Research in Cosmic Microwave Background (CMB) is a crucial aspect of modern cosmology, offering  valuable insights into  the early universe and its evolution. Here are some key areas of research in CMB.

  • Cosmic Origins: Investigating the origins and properties of the CMB to understand the initial moments of the universe after the Big Bang.
  • Cosmological Parameters: Using CMB data to constrain and refine cosmological models, determining parameters like the Hubble constant, density of dark matter and dark energy, and the overall geometry of the universe.
  • Inflationary Cosmology: Studying the imprint of cosmic inflation on the CMB to gain insights into the universe’s rapid expansion in its early stages.
  • Cosmic Structure Formation: The seeds of cosmic structure, including galaxies and galaxy clusters, are imprinted in the CMB. Understanding the formation and evolution of these structures is a key focus of research.
  • Observational Techniques: Utilizing advanced telescopes and instruments to measure the CMB’s temperature and polarization with high  precision.