- #1
member 728827
- TL;DR Summary
- As it seems that I have some issues applying correctly the metric in the case of the Bob twin, which is the non-inertial guy in the twin paradox story, I write down here what I do and what conclusions I get, so hope I can find the mistake(s).
From Wikipedia article about Hyperbolic motion, I have the following coordinate equations of motion for Bob in his accelerated frame:
##t(T)=\frac{c}{g} \cdot \ln{(\sqrt{1+(\frac{g \cdot T}{c})^2}+\frac{g \cdot T}{c})} \quad (1)##
##x(T)=\frac{c^2}{g} \cdot (\sqrt{1+(\frac{g \cdot T}{c})^2}-1) \quad (2)##
where I use lowercase (t,x) to denote the Bob's NIRF coordinates, and uppercase (T,X) to denote Alice's IRF coordinates. Obviously, for Bob, that stays at rest at the origin of its accelerated frame, t is his proper time ##\tau##.
The metric for Bob's accelerated frame is given by:
##ds^2=-(1+\frac{g \cdot x}{c^2})^2 \cdot d(ct)^2+(dx)^2 \quad (3)##
Then, the question is: can Bob use his metric "ruler" to measure or deduce the Alice's proper time? So, Bob in his accelerated laboratory, wants to deduce which is the proper time of Alice using his metric, or at least, check that all equations meet. Let's say, Bob takes about 2.5 years to travel from Earth to somewhere, and he wants to check how many years have elapsep for his twin sister Alice in Earth, as he needs to prepare in advance the birthday's gifts Alice will surely want to receive.
As I was quoted in another thread, it seems that Bob has to solve for ##d\tau## in the following equation:
##c^2 d\tau^2 = c^2 \, \left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, dt^2 - dx^2 \quad (4)##
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt \quad (5)##
where ##t_2## is the proper time for Bob to go from Earth to somewhere planet X.
But, here is the thing. If Bob uses his metric to measure the worldline path of Alice, I think that Bob will obtain... the Bob's proper time that Alice takes to follow that path, not the Alice's proper time! But seems that I'm wrong? If so, I don't understand why ?
So, lets check that, and do the numbers using equation (5) as starting point.
First thing to be cautious. The velocity in equation (5) is the coordinate velocity in Bob's accelerated frame. I attach one of the graphics I used in my thread, from where you can see that the coordinate velocity of Alice is... more that the speed of light. So, go figure.
In that post I wrote:
Let's calculate first the coordinate velocity. Using the parametrized equations (1) and (2), the coordinate velocity will be the quotient of the derivatives of those equations with respect the parameter T, which is the proper time for Alice. And so:
##\frac{d x}{dT}=\frac{g \cdot T}{\sqrt{\left(\frac{g \cdot T}{c}\right)^2}+1} \quad (6)##
##\frac{d t}{dT}=\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)} \quad (7)##
and finally:
##v=g \cdot T \quad (7b)##
As said previously, the coordinate speed seems not limited by the c-limit in an accelerated frame.
From the Wikipedia article, we know that the relation between Alice's and Bob's time is given by:
##T(t)=\frac{c}{g} \cdot \sinh{\left(\frac{g \cdot t}{c}\right)} \quad (8)##
Plugging (2), (7b) and (8) into (5), we finally obtain:
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt=t_2##
Big surprise, isn't it?
But as Saint Thomas the Apostle, lets plug the finger using another approach.
Now, I will do a change of variable in the (5) integral, and instead of ##dt##, I'll use ##dT## instead, and the boundaries of the integration will go from 0 to T_2, being T_2 the proper time Alice's measures for the voyage. Aha, this surely will now work, because something was wrong in the before proceeding.
We previously have obtained the derivative ##\frac{d t}{dT}## in equation (7):
##\frac{d t}{dT}=\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)} \quad (7)##
and so:
##\tau = \int_{0}^{T_2}\sqrt{\left( 1+ \frac{g \cdot x(T)}{c^2} \right)^2 \, - \frac{v(T)^2}{c^2}} \cdot dT \quad (9)##
If you calculate ##\sqrt{\left( 1+ \frac{g \cdot x(T)}{c^2} \right)^2 \, - \frac{v(T)^2}{c^2}}##, this gives 1. That's it, 1. So, equation (9) gets "simplified" to:
##\tau = \int_{0}^{T_2}\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)}\cdot dT \quad (10)##
And the result of the integral is:
##\frac{c}{g} \cdot \sinh^{-1}{\left( \frac{g \cdot T}{c} \right)} \quad (11)##
which for equation (8) is... ##t_2## again. So, no way, it's consistent.
Bob now quits, and breaks the metric "ruler". But, overnight, he decides to think again what's the issue here. He must be doing something wrong using his metric to obtain the Alice's proper time. But, what is it?
Time to go to his old notes when he was studying to become an astronaunt. Let's see, acceleration in Special Relativity, seems weird because SR only deals with constant velocities. Umm. But, how's it's done, what the Physicists did long ago to treat acceleration in SR?
So, how's its made? Then, Bob remembers and argues the following: As the Lorentz Transform goes from one IRF to another IRF, then is a piece of cake, we pull out from our magician relativistic top-hat an MCRF "rabbit", and then we consider that at every instant in time, there's a Momentarily Comoving Reference Frame which is, obviously, Inertial. That MCRF is at rest (coincidence?, God playing dice?...) in that instant with respect that "ugly" accelerated frame in which I rest, so I can Lorentz transform to that frame instead. Isn't that great?
But he also needs to believe in the "Clock hypothesis", so to say that what's really important for SR is the velocity, no how you get to that velocity... in SR, doesn't matter, is not its business. You get to that velocity, and that's it. Ok, let's take that for granted, because it seems plausible, and he thinks that's been experimentally probed up to high g values.
Then for the IRF and thanks to Mr. Lorentz, we can deduce that ##A=\gamma^3\alpha##, and from there to the infinite and beyond. Ok, this is what my hand-written notes read anyway.
So, what I'm (Bob) measuring? What I want to measure? Take it easy, and let's read the fine print of all this stuff. How's it was made? I'm now in deep space, in an accelerated spaceship, but how all this formulas and equations where initially made?
Wait a minute, where is that MCRF that suddenly pops up for Alice, and she says is at rest in my frame? Because is that MCFR what underpins all the acceleration framework in SR! If Alice says there's such MCRF, then that same MCRF is in my frame also, and is... AT REST obviously, but in a x-coordinate that lies in Earth. I have to consider it as it is, has no velocity for me, is at rest in my accelerated frame.
Now, the light-bulb shines upon Bob's head, and he says: Eureka, that's it! The proper time of Alice traveling along her worldline has to be calculated with my "ruler" as the "tiny" time dilations from each of the infinite succession of MCRF's that magically pop up along the path. And then, I know how to apply my "ruler" metric, I must consider that the coordinate velocity of Alice is cero, because I consider the velocity of the MCRF's, and all are AT REST for me. Is not the "ruler" what is wrong, but I was measuring something different with it.
Let's try.
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt \quad (5)##
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2} \cdot dt \quad (12)##
Plugging equation (2) which gives the path of Alice in her wordline, and (8) into (12):
##\tau= \int_{0}^{t_2} \sqrt{\sinh^2{\left(\frac{g \cdot t}{c}\right)}+1} \cdot dt=\frac{c}{g} \cdot \sinh{\left(\frac{g \cdot t_2}{c}\right)}=T_2##
We got it!
But, Bob gets and tachyon-pulsed telegram from the Planet Federation, which says what he argues is not correct, and the Klingon empire has issued a warning!
So, what's wrong? Where's the issue?
Any help would be appreciated.
Thank all.
##t(T)=\frac{c}{g} \cdot \ln{(\sqrt{1+(\frac{g \cdot T}{c})^2}+\frac{g \cdot T}{c})} \quad (1)##
##x(T)=\frac{c^2}{g} \cdot (\sqrt{1+(\frac{g \cdot T}{c})^2}-1) \quad (2)##
where I use lowercase (t,x) to denote the Bob's NIRF coordinates, and uppercase (T,X) to denote Alice's IRF coordinates. Obviously, for Bob, that stays at rest at the origin of its accelerated frame, t is his proper time ##\tau##.
The metric for Bob's accelerated frame is given by:
##ds^2=-(1+\frac{g \cdot x}{c^2})^2 \cdot d(ct)^2+(dx)^2 \quad (3)##
Then, the question is: can Bob use his metric "ruler" to measure or deduce the Alice's proper time? So, Bob in his accelerated laboratory, wants to deduce which is the proper time of Alice using his metric, or at least, check that all equations meet. Let's say, Bob takes about 2.5 years to travel from Earth to somewhere, and he wants to check how many years have elapsep for his twin sister Alice in Earth, as he needs to prepare in advance the birthday's gifts Alice will surely want to receive.
As I was quoted in another thread, it seems that Bob has to solve for ##d\tau## in the following equation:
##c^2 d\tau^2 = c^2 \, \left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, dt^2 - dx^2 \quad (4)##
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt \quad (5)##
where ##t_2## is the proper time for Bob to go from Earth to somewhere planet X.
But, here is the thing. If Bob uses his metric to measure the worldline path of Alice, I think that Bob will obtain... the Bob's proper time that Alice takes to follow that path, not the Alice's proper time! But seems that I'm wrong? If so, I don't understand why ?
So, lets check that, and do the numbers using equation (5) as starting point.
First thing to be cautious. The velocity in equation (5) is the coordinate velocity in Bob's accelerated frame. I attach one of the graphics I used in my thread, from where you can see that the coordinate velocity of Alice is... more that the speed of light. So, go figure.
In that post I wrote:
Unfortunately, that was unanswered and unconfirmed, although it seemed to me and interesting question . Anyway, the v in equation (5) is the coordinate velocity, and is not equal to the velocity Alice observes from Earth.I attach both Alice and Bob's worldlines. For the Alice worldline, remark that the coordinate speed of Alice is faster than the coordinate speed of c, but I think that the "real" speed of light line should be drawn as ##c \cdot (1+\frac{g \cdot x}{c^2})##, as for Bob in the origin of a non-inertial frame, the "speed of light" will be dependent on the position in which "the photon" is located relative to Bob. Someone could confirm this point?
Let's calculate first the coordinate velocity. Using the parametrized equations (1) and (2), the coordinate velocity will be the quotient of the derivatives of those equations with respect the parameter T, which is the proper time for Alice. And so:
##\frac{d x}{dT}=\frac{g \cdot T}{\sqrt{\left(\frac{g \cdot T}{c}\right)^2}+1} \quad (6)##
##\frac{d t}{dT}=\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)} \quad (7)##
and finally:
##v=g \cdot T \quad (7b)##
As said previously, the coordinate speed seems not limited by the c-limit in an accelerated frame.
From the Wikipedia article, we know that the relation between Alice's and Bob's time is given by:
##T(t)=\frac{c}{g} \cdot \sinh{\left(\frac{g \cdot t}{c}\right)} \quad (8)##
Plugging (2), (7b) and (8) into (5), we finally obtain:
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt=t_2##
Big surprise, isn't it?
But as Saint Thomas the Apostle, lets plug the finger using another approach.
Now, I will do a change of variable in the (5) integral, and instead of ##dt##, I'll use ##dT## instead, and the boundaries of the integration will go from 0 to T_2, being T_2 the proper time Alice's measures for the voyage. Aha, this surely will now work, because something was wrong in the before proceeding.
We previously have obtained the derivative ##\frac{d t}{dT}## in equation (7):
##\frac{d t}{dT}=\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)} \quad (7)##
and so:
##\tau = \int_{0}^{T_2}\sqrt{\left( 1+ \frac{g \cdot x(T)}{c^2} \right)^2 \, - \frac{v(T)^2}{c^2}} \cdot dT \quad (9)##
If you calculate ##\sqrt{\left( 1+ \frac{g \cdot x(T)}{c^2} \right)^2 \, - \frac{v(T)^2}{c^2}}##, this gives 1. That's it, 1. So, equation (9) gets "simplified" to:
##\tau = \int_{0}^{T_2}\frac{c \cdot \left(\frac{g^2 \cdot T}{c^2 \cdot \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1}}+\frac{g}{c}\right)}{g \cdot \left( \sqrt{\left(\frac{g \cdot T}{c}\right)^2+1} +\left(\frac{g \cdot T}{c}\right)\right)}\cdot dT \quad (10)##
And the result of the integral is:
##\frac{c}{g} \cdot \sinh^{-1}{\left( \frac{g \cdot T}{c} \right)} \quad (11)##
which for equation (8) is... ##t_2## again. So, no way, it's consistent.
Bob now quits, and breaks the metric "ruler". But, overnight, he decides to think again what's the issue here. He must be doing something wrong using his metric to obtain the Alice's proper time. But, what is it?
Time to go to his old notes when he was studying to become an astronaunt. Let's see, acceleration in Special Relativity, seems weird because SR only deals with constant velocities. Umm. But, how's it's done, what the Physicists did long ago to treat acceleration in SR?
So, how's its made? Then, Bob remembers and argues the following: As the Lorentz Transform goes from one IRF to another IRF, then is a piece of cake, we pull out from our magician relativistic top-hat an MCRF "rabbit", and then we consider that at every instant in time, there's a Momentarily Comoving Reference Frame which is, obviously, Inertial. That MCRF is at rest (coincidence?, God playing dice?...) in that instant with respect that "ugly" accelerated frame in which I rest, so I can Lorentz transform to that frame instead. Isn't that great?
But he also needs to believe in the "Clock hypothesis", so to say that what's really important for SR is the velocity, no how you get to that velocity... in SR, doesn't matter, is not its business. You get to that velocity, and that's it. Ok, let's take that for granted, because it seems plausible, and he thinks that's been experimentally probed up to high g values.
Then for the IRF and thanks to Mr. Lorentz, we can deduce that ##A=\gamma^3\alpha##, and from there to the infinite and beyond. Ok, this is what my hand-written notes read anyway.
So, what I'm (Bob) measuring? What I want to measure? Take it easy, and let's read the fine print of all this stuff. How's it was made? I'm now in deep space, in an accelerated spaceship, but how all this formulas and equations where initially made?
Wait a minute, where is that MCRF that suddenly pops up for Alice, and she says is at rest in my frame? Because is that MCFR what underpins all the acceleration framework in SR! If Alice says there's such MCRF, then that same MCRF is in my frame also, and is... AT REST obviously, but in a x-coordinate that lies in Earth. I have to consider it as it is, has no velocity for me, is at rest in my accelerated frame.
Now, the light-bulb shines upon Bob's head, and he says: Eureka, that's it! The proper time of Alice traveling along her worldline has to be calculated with my "ruler" as the "tiny" time dilations from each of the infinite succession of MCRF's that magically pop up along the path. And then, I know how to apply my "ruler" metric, I must consider that the coordinate velocity of Alice is cero, because I consider the velocity of the MCRF's, and all are AT REST for me. Is not the "ruler" what is wrong, but I was measuring something different with it.
Let's try.
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2 \, - \frac{v^2}{c^2}} \cdot dt \quad (5)##
##\tau = \int_{0}^{t_2}\sqrt{\left( 1+ \frac{g \cdot x}{c^2} \right)^2} \cdot dt \quad (12)##
Plugging equation (2) which gives the path of Alice in her wordline, and (8) into (12):
##\tau= \int_{0}^{t_2} \sqrt{\sinh^2{\left(\frac{g \cdot t}{c}\right)}+1} \cdot dt=\frac{c}{g} \cdot \sinh{\left(\frac{g \cdot t_2}{c}\right)}=T_2##
We got it!
But, Bob gets and tachyon-pulsed telegram from the Planet Federation, which says what he argues is not correct, and the Klingon empire has issued a warning!
So, what's wrong? Where's the issue?
Any help would be appreciated.
Thank all.
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