In Mathematics for Taking Another Look at the Universe, I presented this:
One of the
implications of this chart might not be immediately apparent. Look at the event at t=10,000 million
years ago that can be observed today.
Back at that time, there was a proper distance between the event
location and the observer location of 2,963 million light years.
To reach the
observer, the photon must traverse that proper distance plus the additional distance
due to expansion of space. There are two
odd things about this chart.
For the first, note
that the dashed purple line that intersects with the event (xevent,tevent)
and has a proper distance at t=0 of ctevent. If an event happened at time tevent
ago, then the apparent distance would be that time multiplied by the speed of
light, so also ctevent.
Which means the proper distance of an observable event’s location (at time
of observation) is equal to its apparent distance. This might sound intuitively correct to some,
but intuitively incorrect to others.
The space that any photon traverses will be expanding the whole time and across the whole distance. Consider when a photon has traversed half of
the initial proper distance (that is to say it is at the location that would have
been half of the proper distance at the time that the photon was emitted). The space that it has traversed will have
expanded to some extent already, but any further expansion will not be
experienced by the photon. Therefore, it
seems reasonable to imagine that the location from which a photon is emitted will
end up further away from the observer than the transit time multiplied by the speed
of light.
But this is
apparently not the case per the logic above.
The other oddity is
that the apparent path of a photon from an observed event 10,000 million years ago will end
up further away from the observer before closing in on that observer and eventually
being observed. This does not seem correct
at all. Recall that in a FUGE universe, there is no recession greater
than the speed of light which means, intuitively, that the location of observable events should be at locations greater than ct, where t is the
transit time (as per the above) and the photons should never have a greater proper
distance from the observation location than at the time of emission.
However, the curve should not be considered to be the path of a specific photon. Instead it represents the origin events of all photons that could possibly be observed at t0.
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Imagine a
stationary emitter of some sort, sending photons in our direction for all time. The only motion of that emitter relative to
the observer is due to recession (which in turn is due to expansion).
In this cleaned up
version of the chart, we can see the dashed purple line from t=0 to t≈t0,
which plots the proper distance to the emitter from the observer location over
time (I am going to refer to the proper distance to the emitter as d(t)
in an attempt at clarity). The
approximate symbol is used for the latter time because as t→t0
granularity becomes more of a problem, you can’t really distinguish between
locations when the entire universe has a radius of one unit of Planck length. When t≈t0, the proper
distance to the proper distance between of the notional locations of the hypothetical
emitter and the observer is, effectively, d(t0)=0. At the time of observation, t=0, as
discussed above, d(0)=ctevent.
Again for clarity, “proper
distance” (at least how I am defining it) is the distance given by the time
that it would a photon to travel from one location to another times the speed
of light, if there were no expansion. Wikipedia (paraphrasing from here) explains it like this: “The proper
distance d(t) between two
galaxies at time t is just the distance that would be measured
by rulers between them at that time.”
There are problems with both definitions, but hopefully the concept is
sufficiently clear. Compare with comoving
distances, which don’t
change with expansion (imagine a ruler between two locations was elastic and
stretched at the same rate at which space expanded between those locations, so
the measured distance would never change).
The dashed purple line
can be expressed as:
d(t)=m(t-φ)
The t-intercept,
φ, is merely the value of t when d(t)=0, so φ=t0.
The gradient, m,
can be found by using any two points on the line. We will use the two that we have already
discussed, in the form (0,t0). So, (ctevent,0) and (x2,t2)
and:
m=(d2-d1)/(t2-t1)=-ctevent/t0
Therefore:
d(tevent)=-ctevent/t0.(tevent-t0)=ctevent.(t0-tevent)/t0
Generalising (by removing
the subscript “event”), and noting that x=ct:
d(t)=x.(t0-t)/t0
Multiplying through
by c/c:
d(t)=x.(ct0-ct)/ct0=x.(ct0-x)/ct0=x'
So, for any observable
event, the proper time to that event (at the time of the event), is as
calculated and charted above.
Following the logic
that every observable event is equivalent to a photon emitted at that event (ignoring
energy/frequency/wavelength because we only care about observability). Observed photons that originated at sufficiently distant events (distant in time) must – at first – increase their proper distance from the
observer as we consider incrementally closer origin events (closer in time).
The question then
is … how can that be?
It’s a matter of interpretation. We could select any event along the curve, but
we will stick with an observable event that emitted a photon 10,000 million
years ago.
That photon travels
toward us (when the universe is such that t0=13,800 million
years), at a rate of c, from a location with a proper distance (at that
time) of x'(10,000)=2,753 million light years. Consider this to be the length of a racetrack
along which the photon must travel to reach us.
At that time, where æ is the age of the universe (we need another symbol because t in the equations above expresses time since an event), H(æ=3,800)=0.000263Mly/ly/Mly – using unusual, but significantly more convenient units for this purpose. A location at a distance of 2,753 light years at that rate, will recess by H(3,800).x'(10,000).Δt=36.2 million light years, where Δt=t1-t2=50 million years. So the photon’s position on the racetrack (after Δt=50 million years) will be 2,740 million light years away. However, the entire racetrack along which the photon is travelling will have expanded by a factor of 1+H(3,800).Δt, which gives us a proper distance of x'(9,950)=2,775 million light years – which is a greater distance than we started with. The relevant equation, when generalised, is:
x'(t-Δt)=(x'(t)+H(t0-t).x'(t).Δt-c.Δt).(1+H(t0-t1).Δt)
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The equation above does not look at all like the equation for x' that we have discussed recently. But it is the very same, just expressed differently. What follows is the proof.
Using x=ct
so that x'(t)=ct.(ct0-ct)/ct0 and H(æ)=H(t0-t)=1/(t0-t):
x'(t-Δt)=(ct.(ct0-ct)/ct0+Δt.ct.(ct0-ct)/ct0/(t0-t)-c.Δt).(1+Δt/(t0-t))
Rationalising:
x'(t-Δt)=(ct.(t0-t)/t0+Δt.ct/t0-c.Δt).(1+Δt/(t0-t))
Multiplying the blue term by t0/t0 and rearranging, noting that the green
term above is just the blue term in a different configuration:
x'(t-Δt)=(ct.(t0-t)/t0.+Δt.c.(t-t0)/t0).(1+Δt/(t0-t))
Multiplying the second
bracket by (t0-t)/(t0-t):
x'(t-Δt)=(ct.(t0-t)/t0.+Δt.c.(t-t0)/t0).((t0-t)+Δt)/(t0-t)
Rationalising and rearranging
the terms in the second pair of brackets:
x'(t-Δt)=(ct/t0.+Δt.c/t0).(t0-(t-Δt))
Rearranging:
x'(t-Δt)=c.(t-Δt).(t0-(t-Δt))/t0
Multiplying through
by c/c:
x'(t-Δt)=c(t-Δt).(ct0-c(t-Δt))/ct0
If x'(t-Δt)=x'2,
we could by extension say that x2=c.(t-Δt), and thus:
x'2=x2.(ct0-x2)/ct0
Which, while not arrived at by the most intuitive of proofs (I've tried to make it as clear as possible above), is precisely what we should expect.
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The above has been edited to address a misconception with regard to the OE curve - which is not, as previously and erroneously suggested, a representation of the path of any individual photon.
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