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Cosmological Time Dilation Interval Pair

Apply cosmological observed-to-rest interval factor 1+z using an explicit redshift greater than minus one.

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Description

Apply a supplied cosmological redshift time-dilation factor.

Cosmological quantities depend on scale factor, redshift, distance definition and the dimensionless Hubble parameter h. Proper and comoving distances differ at a specified epoch, and h-scaled units differ from the dimensional Hubble constant. A scalar rescaling or model contribution preserves supplied conventions without fitting a cosmology or inferring an observed distance.

Apply a supplied cosmological redshift time-dilation factor.

When to use this tool

Use Cosmological Time Dilation Interval Pair when you already have restInterval, redshift and need to apply a supplied cosmological redshift time-dilation factor.

How to use the tool and how it works

  1. Enter restInterval, redshift. 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 observedInterval, dilationFactor. Use the output convention below.

Require restInterval>=0 and redshift>-1; return factor=1+z and observedInterval=restInterval*factor.1

Cosmological redshift stretches an emitted time interval by 1+z. Applying that factor does not identify a source redshift or remove other timing effects.2

Input fieldMeaning and unitsAccepted input
restIntervalNonnegative interval in the desired time unit; observedInterval uses the same unit.Required. Finite number; minimum 0.
redshiftDimensionless z>-1; dilation factor=1+z.Required. Finite number; strictly above -1.
Output fieldInterpretationReturned shape
observedIntervalObserved IntervalRequired. Finite number.
dilationFactorDilation FactorRequired. Finite number.
json
{
  "input": {
    "restInterval": 10,
    "redshift": 2
  },
  "output": {
    "observedInterval": 30,
    "dilationFactor": 3
  }
}

Limitations and assumptions

  • Matching time units and the stated source/observer convention are assumed. No redshift, distance, local clock correction or other source of time dilation is determined.
  • 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 the complete cosmological model and its parameter, epoch and unit definitions for a physical inference. Review redshift, distance, lensing and spectrum conventions before combining these local terms; they do not perform line-of-sight integration, parameter estimation or uncertainty analysis.

References

  1. Calculation and input contract: cosmology/cosmological-time-dilation-interval-pair — tool.io

  2. Distance measures in cosmology — David W. Hogg

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