Nevertheless, the mirror thing can be falsified. You just have two mirrors in a vacuum in the same place moving relative to each other. Shine a light pulse at it and detect the reflected light from each. If they arrive at the same time (but different wavelength/frequency), then light speed is not a function of the motion of the mirrors. If light from the approaching mirror gets there first, then we need to rewrite the last 130 years of physics. — noAxioms
I sent a post concerning this in the “The Newtonian gravitational equation seems a bit odd to me" thread.
— Gampa Dee
Which I did not immediately see because you didn't reference me (reply to something of mine say) anywhere in it. — noAxioms
Therefore, it would have predicted the nul result because of this....the light was going to be c relative to the whole experiment
— Gampa Dee
OK, so the M&M setup isn't the optimal experiment to falsify this particle theory. — noAxioms
If the combined velocity of reflected light, in the reference frame of the laboratory, is (c + v), then the ballistic theory, in question, is a new-source theory, in which starlight loses its initial velocities. By contrast, if the combined velocity of reflected light, in the reference frame of the laboratory, is (c + 2v) instead, then the ballistic theory, in question, is an elastic-impact theory, in which starlight does not lose its initial velocities. — Foraj
OK, I got that. I know the difference between the two now. They're both wrong, but they didn't know it at the time. Not sure if the spectra of binaries can falsify both since apparently the new-source theory produces spectra very similar to relativity theory (reflected light speed is neither c+v nor c+2v, but just c. — noAxioms
Check the copyright. Is it legal to paste the whole thing here? You already pasted an email address, which is against the rules for some forums.
What question do you need answered? — noAxioms
So,the addition of vectors in this case is 0...but relative to what?
As I said, it doesn't yield anything meaningful. I don't like the example text. It obfuscates more than it clarifies anything.
It also mixes metric (kg mass) with American units (mi/hr). That's unforgivable in a physics text.
Their momentum vectors seem to have a ratio of about 4, but the text says the ratio is closer to 7. That's poor graphics. — noAxioms
Again,we have a momentum,of -111 kgm/s....what does that even mean?
Just what it says. For instance, if, in space (no friction with road), the car were to hit the truck and stick to it in a tangled wreck, the new 5200 kg mass would be moving left at about 21 m/sec to the left, the total momentum / total mass. Momentum is conserved in a closed system. I put them in space to keep it closed since the road would very much be exerting forces if it was there. — noAxioms
I’ve read some things concerning vector additions that I just don’t get, which maybe you could help me out with.
— Gampa Dee
Maybe. Don't know the problem.
You mean the equation a = GM/r² ? I suppose that would need a unit vector to make it into a vector acceleration and not just a scalar. Nothing on the right side as I wrong it is a vector. — noAxioms
It seems that this would imply the light as having a speed of .5c relative to the mirror
Well, no. In the scenario I outlined, when moving up it has a speed of .134c relative to the mirror, and in the reverse direction the relative speed would be 1.866. That still presumes light is independent of emitter speed. — noAxioms
With emission theory, you'd have to specify the speed of emission, not obvious with a light clock which just reflects the pulse back and forth and has no obvious emission event. I am also unsure what emission theory says about how the speed gets altered when hitting a moving mirror. — noAxioms
If you’re speaking of an observer moving at .866c, relative to the frame of the clock
I wasn't. I was speaking of the clock moving at .866c relative to the ether. Neither the observer nor the frame plays any role in the predictions. That's the general model that the M&M experiment was trying to measure. — noAxioms
I would be interested in learning more about the scientific jargon...I will try to read up on this more.
If you accelerate at 10 m/sec² for 100 million seconds, you achieve a rapidity (or proper velocity) of a billion m/sec. You just add 10 a hundred million times.
But to compute velocity relative to the frame in which you were initially stationary, you add 10 using relativistic addition, all those times. The former adds up to about 3.3c, meaning at that rapidity you move 3.3 light years for every year of your travel. But the velocity is .997c relative to Earth. That sort of illustrates the difference. So if your ship is fast enough, you can cross the 100,000 LY galaxy before you die because there's no upper limit to rapidity. — noAxioms
here's the link that I told you about concerning the "double star experiement"....I hope it works.
Doesn't work. It's just a pdf file name without a website in front of it. I tried searching the web for any site containing that file name and got nothing.
I am interested. Tried googling it, but the name is too generic to get to what you're talking about.
Sure, 2 orbiting stars will alternate approaching and receding, but that just results in redshift and blueshift. I don't know how they'd decide that the images being looked at departed at the same time, so to speak. — noAxioms
From what I understand, in the M&M experiment, the velocity of the light would be c through all paths within a particle theory of light.
— Gampa Dee
Special relativity theory (early 20th century) posited the frame independent fixed speed (not velocity, which is frame dependent) of light. The M&M experiment (late 19th century) neither presumed nor demonstrated the fixed frame independent speed of light.
The speed of light is not dependent on whether one uses a particle or wave model for it. — noAxioms
I don’t understand why you say one path would be longer than the other?
Picture a light clock moving at 0.866c with mirrors separated by a distance of 1. Presume no length contraction. Move the clock with the mirrors to the sides. Light travels a distance of 1 to the left and 1.732 up to get to the other side, a total distance of 2. Another 2 to get back. So it runs at half speed since it has a distance of 4 to go instead of 2 when the clock is stationary. — noAxioms
that is, the receding galaxies with a velocity greater than c would not be interpreted as having those velocities.
Technically, they're rapidities, not velocities. The former adds the normal way (a+b) as opposed to velocity with adds the relativistic way, in natural units: (a+b)/(1+ab) — noAxioms
The better empirical evidence would be something like seeing incoming ejecta before seeing the explosion that caused it, or seeing a star explode well before the neutrinos hit instead of the observed neutrinos coming just before the light. — noAxioms
I agree with what you wrote, except, the Newtonian model would have predicted a null result as Newton believed that light was made up of particles.
— Gampa Dee
Yes and no. Particles would also have taken longer to go the greater distance with the grain than the shorter distance against it.
But the interferometer used by M&M leverages the wave nature of light, something known back in Newton's time since particles don't explain rainbows. I don't know when interferometers were invented. — noAxioms
Einstein claimed the light’s velocity is invariant without any specific reason why
Empirical evidence? Einstein didn't originate the claim. He just ran with it without dragging in the baggage that everybody else tried to keep. — noAxioms
it seems to me that Fitzgerald allowed a mechanism for the length contraction to exist, being the ether, whereas Einstein did not have any mechanism
The heck he didn't. It was explained via Minkowskian geometry. The contraction (and the underlying 4D geometry) derives directly from the frame-invariant speed of light, even if there was a preferred frame. The geometry and contraction were both a byproduct of the work of Minkowski and Lorentz, so that too wasn't something Einstein originated. Lorentz was first, but clung to the 3D ether model like Fitzgerald. That model added complications preventing the special version of the theory coming out before Einstein's, and preventing a general version from coming out until nearly a century after Einstein's. — noAxioms
As I said, there are some empirical tests one can perform to see who is right, but not that one where results can be physically published in a journal. — noAxioms
for what I understand...and for me, it seems that the postulate of the invariant speed of light would fall into the "extraordinary claims require extraordinary evidence” category.
OK. For me it falls under Occam's razor: The simpler model is the more likely one, proposing the fewest additions and complications. — noAxioms
My “personal” opinion would be that the particle theory, which would have predicted a null result
It predicted no such thing since the particle would have longer to go this way than that way. The contraction (which both theories describe, but Newton does not) explains the null result of M&M. — noAxioms
But, what if the light speed was c relative to the source (sort of particle theory)
Then an easy experiment would show it. As I said, this is easily falsified.
The binary star thing doesn't work since there is no way to know when the light you're looking at was emitted. Both stars continuously emit light. You need two relatively moving sources that simultaneously, in each other's presence, emit a short pulse. The further away the emitter the better since it would give one pulse more time to outrun the other, showing up as two pulses at different times at the detector. No such thing is seen. — noAxioms
Distant galaxies receding over c would not be visible due to the light approaching too slowly to stay inside our event horizon, but there they are, with Webb telescope finding ever more distant ones. The visible universe would be far smaller if light speed was dependent on emitter motion. — noAxioms
The length contractions in Fitzgerald's theory is the same as that in Einstein's special relativity - they are both Lotentz transformations. The difference is that in Fitzgerald's theory the frame of reference of the ether was a privileged frame of reference in which light traveled, while Einstein showed that the ether was not needed in the theory and that the frame of reference can be any inertial frame of reference. — PhilosophyRunner
To put is more simply:
According to Fitzgerald: Light traveled in the ether frame of reference. This frame of reference was moving relative to an observer on Earth. Lorentz transformations can be used to explain length contractions due to the observer and ether being in different frames of references.
According to Einstein: The ether is not needed in the theory. Length contractions due to Lorentz transformations are observed when the observer is in a different inertial frame of reference to the experiment, but this is not relevant to the M&M experiment as both the observer and experiment are in the same frame of reference. — PhilosophyRunner
The reason why I brought up this problem was due to it resembling the M&M experiment.
— Gampa Dee
It very much does. Just like with a light clock, without length contraction, the M&M experiment would show it taking more time for light to make the circuit with and against the motion, and less time when it moves perpendicular to the motion. The difference should have been noticed and the Newtonian models were falsified when it wasn't. — noAxioms
Einstein claimed the light’s velocity is invariant without any specific reason why
It's a postulate, not something that can be known. Special relativity used a fairly strong version of the postulate, that light actually goes the same speed regardless of inertial frame choice. Some later papers took much of that metaphysical assertion away and used a weaker statement, that the laws of physics (including any measurement of light speed) are the same relative to any inertial frame.
The latter wording allows for the existence of a preferred frame despite no local way to detect it. — noAxioms
So in the case of the M&M experiment, Einstein would claim that there was no length contractions nor time dilations involved because there was no different inertial frames to measure....
I assure you that the M&M experiment was performed in many different inertial frames. The statement above is false and Einstein would certainly not have said anything to that effect. — noAxioms
But, what if the light speed was c relative to the source (sort of particle theory)
Immediately falsifiable by having two light sources moving at different speeds emit a flash when they pass each other. A distant observer would see one flash from the approaching source sooner than the one from the receding source, thus falsifying Einstein's postulate. Such a result is not observed. Light speed is empirically demonstrated to be independent of the speed of the light source. — noAxioms
The observer outside of the frame
An observer cannot be outside any frame. He's in all of them, just not stationary in them all. — noAxioms
On the other hand, the monoclastic neutrinal differentiation of the autosomatically-determined spin value inherent in all such equitational bivalent transmogrifications cannot be entirely ignored, wouldn't you agree? — alan1000
Particularly if we keep in mind the various M&M chromatic values which may be obtained at little expense in our own time. — alan1000
noAxioms — noAxioms
.Galileo’s law ( all bodies fall at the same rate).
— Gampa Dee
That's not the law, and you wording is trivially falsified. I can drop a rock off a building and simultaneously throw another one downward. The thrown one will fall at a greater rate and arrive first. — noAxioms
However, this part does seem to show that there are some “unknown” elements as well.
Well yea. The alternative is some klnd of solipsism where things are gravitationally attracted only to known object, which makes the knower very special. — noAxioms
if a car comes towards you as you are driving your car, the measured velocity relative to both of you is v..
.,
That's impossible. If a car is moving relative to me at v, then I am moving relative to it at it at -v by definition. — noAxioms
Total v? You want to add velocity of me relative to the road to the velocity of them relative to me? — noAxioms
if a car accelerates towards you as you are accelerating towards it, the total acceleration will “not” be a + a ??
Correct. Nothing is accelerating at a+a (which is zero) nor a-a which is twice something. Doing would violate Newton's laws, F=ma in particular.
Each car is accelerating at 1a, presumably in opposite directions. — noAxioms
Take once again a pair of equal mass planets X&Y orbiting each other with X at coordinate -1, 0 and Y at 1,0..The both trace a unit circle about the origin at 0,0. X has a coordinate acceleration of 1,0 and Y has a coordinate acceleration of -1,0. Nothing is accelerating at 2 anything. The distance between them isn't changing over time, so adding the acceleration magnitudes does not in any way express the rate of change of their separation. — noAxioms
We may be mixing up speed & velocity. Speed is a scalar but velocity is a vector. — EricH
In your example, both cars are traveling at a speed of 0.5v relative to the road (again no direction). In order to calculate the relative velocity we need to do vector calculations (which can get complicated). In the most general situation the two objects may be moving in arbitrary directions and may or may not ever collide. In your simplified one dimensional example, the velocity of one car is .5v and the velocity of the other car is -5v. But these are vectors, so to calculate the relative velocity between the two you cannot simply add the .5v & -5v and get 0.[/quote]
I agree, this is indeed what I was saying; I did claim the total velocity as being v.
However,I was actually talking of accelerations, and the velocity example was only to make a point. PhilosophyRunner wrote saying that I will need to read up on inertial and non-inertial frames because this is the part that confuses me ...and this is what I'll be doing.
— EricH
You have to factor in the direction and do vector math. The end result will be a relative speed of v - and the vector math will show a collision between the two cars at some point in time depending on the values of v and the starting distance between the two cars. — EricH
↪Gampa Dee I suggest you read up on inertial and non-inertial frames of reference. I think your misunderstanding stems from not knowing the difference between them and treating both as if there is no difference. — PhilosophyRunner
Ok; I’ll try to remember to use “a” instead :) ...but I did see some charts which identify planets using g in the same way they use distance in terms of earth distance units (AU).
— Gampa Dee
Those charts would be correct. Gravity (a) on Saturn is ~1.08g and it orbits at about 9.5 AU. Both g and AU are constants. Saturn does not define a different AU any more than it defines a different g.
https://nssdc.gsfc.nasa.gov/planetary/factsheet/planet_table_ratio.html — noAxioms
Well, for me personally, I ask myself whether there is a meaning behind r^2 besides simply being a distance squared. It would seem logical, for me, to view gravity as being, for example, some sort of energy emanating from the massive body (probably at light`s speed), which would continuously be reducing it`s energy density as it travelled away from the mass source,
That's one way of looking at it. A light shining at intensity proportional to the mass would decrease in brightness at the square of the distance from the light. But gravity doesn't travel, so you can take the analogy only so far. — noAxioms
For example, the moon's orbital distance increases by several cm a year as Earth transfers its angular momentum to it. It also transfers about 3% of its angular energy to it, and radiates the remainder away as heat. So energy is lost in the process of the moon's orbital changes. — noAxioms
If the falling body was taken from the ground, that reduces M, and it will thus accelerate less than a similar object falling from space — noAxioms
For a small rock, the difference is immeasurable since the mass of Earth changes more per second than any nitpicking about where you got the rock. — noAxioms
The moon is like that. It is a big rock that was essentially taken from the ground, not having arrived from space. When they brought back the moon rocks, they were quite surprised to find it was a chunk of Earth and not something else like every other moon out there. But it accelerates at Σ GM/r² where Σ is the summation of the accelerations due to every bit of mass out there, mostly the due to the sun and also Earth (what's left of it after the moon was scooped out), but everything else pulls at it as well. — noAxioms
But the equation would still remain a = GM/r^2 + Gm / r^2
This cannot be right. For two equal stationary masses, it says they will not accelerate towards each other since the sum is zero. This is not the case. — noAxioms
Even if you fixed that, the equation there does not express an acceleration, so the 'a=' part in front is blatantly wrong. Nothing accelerates at that rate. — noAxioms
g is a constant. Saturn doesn't have a different g, it has a different acceleration a. — noAxioms
The acceleration is dependent on mass and radius and has little direct connection with density, especially since density of any planet/star varies considerably at different depths. You complicating things needlessly by trying to work with area and/or density. — noAxioms
I do have a hard time with this...is it possible to share this proof?
Nothing in science is actually a proof, but the reasoning goes like this: You have two identical balls of mass M each. They presumably fall at the same rate. Now you connect them by a thin thread or spot of glue, creating one object of mass 2M. Either the connection makes some sort of magical difference, or the 2M mass should fall at the same rate as before. Hence the rate is independent of mass. — noAxioms
One can reason that the connection cannot apply a downward force to both objects (violating Newton's laws), but Newton's laws were not available at that time yet. F=ma was unknown, and the theory of impetus and such was still a thing. — noAxioms
I think we can deal with the Newtonian equation using only one dimention.
— Gampa Dee
Any talk of orbital mechanics has velocity that is not parallel with the acceleration, and thus involves at least two dimensions. Orbits can be described in a plane. Only things falling straight up and down can be described in one dimension. — noAxioms
I don’t believe that Newton had a three dimensional frame of reference in mind
All frames of reference have 3 dimensions of space, and require 3 velocity components to describe. — noAxioms
However , to claim that g is not acceleration I still don’t get
g is acceleration, but is simply a constant scalar. So the gravitational pull on the surface of Saturn is 1.08g. It would be wrong to say Saturn has a slightly larger g. — noAxioms
A frame of reference is a starting point, not something thrown in. Without it, any velocity is completely undefined. — noAxioms
Orbital accelerations are always changing, even in the circular case. Remember that it is a vector. — noAxioms
There's nothing special about M since it works with any M. Galileo actually published a tidy proof that the acceleration is independent of the mass of the thing accelerating. — noAxioms
To use your car example, I am standing on the pavement not accelerating. I see one car (A) moving accelerating at 3m/s2 towards my left and another car (B) accelerating at 5m/s2 towards my right. That is simply the acceleration of the cars. It is meaningless (from a classical mechanics sense) to then add these up and say car A is accelerating at 8m/s2 from the point of view of the car B. Neither car is accelerating at 8m/s2. Car A is accelerating at 3m/s2 and car B at 5m/s2. — --`r
I suppose you can use [the two added equations] to compute the rate of change in distance between the two objects, only in a 1-dimensional case, but that rate isn't acceleration.
— noAxioms
It's not that it's simpler. Adding the equations only produces a useful result if there is no motion except along one axis. So for instance, under Newtonian mechanics, the ISS is continuously accelerating (coordinate acceleration) towards Earth at about 8.7 m/s² and yet its distance from Earth is roughly fixed, and its speed relative to Earth is also roughly fixed. This is because it is not a 1d case. The ISS has motion in a direction other than just the axis between it and Earth.
The ISS example also serves as a wonderful example of the difference between the physics definition of acceleration (rate of change in velocity=8.7 m/s² down) vs street definition (zero change in speed). — noAxioms
Thank you PhilosophyRunner
For example see: https://orbital-mechanics.space/the-n-body-problem/two-body-inertial-motion.html
— PhilosophyRunner — Gampa Dee
The symbol for that is 'a', not 'g'. 'a' is a vector variable acceleration. g is a scalar constant acceleration. Neither are a force. Force is measured in Newtons and uses the symbol F. Try to use standard symbols when discussing such things, as personal preferences only lead to confusion. — noAxioms
:(
— noAxioms
The acceleration of the moon when it is at radius r is exactly that in Newtonian physics. That does not mean it will hit the ground in 3 1/3 seconds like the 10 kg ball. As I said, a small fraction of a second is more likely. — noAxioms
I'm assuming that the dense super-mass is rigid, so yes, the acceleration applies to every point in the moon-ball. I am not assuming Earth is sufficiently rigid to not deform under the ungodly tidal stress the ball would apply to it. The sidewalk slab 60 meters below will be yanked up without waiting for Earth to catch up with it. — noAxioms
:)
— noAxioms
Acceleration is absolute, not relative, so adding them seems to result in a fairly meaningless value — noAxioms
I suppose you can use it to compute the rate of change in distance between the two objects, only in a 1-dimensional case, but that rate isn't acceleration. For instance, if an apple detaches from a tree and the distance between me and it decreases at 9.8 m/sec², that in no way suggests that I am accelerating at that rate, and in fact I'm accelerating (coordinate acceleration, not proper acceleration) away from it a little bit. — noAxioms
The Newtonian gravitational equation, identifying two masses, has only one acceleration , the one caused by the earth.
But there is an equation for each object, each dependent on only that mass, and not on the mass of the thing accelerating towards it. — noAxioms
ok; I think we might be going somewhere. When we measure the acceleration of the rock towards the earth, aren't we not measuring, at the same time, the acceleration of the earth towards the rock? How could you know the difference?
— Gampa Dee
As P-R points out, the coordinate acceleration described by Newton's equations is relative to any inertial coordinate system, and the equations don't work when used with a non-inertial coordinate system such as an accelerating or rotating one (Earth is both).
Mind you, plenty of books treat things like the Earth-moon system in isolation, which is to reference an accelerating coordinate system. It works to an extent, but adds confusion. For instance, few are aware that the moon always accelerates towards the sun since the sun exerts more force on it that does Earth. That means that when the moon is between the two (solar eclipse), the moon is accelerating directly away from Earth.
From the accelerating frame of Earth, the moon seems to maintain a fairly constant distance that isn't much a function of which direction the sun is. Yes the orbit of the moon (like any orbit) is eccentric to a degree, but that again isn't due to the sun. — noAxioms
Secondly why would we include the acceleration of the earth caused by the second mass? That is not what we were calculating - we were calculating the acceleration of the rock. If you wanted to calculate the acceleration of the Earth caused by the rock, that is a separate calculation
an hour ago — PhilosophyRunner
If you want to model a system where both bodies are accelerating you will have to use the two-body equations of motion, — PhilosophyRunner
I have no idea what you might consider the 'gravitational energy' of Earth. Mass divided by 4 π r² gives you, well, I don't know what. It seems vaguely related to area of a circle. — noAxioms
So the acceleration of the rock in earth's gravitational field is not dependent on the mass of the rock. It is dependent on the distance of the rock from the center of mass of the earth, and on the mass of the earth.
You seem to be asking, what if M were different? — PhilosophyRunner
First of all, gravity isn't energy. I have no idea what you might consider the 'gravitational energy' of Earth. Mass divided by 4 π r² gives you, well, I don't know what. It seems vaguely related to area of a circle. You equate this to 'k g', but no idea what 'k' is (kilo?). 'g' is the constant 9.8 m/sec², so you're seemingly equating this function of mass and radius to the constant 9800 m/sec² — noAxioms
Here, if r is small then g can become extremely large.
You seem to be equating g with A. 'g' is a constant magnitude of acceleration (a scalar), so it cannot be smaller or larger. A is a variable, and a vector, not a scalar. A = GM/r², so yes, 'A' becomes quite large if r is small enough. Saying 'g' can be quite large is like saying a meter can be larger if my table is wide enough. — noAxioms
Any other mass g acceleration would need to be added at every point in space...
'mass g' doesn't parse. I don't know what you mean by this. Are you now adding random objects here and there? Then you need to separately compute the acceleration of each and add those accelerations. Newton showed (via shell theorem) that any spherical distribution of mass of radius r can be treated as a point mass by objects outside of r. — noAxioms
Sorry, but I kind of came in late to this discussion and I don't know what you're trying to do beyond what is described by these very simple equations. For small objects, they all fall at the same rate, and the only reason the feather falls slower is due to air friction. They brought a feather to the moon to show it falling at the same rate as a rock. PR stunt..,. tax dollars at work. — noAxioms
In reality, it would take not 3.3 seconds to hit the ground, but probably just a fraction of a second in the dense moon case. You're not going to compute that by just adding the accelerations, which treat both objects as point masses or rigid spheres, which they are not. — noAxioms
But now if you increase the density of that ball to say the mass of the moon, it will hit the ground in less time, not because its initial coordinate acceleration is any greater, but because it has enough mass to significantly cause the ground to come up and meet it — noAxioms
Initial acceleration of an object due to gravity of a primary is mass independent. I mean, F=ma, which if substituted directly into F=GMm/r² gets you A=GM/r², something independent of m altogether. — noAxioms
Ok. And they have the same acceleration because they have different inertias. How does this not answer that? — Pantagruel
But also yes, the overall force realized does vary if the mass of the smaller object varies — Pantagruel
ndeed it is, but the same condition applies with respect to the relationship between force and inertia. The force is a composite product of the two masses, as is the acceleration. — Pantagruel
Different masses accelerate at the same rate towards a reference mass because they also have different inertias, which balances the different forces generated..... — Pantagruel
The reason for this is that the mass of a falling object is negligible in relation to the mass of the Earth. — unenlightened
the mass of the Earth cannot probably still be measured to the ton, and if it could, some of the mass would been the air above and exert a negative force. — unenlightened
That wouldn't work since this has the dimensions of squared meters per seconds and we want something that has the dimensions of seconds.
To arrive at the simplification, note that gamma can be rewritten as 1c2c2−v2c2√=1(c2−v2)c2√1c2c2−v2c2=1(c2−v2)c2 and therefore γ2γ2 is c2c2−v2c2c2−v2
Our expression 2Lcγ(c2−v2)2Lcγ(c2−v2) can therefore be rewritten as 2L⋅γ2c⋅γ2L⋅γ2c⋅γ, which is 2Lγc2Lγc. As gamma is dimensionless, this expression indeed has the dimensions of seconds. — Pierre-Normand
Your thinking was correct, but since both the forward and the return path are travelled by the light pulse at the same speed c (in any referential frame), and since the return path is shorter, the time to travel it is also shorter. This is why you must setup two distinct equations:
d1 = L/gamma + vt_1 = ct_1
d2 = L/gamma - vt_2 = ct_2 — Pierre-Normand
Think of two people walking an unleashed dog at a steady pace v thereby keeping a constant distance L between them. Picture the dog running back and forth between them at constant speed v_2 > v. The forward path for the dog is longer than L since the person ahead keeps moving the 'goalpost' further away until the dog reaches them. Conversely, the person behind moves the 'goalpost' closer during the time when the dog returns. — Pierre-Normand
ok: Would vt_2 be equal to -vt?
— Gampa Dee
No, since vt is the distance travelled by the mirror during the forward path while vt_2 is the distance travelled by the source during the return path, and the return path takes a shorter time. t_2 < t. — Pierre-Normand
From the first equation, t = L/(gamma(c - v))
From the second equation, t_2 = L/(gamma(c + v))
Therefore, the total time
T = t+t_2 = L/(gamma(c - v)) + L/(gamma(c + v))
To simplify this, we can multiply the first term by (c+v)/(c+v) and the second term by (c-v)/(c-v), effectively multiplying each term by 1.
T = L(c + v)/(gamma(c - v)(c + v)) + L(c - v)/(gamma(c - v)(c + v))
= L((c + v) + (c - v))/gamma(c2 - v2) = 2Lc/gamma(c2 - v2)
Next, we can express gamma explicitly as 1/sqrt(1 - v^2/c^2), and divide both the numerator and denominator by c^2 to get
T = (2L/c)sqrt(1 - v^2/c^2)/(1 - v^2/c^2) = 2Lgamma/c
As long as all velocity terms are expressed relative to the same inertial frame of reference, the relative velocities between two material objects (or between a material object and a photon) can be expressed as simple sums or differences (e.g., c + v or c - v). This doesn't involve any Newtonian assumptions. When the light pulse travels at c and the clock at v, their relative velocity is c + v (or c - v). This is because it's the rate at which their separation changes, as measured in the stationary reference frame. — Pierre-Normand
ps: Your name tells me that you might be a french speaking person? I am as well...my name is Andre
Yes, from the Montreal area, in Quebec, Canada. Nice meeting you, André. — Pierre-Normand
In the case of the horizontal clock you indeed have d1 = L/gamma + vt for the first path and d2 = L/gamma - vt_2 for the return path. I use "t_2" since the time for traveling the return path is different (shorter). Since in both cases the distance is travelled at c, we have the two equations:
d1 = L/gamma + vt = ct
d2 = L/gamma + vt_2 = ct_2 — Pierre-Normand
T = L/((gamma(c - v)) + L/(gamma(c + v)) with is the same result I had obtained more directly by considering the relative velocities of the light pulse and clock. — Pierre-Normand
In the case of the horizontal clock you indeed have d1 = L/gamma + vt for the first path and d2 = L/gamma - vt_2 for the return path. I use "t_2" since the time for traveling the return path is different (shorter). Since in both cases the distance is travelled at c, we have the two equations:
d1 = L/gamma + vt = ct
d2 = L/gamma + vt_2 = ct_2 — Pierre-Normand
Yes, you're right that the Lorentz contraction of the path must also be taken into account. The Lorentz factor, gamma, is always greater than 1, so the contracted length is L/gamma. — Pierre-Normand
The time required for the light ray to reach the receding mirror is therefore t1 = d/v1 — Pierre-Normand
Similarly, the time required for the light ray to return to the source is therefore t2 = d/v2 where v2 = c + v. — Pierre-Normand
The total time elapsed is therefore t1 + t2 = L/(gamma(c - v)) + L/(gamma(c+v)). To simplify, you can multiply the numerator and denominator of the first term by c + v and the numerator and denominator of the second term by c - v. — Pierre-Normand
You get
t = L(c + v)/(gamma(c^2-v^2))+L(c - v)/(gamma(c^2-v^2)) = 2Lc/(gamma(c^2-v^2))
Since gamma = 1/sqrt(1-v^2/c^2), 2Lc/(gamma(c^2-v^2)) simplifies to 2L*gamma/c which is the same time registered by the vertical light clock. — Pierre-Normand
(Note that c/(gamma(c^2-v^2) = c*sqrt(1 - v^2/c^2)/c^2-v^2 = sqrt(c^2 - v^2)/(c^2-v^2) = 1/sqrt(c^2-v^2) = 1/(c*sqrt(1-v^2/c^2) = gamma/c.)
Intuitively, as v tends towards c and taking into account the Lorentz contraction of the clock, the duration of the return travel tends towards zero. Meanwhile, the duration of the forward travel tends towards infinity despite the shortened distance, as c - v approaches zero faster than sqrt(1-v^2/c^2) does. — Pierre-Normand