Quantization of mass for black holes?

In summary, Gia Dvali, Cesar Gomez, and Slava Mukhanov argue that the masses of black holes cannot have continuous values and must be quantized in any sensible quantum field theory. They also propose a universal quantization rule for all classicalons, including black holes, which implies that they cannot emit or absorb arbitrarily soft quanta. This has implications for the production of black holes and other classicalons at the LHC. The authors also address concerns about the safety of the LHC, stating that particle physicists have already analyzed this issue in detail. The quantization rule proposed by the authors is m=\sqrt{N}m_P, where m_P is the Planck mass. However, recent LHC results put
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"Black Hole Masses are Quantized," Gia Dvali, Cesar Gomez, Slava Mukhanov, http://arxiv.org/abs/1106.5894
We give a simple argument showing that in any sensible quantum field theory the masses of black holes cannot assume continuous values and must be quantized. Our proof solely relies on Poincare-invariance of the asymptotic background, and is insensitive to geometric characteristics of black holes or other peculiarities of the short distance physics. Therefore, our results are equally-applicable to any other localized objects on asymptotically Poincare-invariant space, such as classicalons. By adding a requirement that in large mass limit the quantization must approximately account for classical results, we derive an universal quantization rule applicable to all classicalons (including black holes) in arbitrary number of dimensions. In particular, this implies, that black holes cannot emit/absorb arbitrarily soft quanta. The effect has phenomenological model-independent implications for black holes and other classicalons that may be created at LHC. We predict, that contrary to naive intuition, the black holes and/or classicalons, will be produced in form of fully-fledged quantum resonances of discrete masses, with the level-spacing controlled by the inverse square-root of cross-section.

There is a nontechnical summary on the arxiv blog: http://www.technologyreview.com/blog/arxiv/ , along with some inflammatory and uninformed speculation about safety at the LHC, including "This is a debate that particle physicists are strangely reluctant to engage in, having ignored most of the questions marks over safety." In fact, particle physicists have analyzed the issue in great detail: Giddings and Mangano, "Comments on claimed risk from metastable black holes," http://arxiv.org/abs/0808.4087

Anyway, getting back to the actual physics of the paper, the quantization rule they propose is [itex]m=\sqrt{N}m_P[/itex], where mP is the Planck mass. The Planck mass is 10^19 GeV in 3+1 dimensions, but it is much lower if you assume large extra dimensions. IIRC recent LHC results are putting some tough constraints on large extra dimensions, so it is probably not likely that that the ideas in this paper can be confirmed. The area would be quantized in integer multiples of the Planck area, which I guess sounds nice in relation to LQG...?
 
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I have already seen such theory long time ago (two years back), I try to dig it up if you are really interested. The way I remember it, the math was very simple.
 

Related to Quantization of mass for black holes?

What is quantization of mass for black holes?

The concept of quantization of mass for black holes is based on the idea that the mass of a black hole can only take on certain discrete values. This is similar to the concept of quantization in other areas of physics, such as in atoms where only certain energy levels are allowed. In the case of black holes, this quantization is thought to occur due to the quantization of the area of the event horizon.

Why is quantization of mass for black holes important?

Quantization of mass for black holes is important because it could provide a key piece of information for understanding the fundamental laws of physics. It has been suggested that if black hole masses are quantized, it could lead to a unification of quantum mechanics and general relativity.

How is the quantization of mass for black holes related to Hawking radiation?

Hawking radiation is a phenomenon where black holes emit particles due to quantum effects. The quantization of mass for black holes is thought to be related to Hawking radiation because the discrete mass values could affect the types and amounts of particles emitted by a black hole.

Has the quantization of mass for black holes been observed?

At this time, there is no direct evidence for the quantization of mass for black holes. However, some theoretical models and calculations have suggested that black hole masses may be quantized. Further research and observations will be needed to confirm or refute this idea.

What are the implications of the quantization of mass for black holes?

If the quantization of mass for black holes is confirmed, it could have significant implications for our understanding of the universe and the laws of physics. It could also provide new insights into the nature of black holes and the behavior of matter at extreme scales.

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