Understanding Proper Acceleration: Definition, Equations, and Applications

In summary, proper acceleration is the rate of change of 4-velocity with respect to proper time, and it is an invariant quantity independent of the observer's frame of reference. It can be calculated using the general approach of differentiating the components of 4-velocity and is given by the formula a = (γ4 a, γ4 va/c). The magnitude of proper acceleration is also invariant, as the norm of any vector is invariant in Minkowski space. This means that the coordinate acceleration measured by all observers will be the same, despite differences in the observer's frame of reference.
  • #1
vin300
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I'm all messed up here trying to learn about proper acceleration. As I understand it, an observer with constant acceleration undergoes parabolic motion but one with constant proper acceleration undergoes hyperbolic motion as seen from an inertial frame.Wikipedia says that proper acceleration is the rate of change of proper velocity with respect to coordinate time, but this doesn't agree with the definition of prop acc given in post 14 in this thread, where it depends on the rate of change of rapidity.In Don Koks' book, according to equation 7.6, the proper acc is γ^3 times the acceleration measured in an inertial frame(x dot equals v).Also, I would like to know how to derive the rindler metric
 
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  • #2
vin300 said:
As I understand it, an observer with constant acceleration undergoes parabolic motion but one with constant proper acceleration undergoes hyperbolic motion as seen from an inertial frame.

The hyperbolic part is right. I think the parabolic part is right (assuming that by constant acceleration there you mean constant coordinate acceleration, i.e., the second derivative of coordinate position, x, with respect to coordinate time, t), although it's not the way I would normally think about this scenario.

vin300 said:
Wikipedia says that proper acceleration is the rate of change of proper velocity with respect to coordinate time,

The Wikipedia page's presentation seems somewhat strange to me, assuming you meant this Wikipedia page:

http://en.wikipedia.org/wiki/Proper_acceleration

It's not the normal way of defining proper acceleration that I'm used to, but without taking more time to look at it I can't say for sure whether it is actually inconsistent with this...

vin300 said:
the definition of prop acc given in post 14 in this thread, where it depends on the rate of change of rapidity.

...which is the (correct) definition that I'm used to seeing.

vin300 said:
In Don Koks' book, according to equation 7.6, the proper acc is γ^3 times the acceleration measured in an inertial frame(x dot equals v).

This looks OK to me, although Google Books isn't letting me look at the actual book page you linked to, so I can't see the context.

vin300 said:
Also, I would like to know how to derive the rindler metric

Try the Wikipedia page here (this one looks OK to me):

http://en.wikipedia.org/wiki/Rindler_coordinates

Or Greg Egan's page here:

http://gregegan.customer.netspace.net.au/SCIENCE/Rindler/RindlerHorizon.html
 
  • #3
vin300, Uniform acceleration is a good example to practice on, but how much you learn from it depends on how you solve it! If you use the rapidity approach you've solved one problem. Better is to use a general approach, and thereby learn how to solve most problems in relativistic kinematics.

The motion of a relativistic particle can be described in either of two ways: in terms of three-dimensional quantities t, x, v and a, or in terms of four-dimensional ones: τ, x, v and a. Of course dt/dτ ≡ γ = (1 - v2/c2)-1/2.

The 4-velocity v = dx/dτ is a timelike 4-vector with space and time components v = (γv, γc). Note that v has dimensions of velocity and is constant length: v·v = c2.

The 4-acceleration a = dv/dτ is a spacelike 4-vector orthogonal to it: v·a = 0. To calculate the components of a you just have to differentiate the components of v. (It helps to do a little algebra on the side first and note that dγ/dt = γ3(v·a)/c2.)

a = dv/dτ = γ dv/dt = (γ2a + γ dγ/dt v, cγ dγ/dt)
= (γ2a + γ4(v·a)/c2, γ4(v·a)/c)

Yes indeed, this is messy! But it's completely general. You can apply this formula to things like circular motion, etc. But to make matters simpler from now on, let's assume the motion is linear. It then reduces to something rather nice:

a = (γ4 a, γ4 va/c)

What is the magnitude of a?

a·a = - γ6 a2, so |a| = γ3 a

That's the result that you found mentioned in Don Koks' book: the γ3 factor between the 4-acceleration and the 3-acceleration.

We still have not assumed the acceleration is uniform. If you do that:

γ3 a = const ≡ A

you get a differential equation

dv/dt = A (1 - v2/c2)3/2

which you can easily integrate to get a hyperbola.
 
  • #4
vin300 said:
I'm all messed up here trying to learn about proper acceleration. As I understand it, an observer with constant acceleration undergoes parabolic motion but one with constant proper acceleration undergoes hyperbolic motion as seen from an inertial frame.Wikipedia says that proper acceleration is the rate of change of proper velocity with respect to coordinate time, but this doesn't agree with the definition of prop acc given in post 14 in this thread, where it depends on the rate of change of rapidity.In Don Koks' book, according to equation 7.6, the proper acc is γ^3 times the acceleration measured in an inertial frame(x dot equals v).Also, I would like to know how to derive the rindler metric

I think the Wikipedia article is wrong. Proper acceleration is the derivative of 4-velocity with respect to proper time, not with respect to coordinate time.
 
  • #5
OK, thank all of you.
BTW, there's a small error here:
Bill_K said:
= (γ2a + γ4(v·a)/c2, γ4(v·a)/c)
 
  • #6
Thanks, should be: (γ2a + γ4v(v·a)/c2, γ4(v·a)/c)
 
  • #7
How to prove using the general approach, that the magnitude of proper acceleration is invariant? The coordinate acceleration measured by all observers is the same, and γ is observer dependent, so the magnitude of four acceleration will be different for different observers.
 
  • #8
vin300 said:
How to prove using the general approach, that the magnitude of proper acceleration is invariant? The coordinate acceleration measured by all observers is the same, and γ is observer dependent, so the magnitude of four acceleration will be different for different observers.

The norm of any vector is invariant (note: norm is defined using the metric, which is Minkowski in SR, not Euclidean). 4-velocity is a vector, proper acceleration (derivative of it by an invariant τ) is thus also vector.
 
  • #9
PAllen said:
The norm of any vector is invariant (note: norm is defined using the metric, which is Minkowski in SR, not Euclidean). 4-velocity is a vector, proper acceleration (derivative of it by an invariant τ) is thus also vector.

And how about the general (not minkowskian) case?
 
  • #10
vin300 said:
How to prove using the general approach, that the magnitude of proper acceleration is invariant? The coordinate acceleration measured by all observers is the same, and γ is observer dependent, so the magnitude of four acceleration will be different for different observers.

The coordinate acceleration is not the same for all observers. If the coordinate acceleration is g in the initial rest frame of a rocket, then it will be g/γ3 in a frame in which the rocket is initially traveling at velocity v.
 
  • #11
TrickyDicky said:
And how about the general (not minkowskian) case?

I'm pointing at the less frequently mentioned situation in GR involving non-inertial observers, certainly in this case one cannot affirm so lightly that 4-acceleration magnitude is an invariant quantity, at most one must say that it is undefined. The fact is that as it happens with energy 4-acceleration magnitude in GR is not a conserved quantity (except in static spacetimes), it is also frame-dependent. My question is then how does the 4-vector concept in SR evolve to the GR context? can it still be considered a 4-vector if its magnitude is not a scalar invariant?
 
  • #12
TrickyDicky said:
And how about the general (not minkowskian) case?

The argument is completely general. I mentioned Minkowski metric only to make sure the questioner understood how the norm is defined (contraction of a vector twice with the metric).
 
  • #13
PAllen said:
The argument is completely general. I mentioned Minkowski metric only to make sure the questioner understood how the norm is defined (contraction of a vector twice with the metric).

I qualified my question in my next post, I guess you missed it.
 
  • #14
TrickyDicky said:
I'm pointing at the less frequently mentioned situation in GR involving non-inertial observers, certainly in this case one cannot affirm so lightly that 4-acceleration magnitude is an invariant quantity, at most one must say that it is undefined. The fact is that as it happens with energy 4-acceleration magnitude in GR is not a conserved quantity (except in static spacetimes), it is also frame-dependent. My question is then how does the 4-vector concept in SR evolve to the GR context? can it still be considered a 4-vector if its magnitude is not a scalar invariant?

Proper acceleration is defined by the same definition in GR as SR and is a well used concept. There is no requirement of static spacetime. It is a geometric invariant by construction. Part of the physical interpretation of GR is that the mathematically defined proper acceleration norm (invariant) is what is measured by an accelerometer. This physical prediction is either true or false for our universe, but there is no ambiguity in the definition or interpretation of proper acceleration in GR.

[Edit: To make explicit, again, the argument: 4-velocity is a vector in GR as well as SR; derivative by tau along a timelike world line is also a vector in GR as well as SR. Norm of a vector is defined as a contraction of the metric with the vector (twice). That contractions to scalars are invariant in diff.geometry is an elementary consequence of definitions. Thus, proper acceleration, so defined, is invariant with no caveats in arbitrary GR spacetimes.]
 
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  • #15
You mean a non-inertial observer will measure the same four-acceleration magnitude than an inertial one?
 
  • #16
TrickyDicky said:
You mean a non-inertial observer will measure the same four-acceleration magnitude than an inertial one?

For any 4-vector Aμ, the quantity gμη Aμ Aη is an invariant---it has the same value to all observers, regardless of whether they are inertial or not.
 
  • #17
TrickyDicky said:
You mean a non-inertial observer will measure the same four-acceleration magnitude than an inertial one?

What? 4-acceleration (with norm of proper acceleration) is a feature of a world line (of some object). The object may be supposed to have an accelerometer. Who observes the measurement being taken is irrelevant. They won't see the instrument read different values. The fact the norm of 4-acceleration is an invariant mathematically captures the irrelevance.
 
  • #18
Nevermind. I had some sort of silly confusion writing about 4-quantities when I was thinking in terms of 3-quantitities.
 

FAQ: Understanding Proper Acceleration: Definition, Equations, and Applications

What is proper acceleration?

Proper acceleration is defined as the rate of change of proper velocity, which is the velocity measured by an observer at rest with respect to the object. It is also known as the acceleration experienced by an object in its own frame of reference.

How is proper acceleration different from coordinate acceleration?

Coordinate acceleration is the acceleration measured by an observer in a different frame of reference than the object, while proper acceleration is the acceleration measured by an observer in the same frame of reference as the object. This means that proper acceleration takes into account the effects of time dilation and length contraction, while coordinate acceleration does not.

What are the equations for proper acceleration?

The equation for proper acceleration can be derived from the Lorentz transformations and is a function of both the object's velocity and the observer's velocity. One common equation for proper acceleration is a = γ^3 * a', where γ is the Lorentz factor and a' is the coordinate acceleration.

What are some real-life applications of understanding proper acceleration?

Proper acceleration is an important concept in the field of relativistic physics, where objects are moving at high speeds close to the speed of light. It is used in the design of spacecraft and satellites, and is also relevant in understanding the motion of particles in particle accelerators. Proper acceleration also plays a role in understanding the behavior of black holes and other celestial bodies.

How does proper acceleration relate to Newton's laws of motion?

While Newton's laws of motion are valid in non-relativistic situations, they do not hold true for objects moving at high speeds. Proper acceleration takes into account the effects of relativity, such as time dilation and length contraction, which are not accounted for in Newton's laws. Proper acceleration is a more accurate measure of an object's motion in these situations.

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