How Does Newton's Second Law Adapt to Relativistic Speeds?

In summary, in Newtonian physics, a force on a object is equal to its mass times acceleration. But in relativity, when the acceleration approaches the speed of light, Newton's Second Law starts to become less accurate because to accelerate a mass more you must keep adding more energy. So in relativistic terms, what equation is there that holds up to speeds near the speed of light? In special relativity, the equation that always holds is F = m0A. This expression holds only when the proper mass is constant in time.
  • #1
hover
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In Newtonian Physics, a force on a object is equal to its mass times acceleration. This is Newton's Second Law. But in relativity, when the acceleration approaches the speed of light, Newton's Second Law starts to become less accurate because to accelerate a mass more you must keep adding more energy. So in relativistic terms, what equation is there that holds up to speeds near the speed of light?

Thanks:biggrin:
 
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  • #2
4-vectors

Hi, Hover,

hover said:
In Newtonian Physics, a force on a object is equal to its mass times acceleration. This is Newton's Second Law. But in relativity, when the acceleration approaches the speed of light, Newton's Second Law starts to become less accurate because to accelerate a mass more you must keep adding more energy. So in relativistic terms, what equation is there that holds up to speeds near the speed of light?
In special relativity it is also F = m0A. And this forumla always works! :smile:

But the difference is that A is a 4-vector. A is the 4-acceleration vector which is basically the derivative of the 4-velocity vector with respect to proper time. And the 4-velocity vector is basically the change in direction in spacetime with respect to proper time. But note that we have four, not three, directions in spacetime!
In addition there is the 4-energy-momentum vector which is mass times the 4-velocity vector.

Four vectors are simple and elegant. :smile:

As you can see it is pretty straightforward, we simply have to add the extra direction in relativity. :smile:
 
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  • #3
hover said:
In Newtonian Physics, a force on a object is equal to its mass times acceleration. This is Newton's Second Law. But in relativity, when the acceleration approaches the speed of light, Newton's Second Law starts to become less accurate because to accelerate a mass more you must keep adding more energy. So in relativistic terms, what equation is there that holds up to speeds near the speed of light?

Thanks:biggrin:

Warning: F = ma does NOT work in general.

F = dP/dt

is the relativistic equation that always holds. The exact form the equations take in terms of "mass" depend on whether or not one uses relativistic mass or invariant mass.

Note that all of the quantities above depend on the observer, including the force.

You will find that the ratio F/a depends on the direction of the force, assuming all measurements are done in the lab frame. This is sometimes discussed under the names "longitudinal mass" and "transverse mass" in older physics books.

I thought there was a FAQ in the sci.physics.faq that had these formulas for F/a, but I couldn't find it offhand. Perhaps someone else will have better luck.

The equations for relativistic momentum in the lab frame are

Px = gamma m vx
Py = gamma m vy
Pz = gamma m vz

where m is the invariant mass, sometimes called the rest mass, of the particle.

and gamma = 1/sqrt{1 - vx^2 - vy^2 - vz^2}

Differentiating the above expression for relativistic momentum will give the correct force / acceleration relationships assuming the forces and the accelerations are measured in the laboratory frame.

Sometimes, accelerations are measured in the frame of the object being accelerated, such as in the relativistic rocket. These are often called proper accelerations. If you are interested in the velocity of a travel accelerated at a constant 'felt' acceleration, you'll want to look at the FAQ on the relativistic rocket at http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
 
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  • #4
[tex]\frac{d\vec p}{dt}=m\frac{d}{dt}\left[\frac{\vec v}
{\sqrt{1-{\vec v}^2}}\right]
= m[\gamma{\bf a}+\gamma^3{\vec v}({\vec v}\cdot{\vec a})]
=m\gamma^3[{\vec a}+{{\vec v}\times({\vecv}\times{\vec a})][/tex]
 
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  • #5
Meir Achuz said:
[tex]\frac{d\bf p}{dt}=m\frac{d}{dt}\left[\frac{\bf v}
{\sqrt{1-{\bf v}^2}}\right]
= m[\gamma{\bf a}+\gamma^3{\bf v(v\cdot a)}]
=m\gamma^3[{\bf a}+{\bf vX(vX a)}][/tex]

This is awfully hard to read. I'd suggest using \vec{} and \times, i.e.

so v X a, for instance, becomes
[tex]
\vec{v} \times \vec{a}
[/tex]

and for good measure, v should probably be |v| to make it clear you're taking the norm

and I suppose some warning about geometric units is called for (though you could always put in those annoying factors of c)
 
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  • #6
MeJennifer said:
In special relativity it is also F = m0A. And this forumla always works! :smile:
That expression holds only when the proper mass is constant in time.

Pete
 
  • #7
pmb_phy said:
That expression holds only when the proper mass is constant in time.
Very true.
 
  • #8
MeJennifer said:
Hi, Hover,


In special relativity it is also F = m0A. And this forumla always works!

But the difference is that A is a 4-vector. A is the 4-acceleration vector which is basically the derivative of the 4-velocity vector with respect to proper time. And the 4-velocity vector is basically the change in direction in spacetime with respect to proper time. But note that we have four, not three, directions in spacetime!
In addition there is the 4-energy-momentum vector which is mass times the 4-velocity vector.

Four vectors are simple and elegant. :smile:

As you can see it is pretty straightforward, we simply have to add the extra direction in relativity.
The F in that equation is the "Minkowski force" and is not dp/dt.
The Minkowski force is defined as
[tex]{\cal F}^\mu=\gamma(dE/dt,dp/dt)[/tex].
Using that would eventually lead to the equation I gave for dp/dt,
but not as easily.
 
  • #9
I have searched for the relativistic acceleration formula involving Force and Mass for a while now. All I can remember is something like this:

a=f/(m(1-v^2/c^2)^(3/2))

I know this is wrong. So can someone tell me the correct equation
 
  • #10
prasannapakkiam said:
I have searched for the relativistic acceleration formula involving Force and Mass for a while now. All I can remember is something like this:

a=f/(m(1-v^2/c^2)^(3/2))

I know this is wrong. So can someone tell me the correct equation
Did you read posting #2?
 
  • #11
Meir Achuz said:
The F in that equation is the "Minkowski force" and is not dp/dt.
The Minkowski force is defined as
[tex]{\cal F}^\mu=\gamma(dE/dt,dp/dt)[/tex].
Using that would eventually lead to the equation I gave for dp/dt,
but not as easily.
Ok, so it is not dp/dt.

Is there perhaps anything wrong with using 4-vectors in relativity?
 
  • #12
So:
a=F/(M*SQRT(1-v^2/c^2))
 
  • #13
4-Vectors

Prasanna, see for a good overview of 4-vectors in relativity http://www.courses.fas.harvard.edu/~phys16/Textbook/ch12.pdf".

Morin, in his introduction writes:

"Although it is possible to derive everything in special relativity without the use of 4-vectors (and indeed, this is the route, give or take, that we took in the previous two chapters), they are extremely helpful in making calculations and concepts much simpler and more transparent."

I cannot help but fully agreeing with Morin.
 
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  • #14
MeJennifer said:
Ok, so it is not dp/dt.

Is there perhaps anything wrong with using 4-vectors in relativity?

No.

[itex]d \tau =dt/\gamma[/itex] gives

[tex]\gamma \frac{d}{dt} = \frac{d}{d \tau}.[/tex]

Thus,

[tex]{\cal F} = \frac{dP}{d\tau},[/tex]

where [itex]P[/itex] is 4-momentum.
 
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  • #15
MeJennifer said:
Ok, so it is not dp/dt.
Is there perhaps anything wrong with using 4-vectors in relativity?
Meir Achuz must have meant that the 3-vector dp/dt is not equal to the 4-vector F = m0A which is quite obvious and you seem to know that anyway (especially with your acceptance of the addendum that I mentioned to you). In that sense Meir Achuz's comment is very confusing to me. George hit it right on the button!

Pete
 
  • #16
pmb_phy said:
Meir Achuz must have meant that the 3-vector dp/dt is not equal to the 4-vector F = m0A which is quite obvious and you seem to know that anyway (especially with your acceptance of the addendum that I mentioned to you). In that sense Meir Achuz's comment is very confusing to me. George hit it right on the button!

Pete
The confusion comes from the fact that a number of things can be called "force" in SR. The Minkowski forces in George's post and mine (They are the same.) are convenient mathematical 4-vectors under a LT, but
[tex]d{\vec p}/dt[/tex] is the force as given by the Lorentz force. [tex]m{\vec a}[/tex] could even be defined as "force" in SR if it was made clear that it just means [tex]m{\vec a}[/tex]. It is clearest if the word "force" is dispensed with in SR.
 
  • #17
Thre are two kind of "forces" in SR:
(1) One is "3-force" which is the rate of change of "3-momentum" with respect to "time"
[tex]{\vec F}=\frac{d {\vec p}}{dt}=\frac{d{\vec u}}{dt}=m{\vec a}+m_0\frac{d\gamma}{dt}{\vec u}[/tex]
where [tex]{\vec u}[/tex] is the 3-velocity [tex]{\vec u}=\frac{d {\vec r}}{dt}[/tex] and [tex]{\vec a}[/tex] is the 3-acceleration [tex]{\vec a}=\frac{d{\vec u}}{dt}[/tex], [tex]m=m_0\gamma[/tex]
(2) Another one is "4-force" which is the rate of change of "4-momentum" with respect to "proper time" [tex]\tau = is/t[/tex]
[tex]{\tilde F}=\frac{d {\tilde p}}{d\tau}=\frac{dt}{d\tau}\frac{d {\tilde p}}{dt}
=\gamma \frac{d}{dt}({\vec p},imc)[/tex]
where [tex]{\tilde p}=({\vec p},imc)[/tex] is the "4-momentum, [tex]s=\sqrt{x^2+y^2+z^2-c^2t^2}[/tex] is the "4-distance" and [tex]\gamma=\frac{1}{\sqrt{1-(u/c)^2}}[/tex], [tex]{\vec u}=(\frac{dx}{dt},\frac{dy}{dt},\frac{dz}{dt})=(u_1,u_2,u_3)[/tex], [tex]u=\sqrt{{u_1}^2+{u_2}^2+{u_3}^2}[/tex] .
 
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  • #18
The name "force" should be defined as "rate of change of momentum" with respect to some kind of "time". We can write [tex]{\vec F}=m_0{\vec A}=
m_0 (\gamma {\vec a}+\frac{d\gamma}{dt}{\vec u})[/tex] and "define" [tex]{\vec A}=\gamma {\vec a}+\frac{d\gamma}{dt}\frac{{d\vec r}}{dt}[/tex] as some kind of "acceleration" if you like. However this "new acceleration" would not be "time rate of change of some kind of velocity" as you can see. The same happens to the 4-force [tex]{\tilde F}[/tex]
 
  • #19
bchui said:
Thre are two kind of "forces" in SR:
(1) One is "3-force" which is the rate of change of "3-momentum" with respect to "time"
[tex]{\vec F}=\frac{d {\vec p}}{dt}=\frac{d{\vec u}}{dt}=m{\vec a}+m_0\frac{d\gamma}{dt}{\vec u}[/tex]
where [tex]{\vec u}[/tex] is the 3-velocity [tex]{\vec u}=\frac{d {\vec r}}{dt}[/tex] and [tex]{\vec a}[/tex] is the 3-acceleration [tex]{\vec a}=\frac{d{\vec u}}{dt}[/tex], [tex]m=m_0\gamma[/tex]
bchui - There appears to be an error here. You write F = dp/dt = du/dt = ... The first equality is correct while the second equality is wrong for obvious reasons.

Best wishes
Pete
 
  • #20
I am really not sure where all these arguments against the use of 4-vectors is coming from. :confused:

bchui said:
However this "new acceleration" would not be "time rate of change of some kind of velocity" as you can see. The same happens to the 4-force
4-acceleration is simply the derivative of the 4-velocity vector with respect to [itex]\tau[/itex]. I fail to see why that is not a""time rate of change of some kind of velocity" as you call it.
 

FAQ: How Does Newton's Second Law Adapt to Relativistic Speeds?

What is the equation for F=ma in relativistic terms?

The equation for F=ma in relativistic terms is F = γm0a, where γ is the Lorentz factor, m0 is the rest mass of the object, and a is the acceleration.

How does the equation for F=ma change in special relativity?

In special relativity, the equation F=ma is modified to take into account the effects of time dilation and length contraction. This results in the equation F = γm0a, where γ is the Lorentz factor and m0 is the rest mass of the object.

What does the Lorentz factor represent in the equation for F=ma in relativistic terms?

The Lorentz factor, represented by the symbol γ, takes into account the effects of time dilation and length contraction on the mass and acceleration of an object moving at relativistic speeds.

How does the equation for F=ma in relativistic terms relate to Einstein's theory of relativity?

The equation F = γm0a is a fundamental equation in special relativity, which is a part of Einstein's theory of relativity. It describes how the force acting on an object is affected by its mass and acceleration at high speeds.

Can the equation F=ma in relativistic terms be applied to all objects?

The equation F = γm0a can be applied to all objects, regardless of their size or speed. However, it is most applicable to objects moving at speeds close to the speed of light, where the effects of special relativity become significant.

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