Connect redshift to expansion ratios without a speed shortcut
Cosmological redshift is the ratio of observed to emitted wavelength minus one. In a homogeneous expanding background with present scale factor one, 1+z=1/a_emit. The scale factor relates large-scale comoving separations; it does not imply that every atom, star or bound galaxy expands with the same rule.
Learning outcome: Close wavelength, energy, time and scale-factor ratios, then identify the additional expansion-history assumptions required for a distance.
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Keep galaxy mass, source calibration, expansion history and independent cosmological evidence distinct.
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At z=1 and emitted 600 nm, the scale factor is 0.5, observed wavelength 1200 nm, photon-energy ratio 0.5 and time-stretch factor 2. The supplied adiabatic background temperature is 5.451 K, not the temperature of every emitting object.
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Does one redshift by itself specify a unique distance or lookback time?
Experiment
Close wavelength, energy, time and scale-factor ratios, then identify the additional expansion-history assumptions required for a distance.
Connect scale factor, photon wavelength and time intervals
Worked teaching model · synthetic values · Original homogeneous expansion with present scale factor 1: a_emit=1/(1+z), lambda_obs=(1+z)lambda_emit, photon energy ratio 1/(1+z), time-stretch 1+z. Reference radiation temperature 2.7255 K scales as 1+z under adiabatic expansion; no peculiar-speed conversion.
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Cosmological redshift connects expansion ratios, not a universal special-relativistic peculiar speed.
Original homogeneous expansion with present scale factor 1: a_emit=1/(1+z), lambda_obs=(1+z)lambda_emit, photon energy ratio 1/(1+z), time-stretch 1+z. Reference radiation temperature 2.7255 K scales as 1+z under adiabatic expansion; no peculiar-speed conversion.
| Quantity | Value | Unit |
|---|---|---|
| Emission scale factor | 0.5000000 | ratio to present |
| Observed photon wavelength | 1200 | nm |
| Observed/emitted photon energy | 0.5000000 | ratio |
| Observed/emitted time interval | 2 | ratio |
| Adiabatic radiation temperature at emission | 5.451000 | K |
These supplied models are not current measured cosmological parameters, a new galaxy discovery or independent actual observing evidence.
Cosmological redshift connects expansion ratios, not a universal special-relativistic peculiar speed.
Original homogeneous expansion with present scale factor 1: a_emit=1/(1+z), lambda_obs=(1+z)lambda_emit, photon energy ratio 1/(1+z), time-stretch 1+z. Reference radiation temperature 2.7255 K scales as 1+z under adiabatic expansion; no peculiar-speed conversion.
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At z=2 and emitted 400 nm, find observed wavelength, emission scale factor and background reference temperature.
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