Accelerating expansion of the universe

Related lectures (30)

Covers the generation of primordial magnetic fields and their backreaction effects in cosmology.

Explores dark energy, the cosmological constant, and their impact on the universe's expansion under various scenarios.

Explores photon propagation, light emission and reception, energy, spectra, flux, intensity, Doppler and red-shift, and universe expansion.

Delves into gravitational instability, structures formation, and CMB temperature, exploring the inhomogeneities in the Universe.

Covers the Doppler-Fizeau effect in astrophysics, including redshift, star rotation, and the search for exoplanets.

Covers the Doppler-Fizeau Effect, redshift, gas cloud motion, and exoplanet search.

Covers the Hubble law derivation and cosmological parameter determination from supernova observations.

Covers numerical methods in hydrodynamics, ideal fluids, plasma universe, dark matter simulation, and baryon modeling.

Discusses the thermal history of the universe and the Cosmic Microwave Background's significance in cosmology.

Explores the evolution of the Universe, from its early stages to the present, covering topics such as astroparticle physics and the thermal history.

Covers the basics of astrophysics, including the structure of the universe and key research concepts.

Explores wave propagation, wave packets, and the Doppler effect for mechanical and electromagnetic waves, including Hubble's law.

Explores the reformulation and resolution of a generalized dissipative oscillator.

Explores Hubble's observations of the early universe, redshift, cepheid stars, and type Ia supernovae.

Explores the Variable Universe through the Cosmic Distance Ladder, focusing on standard candles and the Hubble constant tension.

Covers astroparticle physics, focusing on cosmic rays, dark matter, and the universe's expansion.

Covers cosmology from the big bang to present day, including astrophysics and Hubble's law.

Delves into cosmological relaxation through the dark axion portal and its implications for understanding nature.

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