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Editorial path·Physics·graduate·5 institutions

Curved Spacetime, Black Holes & Holographic Quantum Gravity

Physical law, LIGO gravitational waves, singularity topology, and AdS/CFT entanglement

Follows general relativity and quantum mechanics to their modern frontier with Feynman, Kip Thorne, Roger Penrose, Leonard Susskind, Juan Maldacena, and Nima Arkani-Hamed.

Start Step 16 steps · 13h total

Curriculum sequence

6
Step 1·Cornell University·Richard Feynman· 55:54

The Relation of Mathematics to Physics (Messenger Lecture 2)

Illuminates why deep physical principles admit equivalent geometric and algebraic laws.

Step 2·Caltech·Kip Thorne· 1:10:52

From the Big Bang to Black Holes and Gravitational Waves

Chronicles curved spacetime dynamics and LIGO's detection of merging black holes.

Step 3·University of Oxford·Roger Penrose· 56:22

Singularity Theorems, Black Holes, and Conformal Cyclic Cosmology

Examines global causal structure, trapped surfaces, and cosmological Weyl curvature.

Step 4·Stanford University·Leonard Susskind· 1:47:53

ER = EPR: Wormholes, Horizon Firewalls, and Entanglement

Links Einstein-Rosen wormhole geometry directly to bipartite quantum entanglement.

Step 5·Institute for Advanced Study·Juan Maldacena· 1:14:07

The Meaning of Spacetime: Black Holes and Quantum Entanglement

Shows how bulk gravitational spacetime emerges holographically from boundary quantum mechanics.

Step 6·Cornell University·Nima Arkani-Hamed· 7:17:30

The Future of Fundamental Physics: Spacetime and Quantum Amplitudes

Explores why Planck-scale scattering amplitudes point beyond smooth spacetime.