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Physics
Astrophysics
Cosmology
Structure and evolution of the universe
Large-scale structure of the universe
Cosmic web and its components
Clusters and superclusters
Filaments and voids
Evolutionary models
Hierarchical structure formation
Simulation models and predictions
Observational evidence and refinements
Big Bang theory
Fundamental principles
Initial singularity
Expansion and cooling processes
Formation of fundamental particles and forces
Evidence and implications
Redshift and Hubble's observation
Light element abundance
Cosmic microwave background radiation
Discovery and characteristics
Anisotropies and polarization
Insights on early universe conditions
Dark Matter and Dark Energy
Composition and properties of dark matter
Candidates (WIMPs, axions, MACHOs)
Direct and indirect detection methods
Effects on galaxy rotation curves
Dark energy and its role in cosmology
Cosmological constant vs. quintessence
Influence on large-scale structure formation
Integrated Sachs-Wolfe effect
Effects on universal expansion
Impact on cosmic acceleration
Relationship with cosmological parameters
Experimental observations and constraints
Expansion of the Universe
Hubble's Law and redshift
Velocity-distance relation
Implications for cosmological models
Accelerating universe
Type Ia supernovae as standard candles
Implications for energy density components
The role of dark energy
Observable universe and its boundaries
Cosmic horizon and light cone
Implications for observable phenomena
Limits of current observational capabilities
Cosmic Inflation
Theoretical basis and motivation
Horizon and flatness problems
Predictions of the inflationary model
Models of inflation
Slow-roll inflation
Chaotic and eternal inflation
Evidence and observational tests
Density fluctuations and primordial perturbations
Impacts on cosmic microwave background
Quantum Cosmology
Quantum gravity theories
Loop quantum gravity
String theory and M-theory implications
Early universe conditions
Quantum fluctuations
Role in the formation of large-scale structures
Implications for the multiverse hypothesis
Future of the Universe
Different cosmological scenarios
Big Freeze (heat death)
Big Rip and Big Crunch
Cyclic models and bounce theories
Long-term astrophysical processes
Star and planet evolution
Fate of black holes and other compact objects
Potential role of life in cosmic evolution
2. Celestial Bodies
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4. Astrophysical Phenomena