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Physical Cosmology

Physical cosmology is the scientific branch of physics and astronomy that investigates the origin, large-scale structure, evolution, and ultimate fate of the universe.

Type: Concept Domain: Physics Mathematics Philosophy

Overview

Modern physical cosmology relies on general relativity and quantum field theory, constrained by observational data from space- and ground-based observatories. The Big Bang framework, supported by the cosmic microwave background and observed metric expansion, serves as the standard cosmological model. Within this framework, dark matter and dark energy—inferred respectively from gravitational dynamics and accelerating expansion—remain central observational and theoretical problems.

Why it matters

Empirical cosmological discoveries have revised physical models of space, time, and cosmic history. The field also provides quantitative boundary conditions for particle physics, astrophysics, and the philosophy of science.

What it builds on

Where it leads

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