Spacetime expansion effects on wavelength of travelling light

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SUMMARY

The discussion centers on the effects of cosmological expansion on the wavelength of light traveling through space. It confirms that the redshift of light, denoted by the factor 1+z, occurs due to the expansion of the universe, which is tracked using the scale factor a(t). Specifically, when z = 1, distances and wavelengths double, indicating that the current scale factor a(now) is twice that of a(then) when the light was emitted. This understanding is crucial for accurately interpreting observations of Type Ia supernovae and the rate of cosmic expansion.

PREREQUISITES
  • Understanding of cosmological redshift and its implications
  • Familiarity with the scale factor a(t) in cosmology
  • Knowledge of Type Ia supernovae as standard candles in distance measurement
  • Basic principles of light propagation in expanding mediums
NEXT STEPS
  • Research the mathematical derivation of redshift in cosmology
  • Explore the role of the scale factor a(t) in cosmological models
  • Study the implications of Type Ia supernovae on measuring cosmic distances
  • Investigate the effects of gravitational lensing on light from distant galaxies
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Astronomers, cosmologists, and physics students interested in understanding the implications of cosmic expansion on light propagation and distance measurements in the universe.

H2Bro
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Hello,

Do current theories of cosmological expansion take into account the effects expanding space would have on a beam of light traveling through space? i.e. if an expanding medium of gas with constant pressure decreases the temperature/velocity of particles, would an expanding medium of space decrease the velocity of light? (not sure what the analog of pressure is for spacetime...)

given light's constant speed I assume this would actually redshift the wavelength akin to light exiting supermassive objects. If unaccounted for, this effect might mean observations of SN1A events overestimate distance as well as rate of expansion.
 
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The normal way to think about cosmological redshift is as an expansion effect. It is handled pretty much as your post suggests.

During transit the light's wavelength increases by a factor of 1+z, and that happens if distances in the U have increased by a factor of 1+z while the light was traveling.

Cosmologists use a time dependent number a(t) called "scale factor" to keep track of distances.

If z = 1 that means distances (and wavelengths) have doubled. That means the ratio of scalefactor NOW a(now) to scalefactor THEN when light was emitted is
a(now)/a(then) = 2. Distances now are twice as big as when light was emitted and started on its journey to us.

These are LARGESCALE distances between widelyseparated points each of which is at rest relative to the cosmic background radiation. Not smallscale distances within our solarsystem or galaxy.
 

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