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ICTS
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GR and QG: The Next 100 Years
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ICTS - TIFR
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20th Century Physics
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21st Century Physics
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The Major Challenges to GR
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The Quantum Connection
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The Question
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GR: THE NEXT 100 YEARS
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Obituary
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THE PARADIGM
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More IS Different
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The Fluid called Spacetime
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Spacetime in Arbitrary Coordinates
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Local Inertial Observers
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FLAT SPACETIME
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Thermal fluctuations
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Spacetimes, Like Matter, can be Hot
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Gravity-Thermodynamics Connection
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The Importance Of Being Hot
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Atoms of Matter
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The Quantum of Area
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Holographic Equipartition
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Evolution of spacetime
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Geometry Thermodynamics
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What makes Spacetime Evolve
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Newton's Law of Gravitation
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Macroscopic Nature Of Gravity
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The Challenge
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Atoms Of A Fluid
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Geodesic Interval
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Zero-Point Length
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Area Of A Point
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Atoms of Space
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Quantum of Information
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RECALL
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Our Strange Universe
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Our Stranger Universe
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N bulk
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Accessibility of Cosmic Information
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Cosmic Information: Cosmin
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Cosmin and the A
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The Cosmic Connection
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= 3.835 107, Pinf * = 1.157 1015 Ge V
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Cosmic Conundrums
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Possible new insight
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Cosmic Evolution
Description:
Explore the future of General Relativity and Quantum Gravity in this 53-minute lecture by T. Padmanabhan at the International Centre for Theoretical Sciences. Delve into the major challenges facing General Relativity, the quantum connection, and the paradigm shift in understanding spacetime as a fluid. Examine concepts such as thermal fluctuations in spacetime, the gravity-thermodynamics connection, and holographic equipartition. Investigate the macroscopic nature of gravity, the concept of zero-point length, and the quantum of information. Discover insights into our strange universe, cosmic information, and potential new perspectives on cosmic evolution. Gain a deeper understanding of the interplay between quantum theory and general relativity, and explore the cutting-edge ideas shaping the next hundred years of research in these fundamental areas of physics.

GR and QG - The Next Hundred Years by T Padmanabhan

International Centre for Theoretical Sciences
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