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  2. Intensity mapping - Wikipedia

    en.wikipedia.org/wiki/Intensity_mapping

    In cosmology, intensity mapping is an observational technique for surveying the large-scale structure of the universe by using the integrated radio emission from unresolved gas clouds. In its most common variant, 21 cm intensity mapping, the 21cm emission line of neutral hydrogen is used to trace the gas. The hydrogen follows fluctuations in ...

  3. Hydrogen line - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_line

    An atom of neutral hydrogen consists of an electron bound to a proton.The lowest stationary energy state of the bound electron is called its ground state.Both the electron and the proton have intrinsic magnetic dipole moments ascribed to their spin, whose interaction results in a slight increase in energy when the spins are parallel, and a decrease when antiparallel.

  4. Tianlai experiment - Wikipedia

    en.wikipedia.org/wiki/Tianlai_experiment

    Tianlai Arrays. The Tianlai experiment (Chinese: 天籁) is a radio astronomy experiment run by the National Astronomical Observatories, Chinese Academy of Sciences (NAOC). [1] [2] Its aim is to develop the key techniques of intensity mapping observation for the redshifted 21cm line of neutral hydrogen, in order to probe the large-scale structure, and to detect and measure the dark energy ...

  5. Canadian Hydrogen Intensity Mapping Experiment - Wikipedia

    en.wikipedia.org/wiki/Canadian_Hydrogen...

    The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is an interferometric radio telescope at the Dominion Radio Astrophysical Observatory in British Columbia, Canada which consists of four antennas consisting of 100 x 20 metre cylindrical parabolic reflectors (roughly the size and shape of snowboarding half-pipes) with 1024 dual-polarization radio receivers suspended on a support above ...

  6. File:JWST early Universe observations and ΛCDM cosmology.pdf

    en.wikipedia.org/wiki/File:JWST_early_Universe...

    English: JWST early Universe observations and ΛCDM cosmology.Deep space observations of the JWST have revealed that the structure and masses of very early Universe galaxies at high redshifts (z ∼ 15), existing at ∼0.3 Gyr after the Big Bang, may be as evolved as the galaxies in existence for ∼ 10 Gyr.

  7. Cosmography - Wikipedia

    en.wikipedia.org/wiki/Cosmography

    In astrophysics, the term "cosmography" is beginning to be used to describe attempts to determine the large-scale matter distribution and kinematics of the observable universe, dependent on the Friedmann–Lemaître–Robertson–Walker metric but independent of the temporal dependence of the scale factor on the matter/energy composition of the Universe.

  8. Microcosm–macrocosm analogy - Wikipedia

    en.wikipedia.org/wiki/Microcosm–macrocosm_analogy

    The view itself is ancient, and may be found in many philosophical systems world-wide, for example in ancient Mesopotamia, [5] in ancient Iran, [6] or in ancient Chinese philosophy. [7] However, the terms microcosm and macrocosm refer more specifically to the analogy as it was developed in ancient Greek philosophy and its medieval and early ...

  9. Cosmochemistry - Wikipedia

    en.wikipedia.org/wiki/Cosmochemistry

    Meteorites are often studied as part of cosmochemistry. Cosmochemistry (from Ancient Greek κόσμος (kósmos) 'universe' and χημεία (khēmeía) 'chemistry') or chemical cosmology is the study of the chemical composition of matter in the universe and the processes that led to those compositions. [1]