General Relativity

Einstein's Masterpiece: Gravity is the curvature of spacetime. Mass-energy tells spacetime how to curve, and spacetime tells mass-energy how to move.

Chapter 29: Introduction to Quantum Gravity

Quantum gravity seeks to reconcile general relativity with quantum mechanics. At the Planck scale (10-35 m), spacetime itself should be quantized. This remains one of the greatest open problems in physics.

Why Quantum Gravity?

Singularities

GR predicts infinite curvature at black holes and Big Bang. QG should resolve these.

Non-renormalizability

Naively quantizing GR produces infinities that can't be absorbed into parameters.

Information Paradox

Black hole evaporation seems to destroy information, violating quantum mechanics.

Major Approaches

String Theory

Fundamental objects are strings, not particles. Includes gravity naturally. Extra dimensions.

Loop Quantum Gravity

Quantize spacetime directly. Area and volume are quantized. Background-independent.

Asymptotic Safety

GR becomes renormalizable at high energies via a UV fixed point.

Causal Set Theory

Spacetime is fundamentally discreteβ€”a partially ordered set of events.

Planck Scale

Planck Length

\( \ell_P = \sqrt{\frac{\hbar G}{c^3}} \approx 10^{-35} \text{ m} \)

Planck Time

\( t_P = \sqrt{\frac{\hbar G}{c^5}} \approx 10^{-44} \text{ s} \)

Planck Mass

\( m_P = \sqrt{\frac{\hbar c}{G}} \approx 10^{19} \text{ GeV} \)