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Quantum Gravity improved black holes Astro Coffee • 27. Jan 2015, 14:00-15:00 • FIAS 0.101 Quantum Gravity group of Piero Nicolini / Marcus Bleicher Sven Köppel koeppel@fias.uni-frankfurt.de

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Page 1: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

Quantum Gravity improved black holes

Astro Coffee • 27. Jan 2015, 14:00-15:00 • FIAS 0.101

Quantum Gravity group of Piero Nicolini / Marcus Bleicher

Sven Kö[email protected]

Page 2: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

OutlineQuantum Gravity improved black holes

Sven Köppel

1. Quantum effects at the BH coreSchwarzschild singularityParticle compression

2. Minimal resolution approach: GUPGravity as nonlocal field theoryGeometry and properties of the GUP BHFeatures

3. What's nextLarge extradimensional scenarioOther BH core modelsExperimental evidence

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Schwarzschild BHs exhibit problems

The Schwarzschild black hole is not suitable to describe „smallest distances“:

Curvature singularity ill defined thermodynamics

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There is a widespread belief in a minimal spatial resolution in nature: Planck scale

Incooperating gravitational effects in quantum mechanics

Example Gedankenexperiments:Heisenberg Microscope Shrinking a volume of matter:

The Planck scale

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Incooperating gravitational effects in quantum mechanics

There is a widespread belief in a minimal spatial resolution in nature: Planck scale

Shrinking a volume of matter:

Physically allowed regionby GUP prediction

Generalized Uncertainty Principle (GUP)

Page 6: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

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Incooperating gravitational effects in quantum mechanics

There is a widespread belief in a minimal spatial resolution in nature: Planck scale

Shrinking a volume of matter:

Physically allowed regionby GUP prediction

Generalized Uncertainty Principle (GUP)

Page 7: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

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Incooperating gravitational effects in quantum mechanics

There is a widespread belief in a minimal spatial resolution in nature: Planck scale

Generalized Uncertainty Principle (GUP)

Fourier Transformation in

coordinate frame of a freely

infalling observer

→ gives us a momentum space cutoff. Use Cutoff to determine sharpest possible object in GUP:

→ maximal localized momentum states and

Page 8: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

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The GUP-inspired black hole

Big masses:Classical Schwarzschildbehaviour

Page 9: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

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Big masses:Classical Schwarzschildbehaviour

Extremal mass:One degenerate horizon

The GUP-inspired black hole

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Too light mass:no black hole (G-Lump)

Big masses:Classical Schwarzschildbehaviour

Extremal mass:One degenerate horizon

The GUP-inspired black hole

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Too light mass:no black hole (G-Lump)

Big masses:Classical Schwarzschildbehaviour

Extremal mass:One degenerate horizon

The GUP-inspired black hole

Features:

● Schwarzschild at large distances● String theory motivated modification at Planck scale● Still left: Curvature singularity at origin

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The GUP-inspired black hole

Further features:

● Regular thermodynamics● The existance of a remnant● Self-completeness of gravity

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The black hole remnant: thermodynamics

semiclassical regimecooldownphase

inaccessibleregime

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The black hole remnant: thermodynamics

semiclassical regimecooldownphase

inaccessibleregime

Phase transitionHeatcapacity

Temperature:

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The black hole remnant: thermodynamics

semiclassical regimecooldownphase

inaccessibleregime

Phase transitionHeatcapacity

Temperature:

Entropy

Zero entropy remnant

The remnant:A cold stableevaporationendpoint

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The GUP-inspired black hole

An ongoing project: Extending GUP black holes to extra dimensions.

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The weak hierarchy problem of the Standard Model

Elektroweak scalevs.

Planck scale

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Large Extra Dimensions

ADD scenario

Integrated huge Volume ofextra dimensions

Large µm up to mm

Arkani-HamedDimopoulosDvali 1998

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Large Extra Dimensions

n=1n=2

n=5

Maybe modify GUP for LXDsongoing work

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Outlook: Different metrics

The self-regular metric:● Regular center? Yes● Classical low-energy limit? Yes● Self-encoding? Yes● Holographic picture holds? No

Regular De Sitter core:Quantum outward pressure

DeSitterSchwarzschild

The holographic metric:● Regular center? No● Classical low-energy limit? Yes● Self-encoding? Yes● Holographic picture holds? Yes

Page 21: Quantum Gravity improved black holes - … · Outline Quantum Gravity improved black holes Sven Köppel 1. Quantum effects at the BH core Schwarzschild singularity Particle compression

Macroscopic Microscopic

Conclusion

Literature

Nicolini, SpallucciHolographic screens in UV self-complete QR[arXiv:1210.0015]

Ongoing: Isi, Knipfer, Köppel, Mureika, NicoliniSelf-Completeness and the GUP in extradimensions

Ongoing: Bleicher, Dirkes, Frassino, Knipfer, Köppel, NicoliniGUP and BHs – a paedagogical review

Picture Credits

Bernhard Carr [KSM 2012]Bekenstein, Kamajian [Scientific American 2005]SM particle chart: Phys. Today 65, 9, 12 (2012)