Many Aspects of BH-Info Paradox

Many Aspects of BH-Info Paradox

MINOS AXENIDES –2020- NCSR – DEMOKRITOS, INPP THEORETICAL HIGH ENERGY PHYSICS GROUP 2020 funding 3 national grants ( 1 ΕΛΙΔΕΚ,1 ΙΚΥ,1 ΕΣΠΑ) # Grant/Fellowship Amount Period Scientist in charge G. Pastras HFRI E-12300: Holographic applications 1 200 k€ 2018-21 of quantum entanglement (HAPPEN) M. Axenides 2 IKY (doctoral fellows) 30 k€ 2018-21 D. Katsinis E. Floratos ΕΔΒΜ 103: Χαοτική Δυναμική και 3 45 k€ 2020-21 Μελανές Οπές στη Θεωρία BMN M. Axenides BH PHENOMENOLOGY EVENT HORIZON TELESCOPE 2-BLACK HOLE MERGER 1st IMAGE ever BH-Info Paradox at a Crossroads 2020 Quantum Mechanics of Extremal Black Holes : Discrete Spacetime -AdS2(N)- Near Horizon Geometry Proposal with a proof of a Continuum limit AdS2(N) -> AdS2 ( EF + SN) Published : SIGMA-17-(2021), 004 Previous Publications : • The quantum cat map on the modular discretization of extremal black hole horizons Minos Axenides (Democritos Nucl. Res. Ctr.), Emmanuel Floratos (Democritos Nucl. Res. Ctr. & Athens U.), Stam Nicolis (Fed. Denis Poisson, Tours). Published in Eur.Phys.J. C78 (2018) no.5, 412 • Modular discretization of the AdS2/CFT1 holography Minos Axenides (Democritos Nucl. Res. Ctr.), E.G. Floratos (Democritos Nucl. Res. Ctr. & CERN & Athens U.), S. Nicolis (Tours U.). Jun 24, 2013. 31 pp. Published in JHEP 1402 (2014) 109 . • Chaotic Information Processing by Extremal Black Holes Minos Axenides (Democritos Nucl. Res. Ctr.), Emmanuel Floratos (Democritos Nucl. Res. Ctr. & Athens U.), Stam Nicolis (Fed. Denis Poisson, Tours & Tours U.). Apr 2, 2015. 7 pp. Published in Int.J.Mod.Phys. D24 (2015) no.09, 1542012. Strong GRAVITY : 1. Planck Scale ≈ ퟏퟎ−ퟑퟑcm 2. BH horizon R ≈ GM/풄ퟐ F G M1M2 N D2 10−33 c c2 2 F GN 1 c2 D4 BH-Near Horizon Stretched Space-time Few puzzling observations Black holes possess quantum substructure ( qubits) giving rise to thermal behaviour.—Hawking (1974) • They have entropy[Bekenstein] S(bh) = 푐3 푅2/ h G Minimun Energy per qubit--- hc/R Total Energy of a BH of radius R = 푐4R/G 3 2 No. of bits = 퐸푏ℎ / 퐸푏푡 = 푐 푅 / h G • They Radiate with temperature[Hawking] kT = hc/R • What are these bits??? BH- INFO-PARADOX= PURE INCOMING STATES MIXED OUTGOING STATES HOLOGRAPHY => INFORMATION OF A VOLUME IS ENCODED ON ITS SURFACE BOUNDARY additional properties of the black hole degrees degrees of freedom • Non locality • Chaotic and random dynamics • BHs as the fast scramblers of incoming information • Entanglement between the outgoing –incoming pairs of particles which carry away the “lost information” saving unitarity PROPOSAL # bits = N spacetime discretum DISCRETE and Random GEOMETRY IS AN APPROPRIATE FRAMEWORK FOR THE BH QUANTUM INFORMATION PARADOX IN THE BH- NEAR HORIZON SPACETIME ARITHMETIC GEOMETRY A MODEL FOR PLANCK SCALE SPACE-TIME FOR NEAR HORIZON BH-SPACETIME • MODULAR ARITHMETIC -> RANDOM POINT GEOMETRIES • MODULAR DYNAMICS A= 2X2 MODULAR MATRICES IN SL[2,Z[N]] -> CHAOS AUTOMATIC • FINITE DIMENSIONAL HILBERT SPACES • FINITE QUANTUM MECHANICS AND QUANTUM FIELD THEORIES • N=p^n, QUDITS OF INFORMATION, • FINITE DIMENSIONAL UNITARY RANDOM EVOLUTION OPERATORS U[A] FINITE BEKENSTEIN-HAWKING BH-ENTROPY IMPLIES —FINITE DIM.HILBERT SPACE d • FINITENES OF B-H ENTROPY S ≈ A/4 -> FINITE DIMENSIONAL HILBERT SPACEACK HOLE MICROSCOPIC STATES Dim[H]=Exp[S] •FINITE DIMENSIONAL HILBERT SPACE -> DISCRETE AND FINITE SPACE-TIME • THE SIMPLEST MODEL FOR SINGLE PARTICLE DYNAMICS A DISCRETE AND FINITE PHASE SPACE Z[N]XZ[N] Z[N]={0,1,2,3,..,N-1} ALL INTEGERS MODULO N FOR N=PRIME INTEGER=p GALOIS FIELD F[p] -> MODULAR ARITHMETICS CONCLUSIONS • DISCRETIZING AdS2 RADIAL AND TIME NEAR HORIZON GEOMETRY OF EXTREMAL BLACKHOLES AND AT THE SAME TIME PRESERVING THE ALGEBRAIC STRUCTURE OF THE ISOMETRIES NECESSARILY LEADS TO THE MOD[N] ARITHMETIC DISCRETIZATION • WITH HOLOGRAPHY AdS2[N]/CFT1[N], • We make IT QUANTUM THROUGH FINITE QUANTUM MECHANICS .

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