The Hubble parameter (H) describes the expansion rate of the universe at any given time. Its present-day value, the Hubble constant (H₀), is about 70 km/s/Mpc and is a cornerstone of modern cosmology, linking the age, composition, and fate of the cosmos.
The Higgs mechanism explains how elementary particles acquire mass through interaction with the Higgs field. This field, which permeates all of space, broke symmetry in the early universe and gave rise to the masses of W and Z bosons while leaving the photon massless, a cornerstone of the Standard Model.
Big Bang Nucleosynthesis (BBN) uses the primordial abundances of light elements to limit the number of neutrino species. This article explains the physics behind the constraint, the role of cosmic epochs, and the current evidence from cosmology.
The 21-cm line is a faint radio emission from neutral hydrogen atoms, produced by a spin-flip transition. It is a powerful tool for mapping the Milky Way and probing the early universe, including the cosmic Dark Ages and the epoch of reionization.
The flatness problem is a cosmological fine-tuning puzzle: why is the universe so precisely flat when standard Big Bang theory predicts it should curve over time? Inflation offers a compelling solution, and measurements from COBE, WMAP, and Planck confirm the near-perfect flatness of space.
The COBE satellite measured the cosmic microwave background (CMB) with unprecedented precision, confirming its perfect blackbody spectrum and detecting the tiny anisotropies that seeded galaxies. Its findings solidified the Big Bang model and opened the era of precision cosmology.
The cosmological principle—the assumption that the universe is homogeneous and isotropic on large scales—underpins modern cosmology. This article explores how astronomers test it using galaxy surveys, the cosmic microwave background, and baryon acoustic oscillations, and examines recent challenges and the current scientific consensus.
Primordial gravitational waves are ripples in spacetime generated during cosmic inflation. They leave a unique imprint called B-modes in the polarization of the cosmic microwave background, offering a direct window into the universe’s first fraction of a second and the physics at energies far beyond particle accelerators.
This comprehensive guide explains how astronomers measure galaxy redshift and uses that measurement as a key to understanding the origin and evolution of the universe, from the Planck epoch to the present day. It includes a detailed timeline of cosmic epochs, the role of the cosmic microwave background, and the missions that revealed them.
CMB lensing is the subtle gravitational deflection of cosmic microwave background photons by dark matter and large-scale structure. It turns the oldest light into a backlight that maps the invisible dark matter distribution. Measurements from Planck and future experiments use this effect to constrain dark matter, neutrino masses, and the growth of cosmic structure.
