It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Thank you.
Some features of ATS will be disabled while you continue to use an ad-blocker.
Actually they grow, not evaporate.
originally posted by: joelr
BH do radiate some energy away which causes them to eventually evaporate.
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.
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 solar mass will vanish in around 2×10^66 years.
tiny black holes with mass smaller than that of the moon,
If you have a time index to what you're talking about, I'll watch it at that time index, but that's an hour long video so I'm not going to watch the whole thing to see what you're talking about. As far as I know such small black holes have been hypothesized but never observed.
originally posted by: KrzYma
a reply to: Arbitrageur
tiny black holes with mass smaller than that of the moon,
why not a black hole with the mass of 2 protons ??
this is a joke, right ?
if you don't know watch this...
www.youtube.com...
6. CONCLUSION
In this paper, we considered a minimal extension of the SIDM parameter space, in which a self-interacting component comprises only a fraction of the dark matter. For f > 0:1, this evades all prior constraints on SIDM models. We highlighted the uSIDM regime, where the SIDM component is subdominant but ultra-strongly self-interacting, with f 1 and 1 cm2=g. In the setup considered here, the presence of uSIDM leads to the production of black holes with a mass of around 2% of the total uSIDM mass in the halo at very early times. In particular, such black holes can act as seeds for baryon accretion starting soon after halo formation, alleviating potential diculties with accommodating massive quasars at high redshifts within the standard CDM cosmology. If black holes are formedubiquitously in dwarf halos before they undergo mergers, they may also resolve the Too Big to Fail problem by ejecting matter from cores during black hole mergers.
More detailed cosmological simulations are needed to conrm the conclusions of this paper and suggest other potential observational consequences of uSIDM. Setting aside the detailed predictions, this paper has demonstrated that multi-componentdark matter can have strong eects on small scales while still evading existing constraints.
In the toy model discussed here, the strong eect was the result of the gravothermal catastrophe. Gravothermal collapse of a strongly-interacting dark matter component is a novel mechanism for production of seed black holes, potentially one with many implications. Given its appearance in the simple extension of CDM considered here, it is plausible that Gravothermal collapse and its observational consequences, such as seed black hole formation, aregeneric features of more detailed models. It is important to consider, and then observe or constrain, this and other observational consequences that are qualitatively dierent from the predictions of the standard cosmological model.
Our discussion has been purely phenomenological, so it is reassuring to note the existence of a class of hidden-sector models [93] which naturally produce a subdominant stronglyinteractingdark matter component, with self-interaction cross-sections ranging as high as1011 cm2=g.
Very interestingly, some models give both a dominant component with ' 0:1 1 cm2=g, as needed to alleviate discrepancies between CDM and observations,and a uSIDM component with ' 105 107 cm2=g, which could produce seed black holes via the mechanism described in this paper.
We thank Shmulik Balberg, James Bullock, Renyue Chen, Phil Hopkins, Jun Koda, Sasha Muratov, Lisa Randall, Paul Shapiro, Stu Shapiro, Charles Steinhardt, and Naoki Yoshidafor helpful discussions. We thank especially Sasha Muratov for measuring concentration
28 parameters at high redshifts in the FIRE runs and providing us with the resulting halo catalogs. This research is funded in part by DOE Grant #DE-SC0011632, and by theGordon and Betty Moore Foundation through Grant #776 to the Caltech Moore Center for
Theoretical Cosmology and Physics.[1]
He never said anything about 2 protons black hole, in fact it wasn't until the last few seconds of the video that he even talked about small black holes and how they evaporate. He also explained that's probably why we never see any because even if there once were some micro black holes, maybe they already evaporated.
originally posted by: KrzYma
well, maybe you should watch it all, right now from what you talking about I even recommend it for you !
You theorizing about 2 protons Black Hole ?? WTF !
Your whole theory leaves one important force out of your empty heads theories !
Coulomb force, IDIO.. !!!
A black hole the weight of a car would have a diameter of about 10^−24 m and take a nanosecond to evaporate, during which time it would briefly have a luminosity more than 200 times that of the Sun. Lower-mass black holes are expected to evaporate even faster; for example, a black hole of mass 1 TeV/c2 would take less than 10^−88 seconds to evaporate completely.
originally posted by: dragonridr
a reply to: KrzYma
You do realize we can make two protons slam into each other right? Repulsive forces can be overcome with energy. Since energy equals mass as we all know the faster we can mive a particle the more mass it has. Thr LHC already did some experiments with lead creating a super dense mass. With the New upgrades they believe they can make a blackhole.Maybe in the future you might want to know what your talking about before you try to correct someone.
m.livescience.com...
If a black hole with the mass of a car will evaporate in a nanosecond while briefly emitting radiation at a rate 200 times greater than the sun, and smaller mass black holes will evaporate even faster, so why are you even asking about "holding masses together"? Most predictions are more along these lines:
originally posted by: KrzYma
and what in the world has some random smashing to do with bend space time ???
so... you do agree, those masses recoil each other in those collisions, right ?
how do you hold those masses together than for a black hole to be created ?
I don't see how the question "how do you hold those masses together? " applies to an event lasting .00000000000000000000000001 seconds.
Particle collisions at energies above the Planck scale must create black holes, because they put large amounts of energy within a small enough region (the so-called Schwarzschild radius). Giddings and Thomas [6] and Dimopoulos and Landsberg [7] realized that this logic, applied to the ADD model, implies that high-energy collisions at TeV energies should produce black holes. They did not consider this a danger but rather an exciting possibility. They imagined that the black holes would glow with a temperature of about 1TeV/kB, emit large numbers of quarks, leptons, and bosons through Hawking radiation [8], and evaporate in 10^-26s. This process would produce unique and unmistakable events detectable by the LHC experiments.
We didn't have proof of the Higgs boson until recently, so just because we temporarily lack proof of an idea doesn't mean the idea isn't true. So is the idea of black holes evaporating just a wild guess, or is it a sound idea likely to be verified by observation at some point, possibly even with the upgraded LHC? I think this supports the latter rather than the former:
originally posted by: KrzYma
a reply to: Arbitrageur
black hole can evaporate thanks to another theory, QM
is this your explanation and the proof ?
So it's not proven until it's proven, but the theoretical evidence for it is pretty strong.
But what if Hawking’s prediction that black holes emit radiation is incorrect? There is no direct evidence for Hawking radiation. The only black holes we have seen in nature are the size of stars or galaxies, and their Hawking radiation is invisible.... However, the theoretical evidence for Hawking radiation is very strong. Numerous calculations from different points of view agree on the detailed formulae for the Hawking temperature and spectrum. A related effect, the Unruh effect of radiation from an accelerated body, is demonstrable from quantum electrodynamics. Models have been proposed, including one by Unruh himself, in which black holes do not radiate. That model, however, requires violation of Lorentz invariance, which is plausible at 1019GeV but is completely excluded at TeV energies.
What? Who is killing for theoretical physics or LHC research?
Like God..., people still kill for it rather than rethink and understand
If you tried to collide only 2 protons, would you be surprised to learn that they may not collide?
originally posted by: KrzYma
a reply to: ErosA433
you forget to mention, the are not just 2 protons smashing but some billions? is it right ??, not that it matters, more than 2 is more than too much to see the true interaction.
So yes of course they have way more than one proton in each beam so that something happens. I read somewhere it's about 281 trillion protons per beam but I'm not sure if that's correct, but it's definitely way more than one proton per beam.
The particles are so tiny that the task of making them collide is akin to firing two needles 10 kilometres apart with such precision that they meet halfway.
That depends on the distance of the charges from each other, and the distance of the observer from the charges. If the observer is close enough to the charges, yes of course you don't observe zero charge. But if you calculate the electric field at various distances from those two charges, you find that even if the theoretical value may be slightly above zero, for all practical purposes, zero becomes a pretty good approximation at some distance from the charges, though I don't understand how this has anything to do with the topic of this thread.
like I've said in another thread, charges -1 and +1 close together is not equal 0