DPG Conference, Hamburg

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DPG Conference, Hamburg Microscopic black holes and their significance in quantum theories of gravity Why is grav force so different Next: em grav mm ----- R2 Gerard ’t Hooft, Utrecht University DPG Conference, Hamburg March 2, 2016

Karl Schwarzschild 1916 “Über das Gravitationsfeld eines Massenpunktes nach der Einsteinschen Theorie” New radial coordinate

Local observer thinks time continues, moves to singularity Black Hole or wormhole? Universe I Local observer thinks time continues, moves to singularity “Time” stands still at the horizon Next: 2 astronauts Universe II So, one cannot travel from one universe to the other -

Where are the strongest possible gravitational fields ? The field is strongest in the tiniest black holes !

Planck Units Next: highway through desert

The highway across the desert ??? Smallest Black holes? Planck length: Quantum Gravity The highway across the desert GUTs LHC Next instability against implosion

Next : Hawking Radiation

Stephen Hawking’s great discovery: Black hole emits particles !! Next : vacuum fluctuations

While emitting particles, the black hole loses energy, hence mass ... it becomes smaller. Lighter (smaller) black holes emit more intense radiation than heavier (larger) ones Next: in clock, ou keys,coins The emission becomes more and more intense, and ends with ...

As seen by distant As observer experienced by astro- naut himself Time stands still at the horizon Continues his way through Next Hawking, Einstein, Newton in Star Trek They experience time differently. Mathematics tells us that, consequently, they experience particles differently as well

creates a particle annihilates a particle Horizon In quantum field theories, Fourier transform a field in the time direction:

The vacuum state is defined by demanding: But the outside observer defines time t differently from the local observer’s time. Therefore, they calculate their Fourier coefficients differently, so that positive and negative ω mix ! The vacuum state is defined by demanding: only if And therefore, the vacuum state is not the same for the different observers !

And so it was discovered that black holes behave much like other forms of matter … Are black holes just “elementary particles”? Are elementary particles just “black holes”? Imploding matter Hawking particles Next: one would expect everything to be computable now Black hole “particle”

Particles emerging from Black holes (appear to) have an ideal, thermal spectrum: Hawking particles come from vacuum fluctuations, and the vacuum (for one given observer) is the same everywhere. One then simply derives the entropy of such black holes. And with that, the distribution of their quantum states

In a black hole: If we had the amplitude , we could compare the absorption process with the emission process. This gives: (phase space of heavier BH) (phase space of lighter BH) In a black hole: compare Hawking’s particle emission process with the absorption process:  same W !! 12 6 3 9 12 6 3 9 Black hole plus matter   black hole plus matter Heavier black hole

the black hole as an information processing machine One finds the black hole as an information processing machine The constant of integration: a few “bits” on the side ... Next: BH = elementary particle

The Black Hole Information Paradox This would suggest black holes obey a Schrödinger equation. And that would imply that they evolve according to a unitary evolution operator … as usual in quantum mechanics ! But how do we derive the microstates from first principles? The evolution should be described by a unitary evolution operator, , Different in-states should evolve into different out-states. How can that be if they went into a black hole? The Black Hole Information Paradox

The Black Hole Information Paradox How do the Hawking particles depend on the particles that went into the black hole? According to Hawking: Not at all ! Do Hawking’s particles – derived from applying QM to the Schwarzschild metric – themselves violate basic QM laws ?

That can’t be right !! Leonard Susskind, 2008

vacuum Hawking radiation vacuum Hawking radiation matter going in

But the particles in region II cannot be observed – they disappear Horizon The quantum states in regions I and II are entangled Region II Region I space time entanglement But the particles in region II cannot be observed – they disappear Next: thermal distribution: mixed state This seems to prohibit the description of the black hole entire as a single quantum object

Alternative theories: Indeed, loss of quantum coherence; no pure quantum description of BH (problem: energy conservation) Hawking ~ 1975 2. After explosion by radiation: black hole remnant (problem: infinite degeneracy of the remnants) ~ 2000 3a. Information returns in the Hawking radiation, but only at the end. Next: paradox ~ 2015 3b. Information returns in the Hawking radiation, immediately. Me ~ 1984 - present

interaction horizon Next: heavy ion scattering, eikonal approximation

By taking back reaction into account, one can study how ingoing particles affect the outgoing ones … Next: Black against white holes ❖

The horizon was a perfect sphere, until the in- and out going particles distorted it by their gravitational fields. These calculations turn out to be almost identical to the caculations for the motion of closed strings Are black holes described by string theory?

black hole information problem But the main problem with black holes is the question how to handle the quantum states they should form: the microstates. How is the information describing these microstates encoded on the horizon? How do the in going particles transform their data onto the Hawking particles going out? black hole information problem Conventional string theories describe the formation of higher dimensional “membranes”. Stacks of these membranes take the shape of black holes. These black holes are usually quite different from Schwarzschild’s solution. They have maximal charges or angular momenta. That makes their horizons look quite different. They do get their microstates as expected. But do we then also understand Schwarzschild’s black hole?

vacuum vacuum Hawking radiation comes from vacuum fluctuations. And these fluctuations are correlated! The gravitational field of the in going particles drags the Hawking particles along ! And this can be calculated. vacuum Hawking radiation vacuum Hawking radiation matter going in So the radiation going in does have an effect on the particles coming out.

IV III region II region I Recently, we did the calculation more extensively: Will spherical waves of in-going particles produce spherical waves of outgoing ones? YES ! but … IV Hawking radiation region II region I matter going in III What happens with the particles disappearing into region II ???

Region II must be exactly as physical as region I But what is it ? A natural suggestion: points at opposite side of BH ! (antipodal points) If that is true, it would yield a remarkable “prediction” for the Hawking particles: the vacuum for a local observer, would correspond to particle-antiparticle pairs for the Schwarzschild observer. But the antiparticles go into the negative time direction ! Conclusion (tentative): Every Hawking particle at one side of the BH, is 100 % entangled with a particle at the antipodal point ! Only further theoretical analysis can tell us if this is correct …

Black hole information and holography: The Next Step A small step for Mankind , … A giant leap for me !

THE END