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| Tags: field, projectile, relativistic |
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#1
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Send me to the FAQY if you must, but ...
What is the correct generalization of Newtonian gravity for massive relativistic projectiles? Assume a region of (flat) uniform gravitational field g, and consider a relativistic projectile, rest mass m0, altitude z. Is it still true that d^2z/dt^2 = g? |
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#2
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Moiraine wrote in message . ..
On 26 Jul 2003 09:06:59 -0700, (Edward Green) wrote: Send me to the FAQY if you must, but ... What is the correct generalization of Newtonian gravity for massive relativistic projectiles? Assume a region of (flat) uniform gravitational field g, and consider a relativistic projectile, rest mass m0, altitude z. Is it still true that d^2z/dt^2 = g? The latest gravity experiment that is close to yielding an objective answer is Gravity Probe B. The experiment is being performed at close to zero gravity and near the lambda point of helium to avoid contamination of data. Should yield the most accurate compelling evidence so far. http://einstein.stanford.edu/gen_int...b/gpbsty1.html Thank you for the reference. Of course experiment trumps all ... but surely plain old GTR must make some unambiguous predictions here? |
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#4
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"Edward Green" wrote in message
om... Send me to the FAQY if you must, but ... What is the correct generalization of Newtonian gravity for massive relativistic projectiles? Assume a region of (flat) uniform gravitational field g, and consider a relativistic projectile, rest mass m0, altitude z. Is it still true that d^2z/dt^2 = g? "Kinetic Energy and the Equivalence Priciple", S. Carlip, http://arxiv.org/abs/gr-qc/9909014 |
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#5
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"Old Man" wrote in message news:3f23a31a_4@newsfeed...
Edward Green wrote in message om... .... surely plain old GTR must make some unambiguous predictions here? Ed has it right. Use the equivalence principle. Just replace the uniform gravitational field with a rocket ship accelerating at g. [Old Man] Sigh. I was afraid you might say something like that. You want me to "think"? Ok ... girding my loins to the sticking place: Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. OTOH, we know that clocks on the projectile moving past at relativistic velocity appear to run slower by gamma; in other words, the projectile falls past a fixed set of z-indicia in the rocket attached frame in less proper time. Since delta z = (1/2)gt^2, we conclude g will appear to grow by a factor of gamma^2 on the projectile. Any contention with any of this? I've been thinking of that damn silly "relativistic submarine" paradox. A reference was provided discussing the gravitational effect of relativistic mass: however, on this level, that doesn't seem relevant. We have reached the conclusion that relativistically varying masses fall exactly the same way otherwise varying masses do -- there is no variation in the kinematics. *Is this true? Or must we still include some correction moving back and forth between rocket and rest clocks? |
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#6
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"Old Man" wrote in message news:3f249770_4@newsfeed...
Edward Green wrote in message om... Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. This sounds correct. The OTOH part, below, is too complicated for Old Man . It's a mater of mind and time over matter. [Old Man] No damn fair! You have pushed me into the thorny and painful byways of "thought", and now you must join me in the bracken field! (I had to retype that three damn times because of software glitches, and each time the joke grew more ornate -- so it's no my, dare I say, damn, fault ;-). Anyway, the snipped part below was relatively straight forward ... just involving the time dilation in the inertial projectile's frame, and the effect it would have on the apparent acceleration in that frame past the ... err ... frames of the rocket. The "*" statement worries me more, since I'm not sure if some baby-bathwater escapage did not occur there -- needs more thought about clocks in accelerated frames. I did make a baby/bathwater kind of error in your orbital angular momentum thread, BTW -- though I claim I left suitable hedges :-) Viz., I blithly claimed a course change is a course change, and costs us locally the same whatever we think of the global energetic orbital implications. I still stand by this ... but the expert John Prussing points out that your solution lies precisely in using awareness of the global properties of the orbits to pick the optimal points to spend your course change currency. I am happy you have the energy to spend on sci.physics. I saw some mock kung-fu knife fighting at a street fair Sunday, and while the dancing and athletics were impressive, the effect was lessened by the steely knives flapping in the wind! Your knife remains tempered, however, and just the right foil. (I'm trying my hand at a bit of sycophancy, and you must excuse any clumsiness in the unfamiliar form :-). |
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#7
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Edward Green wrote in message om... "Old Man" wrote in message news:3f249770_4@newsfeed... Edward Green wrote in message om... Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. This sounds correct. The OTOH part, below, is too complicated for Old Man . It's a mater of mind and time over matter. [Old Man] No damn fair! You have pushed me into the thorny and painful byways of "thought", and now you must join me in the bracken field! OK, I'll make an attempt. It's not that relativity problems aren't interesting, but I usually screw-up. The subject is motion in directions transverse to the relativistic velocity vector of a massive body. A familiar example is that of a charged particle accelerating in a uniform electric field, wherein the particle has initial momentum in a direction transverse to the electric field. As in Ed's problem, we will assume that the initial transverse velocity is relativistic. For a stationary observer, the transverse momentum is conserved, but the transverse velocity approaches zero as the velocity parallel to the field approaches that of light. Here is a calculation: Consider the following problem: An observer is standing at rest at the origin of a Cartesian coordinate system. A uniform electric field, E, exists with direction parallel to the y - axis. A test particle with rest mass, M, and charge, Q, has an initial momentum, Pxo, with direction parallel to the x - axis. The initial conditions a Uniform electric field ( Ex, Ey, Ez ) = ( 0, E, 0 ) for all space and for all times. Test charge momentum ( Px, Py, Pz ) = ( Pxo, 0, 0 ) at tine T=0. M is the rest mass of the charge. The solution is obtained by setting dPy / dT = QE (2) Px = Pxo = MVx / sqrt( 1- (V/C)^2 ) (3a) Py = MVy / sqrt( 1- (V/C)^2 ) (3b) Pz = 0 (4) where V is the test particle speed and ( Vx, Vy, Vz ) are its vector components. Solving these equations yields Vy / C = QET / sqrt( (QET)^2 + (MC)^2 + Pxo^2 ) (5) Vx / C = Pxo / sqrt( (QET)^2 + (MC)^2 + Pxo^2 ) (6) Vz / C = 0 (7) From equation (5), it is apparent that as time, T, increases without bound, Vy approaches C. This is expected since the only force upon the particle is in the y-direction. From equation (6), it is apparent that as time, T, increases without bound, Vx approaches zero. This is not expected since there is no force applied in the x - direction. Now, what if we replace the electric field with a gravitational field? That is, set QE = Mg ? Is the solution the same? For an observer traveling on the charge, there is a definite difference: In an electric field, the observer will feel the acceleration of the charge in the direction of the field, and this will have an effect on his time piece, but, in a gravitational field, the observer is in free fall and feels no forces. This will have a different effect on his time piece. The situation for the stationary observer is similarly complicated. [Old Man] |
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#8
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In article , (Edward Green) writes:
"Old Man" wrote in message news:3f249770_4@newsfeed... Edward Green wrote in message om... Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. This sounds correct. The OTOH part, below, is too complicated for Old Man . It's a mater of mind and time over matter. [Old Man] No damn fair! You have pushed me into the thorny and painful byways of "thought", and now you must join me in the bracken field! (I had to retype that three damn times because of software glitches, and each time the joke grew more ornate -- so it's no my, dare I say, damn, fault ;-). Anyway, the snipped part below was relatively straight forward ... just involving the time dilation in the inertial projectile's frame, and the effect it would have on the apparent acceleration in that frame past the ... err ... frames of the rocket. The "*" statement worries me more, since I'm not sure if some baby-bathwater escapage did not occur there -- needs more thought about clocks in accelerated frames. I did make a baby/bathwater kind of error in your orbital angular momentum thread, BTW -- though I claim I left suitable hedges :-) Viz., I blithly claimed a course change is a course change, and costs us locally the same whatever we think of the global energetic orbital implications. Well, you did some good thinking there, so let me add the few missing bits. First, yes, it is a good idea to consider things locally, it simplifies matters enormously. Especially, it is a good idea (with rockets) to think in terms of "short burn", one occuring fast enough so that for all practical purposes the craft remains in the same location on orbit during the burn. This enables you to ignore gravity alltogether when analyzing the results. As for "change" and "cost", you've to be a bit careful. Yes, a momentum change is a momentum change and once you found it relative to one reference frame, you got it. Also, the energy expended for this change is the same relative to all reference frames. *However*, the split of said energy into the part that's thrown away with the exhaust and the part which stays with the craft, this *is* reference frame dependent. And as for change in angular momentum, this is most certainly reference frame dependent. I still stand by this ... but the expert John Prussing points out that your solution lies precisely in using awareness of the global properties of the orbits to pick the optimal points to spend your course change currency. John knows his stuff. To put what he wrote in the most simplified form possible, the rules of thumb a 1) For a given delta_v (meaning given amount of fuel used) you get the maximal change in energy by performing the burn at peri...whatever (and you should thrust along the direction of motion) 2) For a given delta_v you get the maximal change in angular momentum by performing the burn at ap...whatever. Mati Meron | "When you argue with a fool, | chances are he is doing just the same" |
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#9
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In writes:
In article , (Edward Green) writes: "Old Man" wrote in message news:3f249770_4@newsfeed... Edward Green wrote in message om... Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. This sounds correct. The OTOH part, below, is too complicated for Old Man . It's a mater of mind and time over matter. [Old Man] No damn fair! You have pushed me into the thorny and painful byways of "thought", and now you must join me in the bracken field! (I had to retype that three damn times because of software glitches, and each time the joke grew more ornate -- so it's no my, dare I say, damn, fault ;-). Anyway, the snipped part below was relatively straight forward ... just involving the time dilation in the inertial projectile's frame, and the effect it would have on the apparent acceleration in that frame past the ... err ... frames of the rocket. The "*" statement worries me more, since I'm not sure if some baby-bathwater escapage did not occur there -- needs more thought about clocks in accelerated frames. I did make a baby/bathwater kind of error in your orbital angular momentum thread, BTW -- though I claim I left suitable hedges :-) Viz., I blithly claimed a course change is a course change, and costs us locally the same whatever we think of the global energetic orbital implications. Well, you did some good thinking there, so let me add the few missing bits. First, yes, it is a good idea to consider things locally, it simplifies matters enormously. Especially, it is a good idea (with rockets) to think in terms of "short burn", one occuring fast enough so that for all practical purposes the craft remains in the same location on orbit during the burn. This enables you to ignore gravity alltogether when analyzing the results. As for "change" and "cost", you've to be a bit careful. Yes, a momentum change is a momentum change and once you found it relative to one reference frame, you got it. Also, the energy expended for this change is the same relative to all reference frames. *However*, the split of said energy into the part that's thrown away with the exhaust and the part which stays with the craft, this *is* reference frame dependent. And as for change in angular momentum, this is most certainly reference frame dependent. I still stand by this ... but the expert John Prussing points out that your solution lies precisely in using awareness of the global properties of the orbits to pick the optimal points to spend your course change currency. John knows his stuff. To put what he wrote in the most simplified form possible, the rules of thumb a 1) For a given delta_v (meaning given amount of fuel used) you get the maximal change in energy by performing the burn at peri...whatever (and you should thrust along the direction of motion) 2) For a given delta_v you get the maximal change in angular momentum by performing the burn at ap...whatever. And you could add (and you should thrust normal to the radius.) You make it sound so simple! But, as you know, situations don't always fit the ideal case. Murphy's Law seems to prevail, as usual. Re peri...whatever, the generic term usually used is periapse, where apse means point. In specific cases perigee, perihelion, perijove (Jupiter) are used. And you have a choice between perilune or periselenium for the moon, depending on whether you prefer the Latin or Greek word for moon. Mati Meron | "When you argue with a fool, | chances are he is doing just the same" -- John E. Prussing University of Illinois at Urbana-Champaign Department of Aerospace Engineering http://www.uiuc.edu/~prussing |
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#10
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In article , (John E. Prussing) writes:
In writes: In article , (Edward Green) writes: "Old Man" wrote in message news:3f249770_4@newsfeed... Edward Green wrote in message om... Consider the instantaneous rest frame of a rocket accelerating at 1g in the z direction, and consider two particles at altitude z0 at t0; one is stationary in the instantaneous rest frame of the rocket, the other has no z component of velocity but a relativistic x component perpendicular to z. Well ... it is perfectly damn evident that, since in this case the rocket is "really" doing the moving, that the two particles will "fall" towards the floor of the rocket at exactly the same rate. The orthogonal velocity of the second is irrelevant, it's holding at constant z in our initial inertial frame -- and since we chose the instantaneous rest frame, there are to first order no relativistic corrections between rocket frame and rest frame.* OK. That's pretty damn unambiguous. Since we may extend this argument to arbitrary particle trajectories, we predict from the EP that all objects accelerate at the same rate in a uniform G field, relativistic velocities be damned. This sounds correct. The OTOH part, below, is too complicated for Old Man . It's a mater of mind and time over matter. [Old Man] No damn fair! You have pushed me into the thorny and painful byways of "thought", and now you must join me in the bracken field! (I had to retype that three damn times because of software glitches, and each time the joke grew more ornate -- so it's no my, dare I say, damn, fault ;-). Anyway, the snipped part below was relatively straight forward ... just involving the time dilation in the inertial projectile's frame, and the effect it would have on the apparent acceleration in that frame past the ... err ... frames of the rocket. The "*" statement worries me more, since I'm not sure if some baby-bathwater escapage did not occur there -- needs more thought about clocks in accelerated frames. I did make a baby/bathwater kind of error in your orbital angular momentum thread, BTW -- though I claim I left suitable hedges :-) Viz., I blithly claimed a course change is a course change, and costs us locally the same whatever we think of the global energetic orbital implications. Well, you did some good thinking there, so let me add the few missing bits. First, yes, it is a good idea to consider things locally, it simplifies matters enormously. Especially, it is a good idea (with rockets) to think in terms of "short burn", one occuring fast enough so that for all practical purposes the craft remains in the same location on orbit during the burn. This enables you to ignore gravity alltogether when analyzing the results. As for "change" and "cost", you've to be a bit careful. Yes, a momentum change is a momentum change and once you found it relative to one reference frame, you got it. Also, the energy expended for this change is the same relative to all reference frames. *However*, the split of said energy into the part that's thrown away with the exhaust and the part which stays with the craft, this *is* reference frame dependent. And as for change in angular momentum, this is most certainly reference frame dependent. I still stand by this ... but the expert John Prussing points out that your solution lies precisely in using awareness of the global properties of the orbits to pick the optimal points to spend your course change currency. John knows his stuff. To put what he wrote in the most simplified form possible, the rules of thumb a 1) For a given delta_v (meaning given amount of fuel used) you get the maximal change in energy by performing the burn at peri...whatever (and you should thrust along the direction of motion) 2) For a given delta_v you get the maximal change in angular momentum by performing the burn at ap...whatever. And you could add (and you should thrust normal to the radius.) Yes, certainly. You make it sound so simple! But, as you know, situations don't always fit the ideal case. Murphy's Law seems to prevail, as usual. That's for sure, being an experimentalist I'm painfully aware of this fact. Murphy's Law is the one you can always count on:-) Re peri...whatever, the generic term usually used is periapse, where apse means point. Oh, thanks, that's the word I was missing. In specific cases perigee, perihelion, perijove (Jupiter) are used. And you have a choice between perilune or periselenium for the moon, depending on whether you prefer the Latin or Greek word for moon. I like the sound of periselenium, but chemists may find it confusing. Mati Meron | "When you argue with a fool, | chances are he is doing just the same" |
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