Comoving volume cosmology

  • How do you calculate comoving volume?

    The total, comoving volume to a comoving distance d is just V=4πd3/3, so the volume of the shell between z=2 and z=3 is V2→3=V3u221.

    1. V2=4π3(d33−d32)
    2. .Jun 16, 2021

  • What are comoving coordinates in cosmology?

    A comoving coordinate system is a reference frame that expands in tandem with the expansion of the Universe, thus factoring out the effect of the Hubble expansion..

  • What does comoving mean in cosmology?

    Comoving distance and proper distance.
    Comoving distance is the distance between two points measured along a path defined at the present cosmological time.
    For objects moving with the Hubble flow, it is deemed to remain constant in time..

  • What is redshift and comoving distance?

    The line-of-sight comoving distance between two nearby events (ie, close in redshift or distance) is the distance which we would measure locally between the events today if those two points were locked into the Hubble flow..

  • What is the comoving volume as a function of redshift?

    The comoving volume VC is the volume in which the number densities of non-evolving objects locked into the Hubble flow are constant with redshift.
    It is the proper volume times three factors of the relative scale factor from the present epoch to the time at redshift z, or (1 + z)3..

  • What is the formula for comoving distance?

    The comoving distance should be calculated using the value of z that would pertain if neither the object nor we had a peculiar velocity.
    Together with the scale factor it gives the proper distance at the time: d = a d C..

  • The comoving distance (line of sight) DC between two nearby objects in the Universe is the distance between them which remains constant with epoch if the two objects are moving with the Hubble flow.
  • The comoving distance should be calculated using the value of z that would pertain if neither the object nor we had a peculiar velocity.
    Together with the scale factor it gives the proper distance at the time: d = a d C.
The comoving volume V

What is comoving volume?

It can be thought of as the cosmological volume with the expansion of the Universe factored out, i.e. the comoving volume defined by a fixed set of objects remains constant, and is useful in cosmological calculations.
All material is © Swinburne University of Technology except where indicated.

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What is the comoving distance based on observational methods?

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