Spacetime expansion effects on wavelength of travelling light

AI Thread Summary
Current theories of cosmological expansion account for the effects of expanding space on light traveling through it, resulting in redshift akin to light escaping supermassive objects. As light travels, its wavelength increases by a factor of 1+z, corresponding to the expansion of distances in the universe. Cosmologists utilize a time-dependent scale factor, a(t), to track these distances, indicating that if z = 1, distances have doubled since the light was emitted. This redshift phenomenon primarily pertains to large-scale distances between points at rest relative to cosmic background radiation, rather than small-scale distances within our solar system or galaxy. Understanding these dynamics is crucial for accurate observations of distant supernovae and the universe's expansion rate.
H2Bro
Messages
164
Reaction score
4
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.
 
Astronomy news on Phys.org
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.
 
Is a homemade radio telescope realistic? There seems to be a confluence of multiple technologies that makes the situation better than when I was a wee lad: software-defined radio (SDR), the easy availability of satellite dishes, surveillance drives, and fast CPUs. Let's take a step back - it is trivial to see the sun in radio. An old analog TV, a set of "rabbit ears" antenna, and you're good to go. Point the antenna at the sun (i.e. the ears are perpendicular to it) and there is...
This thread is dedicated to the beauty and awesomeness of our Universe. If you feel like it, please share video clips and photos (or nice animations) of space and objects in space in this thread. Your posts, clips and photos may by all means include scientific information; that does not make it less beautiful to me (n.b. the posts must of course comply with the PF guidelines, i.e. regarding science, only mainstream science is allowed, fringe/pseudoscience is not allowed). n.b. I start this...
Back
Top