to evaporate), a black hole needs to have less mass than the Moon. Such a black hole would have a diameter of less than a tenth of a millimeter.
Observations suggest that the expansion of the universe will continue forever. If so, the Universe will cool as it expands, eventually becoming too cold to sustain life. For this reason, this future scenario is popularly called the Big Freeze.
doga_lover54: Do black holes expand and grow?
Jerry: We've found at least a dozen solar mass black holes in our own galaxy. There are probably millions of supermassive black holes at the centers of other galaxies but so far we've only seen a few of the nearest of these.
Akarsh_Valsan: Can black holes really suck things up?
Jerry: At a distance, black holes really don't have more gravity than normal objects, so at a distance they really won't suck things in any more than a normal object of the same mass.
by definition at some distant point in the future, the black holes will have swallowed everything including each other till there is only 1 mega black hole containing the whole universe.
Jerry: When two black hole collide (they actually don't collide, but circle each other until they coalesce) enormous "gravity waves" are thought to be emitted.
Jerry: It's impossible to see inside of a black hole.
originally posted by: johnb
a reply to: Develo
from NASA black hole q&a
doga_lover54: Do black holes expand and grow?
Jerry: We've found at least a dozen solar mass black holes in our own galaxy. There are probably millions of supermassive black holes at the centers of other galaxies but so far we've only seen a few of the nearest of these.
Akarsh_Valsan: Can black holes really suck things up?
Jerry: At a distance, black holes really don't have more gravity than normal objects, so at a distance they really won't suck things in any more than a normal object of the same mass.
So as the black hole grows so does the event horizon presumably??
So surely over billions/trillions of years they would merge and grow so massive there would be nothing else left apart from one giant black hole containing everything.
I don't know about everything, but they will become dominant until they evaporate, but since you asked about the end of our universe, I think they will probably evaporate in the end and will just be a "phase" on the way to the end:
originally posted by: johnb
I can see the logic of that, however if the black holes are moving and growing in mass all the time and presumably new ones are being continuously formed throughout the universe is it not possible that eventually they would consume everything?
Black Hole Era
10^40 years to 10^100 years
After 10^40 years, black holes will dominate the Universe. They will slowly evaporate via Hawking radiation. A black hole with a mass of around 1 M☉ will vanish in around 2×10^66 years. As the lifetime of a black hole is proportional to the cube of its mass, more massive black holes take longer to decay. A supermassive black hole with a mass of 10^11 (100 billion) M☉ will evaporate in around 2×10^99 years.
Hawking radiation has a thermal spectrum. During most of a black hole's lifetime, the radiation has a low temperature and is mainly in the form of massless particles such as photons and hypothetical gravitons. As the black hole's mass decreases, its temperature increases, becoming comparable to the Sun's by the time the black hole mass has decreased to 10^19 kilograms. The hole then provides a temporary source of light during the general darkness of the Black Hole Era. During the last stages of its evaporation, a black hole will emit not only massless particles but also heavier particles such as electrons, positrons, protons and antiprotons.
If protons do not decay as described above
In the event the proton does not decay as described above, the Degenerate Era will last longer, and will overlap the Black Hole Era. In a timescale of approximately 10^65 years, apparently rigid objects such as rocks will be able to rearrange their atoms and molecules via quantum tunnelling, behaving as a liquid does, but more slowly. However, the proton is still expected to decay, for example via processes involving virtual black holes, or other higher-order processes, with a half-life of under 10^200 years. For example, under the Standard Model, groups of 2 or more nucleons are theoretically unstable because chiral anomaly allows processes that change baryon number by a multiple of 3.
Dark Era and Photon Age
From 10^100 years
The lonely photon is now king of the universe as the last of the supermassive black holes evaporates.
After all the black holes have evaporated (and after all the ordinary matter made of protons has disintegrated, if protons are unstable), the Universe will be nearly empty. Photons, neutrinos, electrons, and positrons will fly from place to place, hardly ever encountering each other.