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Cosmological Lookback Time Local Increment Tool

Local differential dtLookback=dz/[(1+z)*H(z)], rather than a finite-redshift integration.

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Description

Return a local lookback-time increment.

Cosmology uses several distance measures and often expresses the expansion rate in mixed astronomical units. Scale-factor relations, inverse-Hubble scales and relativistic velocity composition answer different questions; units and the distinction between local algebra and an integrated expansion history are essential.

Return a local lookback-time increment.

When to use this tool

Use Cosmological Lookback Time Local Increment when checking one explicit cosmological distance, redshift-factor or unit convention.

How to use the tool and how it works

  1. Enter redshift, redshiftIncrement, hubbleAtRedshift. Use the units and conventions below.
  2. Run the tool. Correct any format, range, or cross-field input error before interpreting the output.
  3. Read lookbackIncrement. Use the output convention below.

Return a local lookback-time increment. Require z > -1 and hubbleAtRedshift > 0; increment = redshiftIncrement/((1+z)*H(z)).1

Cosmological distance, volume and lookback-time relations require the appropriate expansion-rate and distance conventions; local factors do not replace integration.2

Input fieldMeaning and unitsAccepted input
redshiftDimensionless redshift z; the stated scaling formulas require z > -1.Required. Finite number; strictly above -1.
redshiftIncrementRedshift IncrementRequired. Finite number.
hubbleAtRedshiftHubble At RedshiftRequired. Finite number; strictly above 0.
Output fieldInterpretationReturned shape
lookbackIncrementSigned differential lookback-time contribution in inverse-Hubble time units; not a finite integral.Required. Finite number.
json
{
  "input": {
    "redshift": 1,
    "redshiftIncrement": 0.1,
    "hubbleAtRedshift": 2
  },
  "output": {
    "lookbackIncrement": 0.025
  }
}

Limitations and assumptions

  • H sets inverse-time units; this differential step is not a finite-bin integral or a complete universe-age calculation.
  • Inputs must satisfy both the field types and the cross-field conditions above. Invalid input causes an error; a successful false flag or documented placeholder is a different result.
  • Numeric calculations use binary floating point unless exact decimal-integer arithmetic is explicitly stated. No hidden measurement tolerance or decimal rounding is added; nonfinite or out-of-contract results are rejected. Numeric signed-zero results are exported as zero.

Alternative or Complementary methods

Use a complete cosmological distance/time calculation and the appropriate observation model when an actual source distance, age or velocity is required.

References

  1. Calculation and input contract: cosmology/cosmological-lookback-time-local-increment — tool.io

  2. Distance measures in cosmology — David W. Hogg

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