Derivation of the Equation for Relativistic Mass

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SUMMARY

The equation for relativistic mass, expressed as m = m0 / √(1 - v2 / c2), derives from Lorentz transformations and the principles of special relativity. Key insights include the relationship between energy and mass, as articulated in E=mc2, and the conservation of momentum in relativistic collisions. Various derivations, including those by R.C. Tolman, utilize thought experiments involving collisions to illustrate how relativistic mass emerges from classical mechanics under relativistic conditions.

PREREQUISITES
  • Understanding of Lorentz transformations
  • Familiarity with the concept of four-momentum
  • Knowledge of energy-mass equivalence (E=mc2)
  • Basic principles of special relativity
NEXT STEPS
  • Study the derivation of relativistic momentum using collision thought experiments
  • Explore R.C. Tolman's works on relativistic mass and momentum
  • Learn about the implications of time dilation and length contraction in special relativity
  • Investigate the role of four-velocity in relativistic physics
USEFUL FOR

Students and educators in physics, particularly those studying special relativity, as well as researchers interested in the foundational concepts of relativistic dynamics.

  • #61
Let me add:

I only wanted to say that there exists a "access to" SR where the formula m=... simply is a abreviation. I admit, for understanding some textbooks this might not be a helpfull remark... I can only commend Noltings textbooks - I don't know if they have been translated to english.
 
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  • #62
rjb, I liked your thought experiment. And Sunset, a valid reply. It made me realize that y in your setup is similar to ds in mine (above). As far as special relativity is concerned, directions transverse to the motion (y, z) are just as invariant as the proper interval s. But in my example, the tranverse momentum (along s) is invariant because it is proportional to the rest energy. Relativity is also designed to make that true.
 
  • #63
Sunset said:
The relativistic momentum p_r = \frac{m_0 v}{\sqrt{1-\frac{v^2}{c^2}}} is defined in that way, because you want to have momentum-conservation.
Let me explain:
When you step from classical mechanics (Newtons axioms) to relativistic mechanics you need a new axiom-system.

but

p = \frac{m_0 v}{\sqrt{1-\frac{v^2}{c^2}}}

is not either of the axioms. it is a result.

the axioms are:

1. Observation of physical phenomena by more than one inertial observer must result in agreement between the observers as to the nature of reality. Or, the nature of the universe must not change for an observer if their inertial state changes. Or, every physical theory should look the same mathematically to every inertial observer. Or, the laws of the universe are the same regardless of inertial frame of reference.

2. (invariance of c) Light is always propagated in empty space with a definite velocity c that is independent of the state of motion of the emitting body, and all observers observe the speed of light in vacuo to be the same value, c.

and the original poster was asking how to get to

m = \frac{m_0}{\sqrt{1-\frac{v^2}{c^2}}}

from those axioms. i skipped over deriving time-dilation (since he/she didn't ask about that and i assume knew about it) but from these first principles and time-dilation (which also comes from the same two first principles). it's a derived result, not an axiom.
 
  • #64
NanakiXIII said:
Simple to you, perhaps. Either I am to use techniques I'm not familiar with, or I'm just not seeing it. The variable v is in there three times, I've been trying but I can't seem to get it to one side the the equal sign.

By "degree 2 in v", you mean I should square the equation? I looked into that but still see no obvious solution.

You get:

u_x_R*v^2/c^2-2v+u_x_R=0

with the obvious solution : v=c^2/u_x_R(1-\sqrt(1-u_x_R^2/c^2)
 
  • #65
NanakiXIII said:
By "degree 2 in v", you mean I should square the equation?

Do you remember the formula for solving a quadratic equation? If

ax^2 + bx + c = 0

then

x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}
 
  • #66
Alright, I think I got it. In nakurusil's solution, is the part between (brackets) multiplied by c^2 or u_xR? In your equation it looks like it's multiplied by the denominator, while as I calculated, it's multiplied by the numerator. Did I do something wrong or am I just reading the equation wrong?

Also, to get the solution, the abc-formula with the minus-sign was used and not with the plus-sign (I apologize for my lack of a better description so early in the morning). Why?
 
  • #67
Sunset said:
Hi rbj,



The relativistic momentum p_r = \frac{m_0 v}{\sqrt{1-\frac{v^2}{c^2}}} is defined in that way, because you want to have momentum-conservation.
Let me explain:
When you step from classical mechanics (Newtons axioms) to relativistic mechanics you need a new axiom-system. You have to define p_r in such a way that your relativistic theory is covariant and reproduces classical mechanics for low v. There might be indeed other choices for p_r which fullfill those two conditions - its simply the question if they describe reality.
p_r = \frac{m_0 v}{\sqrt{1-\frac{v^2}{c^2}}}
is the easiest choice which garantees conservation of p_r (e.g. Nolting, a german text-book, discusses this). Indeed it doesn't mean there are other possible choices, then you could describe physics with this p_r ' , too! The thing is you have a NEW physical quantity, which you should call "relativistic momentum".

Martin

Is it wrong to say that when you steo from classical mechanics to relativistic mechanics then there should use the addition law of relativistic velocities? So
p=mu (1)
p'=m'u' (2)
p/m=p'/m'(u/u') (3).
Expressing the right side of (3) as a function of physical quantities measured in I' via the addition law of relativistic velocities the way is paved for the transformation of momentum, mass(energy).
 
  • #68
NanakiXIII said:
Alright, I think I got it. In nakurusil's solution, is the part between (brackets) multiplied by c^2 or u_xR? In your equation it looks like it's multiplied by the denominator, while as I calculated, it's multiplied by the numerator. Did I do something wrong or am I just reading the equation wrong?

Come on, I gave you the equation, for sure you can solve it. How can you get involved with physics when your math is so weak?

v=c^2/u_x_R(1-\sqrt(1-u_x_R^2/c^2)=v=(1-\sqrt(1-u_x_R^2/c^2)*c^2/u_x_R


Also, to get the solution, the abc-formula with the minus-sign was used and not with the plus-sign (I apologize for my lack of a better description so early in the morning). Why?
For the obvious reason that the "+" solution would produce a v larger than c.
 
  • #69
Actually, I found your method of writing the equation rather ambiguous. But let's not turn this into another name-calling match, nakurusil.

I'll thank you for your help and leave it at that.
 
  • #70
NanakiXIII said:
Actually, I found your method of writing the equation rather ambiguous. But let's not turn this into another name-calling match, nakurusil.

I'll thank you for your help and leave it at that.

Good, I am sorry. I got frustrated with your math. The important thing is that you got a good solution.
 
  • #71
NanakiXIII said:
If anyone knows, however, of a derivation of this equation using the Lorentz transformations and preferably no other assumptions that are specifically within the theory of Special Relativity, if such a derivation exists at all, that would be the greatest help.
I gave this to you in your PM but I think its okay if I post it now. Since I had a feeling that someone would want to follow this derivation someday I placed it on my web page here.

http://www.geocities.com/physics_world/sr/inertial_mass.htm

Now others can read it and ask any questions they might have about it. The Lorent transformation manifests itself through the velocity transformation relations.

Pete
 
  • #72
Yes NanakiXIII, you are right. The literature usually skips over this derivation and the four-vector approach, while rigorous, usually leaves me cold. And, it is not the one that Einstein used.

I think, but I am not sure, that he used the idea of bouncing elastic balls, you know, one thrown from a moving train and the other one on the stationary platform.

But in the meantime, if you are comfortable with the idea of a Taylor's Series, you can expand "gamma" as a power series in "beta" and if you *start* with the idea that m/m0 = gamma = 1 + (1/2)beta2 + ... (higher powers) and this leads to the expression for kinetic energy:

(m-m0)c2 = (1/2)m0v2 + ... (higher terms),

So, it then becomes reasonable that (m-m0)c2 is in fact the kinetic energy and this of course makes us feel that this is probably the correct expression for relativistic mass. It does have the right form.

Einstein's approach to SR was quite novel. He *assumed* that a relativity principle applied not only to mechanical phenomena, but electromagnetic as well ... and that was a great leap of faith. It turns out that he was quite right, but he was the only one at the time to venture such an idea.
 
  • #73
By special relativity, we have time dilation and space contraction by this "gamma." Time is increased by division of the reference time by this gamma and distance is reduced by multiplication by this gamma. For f = ma, because the translation distance is shortened by this factor, the acceleration, compared to the inertial reference is shortened, but force is constant, so the mass must be increased to make up for the lost acceleration.

The derivation of this gamma is done by Einstein in his relativity book. It is an algebraic derivation with no calculus.

Once we know that relativistic mass changes with velocity, we show that a loss in velocity results in a loss in mass and pure energy being releasedf (delta m x c^2)

remember [(1 - v^2/c^2)]^-1/2 = (closely) 1 + (1/2)(v^2/c^2)

relativistic mass - inertial mass = inertial mass + (1/2)inertial mass x loss in velocity^2/c^2) - inertial mass = (1/2)inertial mass x loss in velocity^2/c^2)
delta mass x c^w = 1/2inertail mass x loss in velocity^2 = "mc^2" qed

Again, this requires that relativistic mass is increased from inertial mass by division by this gamma and it is the law of ther conservation of momentum or energy which requires mass to increase when linear acceleration id reduced by space contraction.
 
  • #74
jhigbie said:
Einstein's approach to SR was quite novel. He *assumed* that a relativity principle applied not only to mechanical phenomena, but electromagnetic as well ... and that was a great leap of faith. It turns out that he was quite right, but he was the only one at the time to venture such an idea.

PMFJI, but this isn't true. Lorentz derived the Lorentz transformation well before Einstein did, as did Larmor. Their derivations were specifically intended to find the transformation laws for the electromagnetic field that would be compatible with Maxwell's Equations. See the section on "Historical Developments" in the "[URL page on Maxwell's Equations[/URL]. What Einstein did was to assume that *mechanical* phenomena were governed by the Lorentz transformation, and work out the consequences; the consequences for electromagnetism were already well known.
 
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  • #75
jhigbie said:
I think, but I am not sure, that he used the idea of bouncing elastic balls, you know, one thrown from a moving train and the other one on the stationary platform.

In the version of this thought experiment that's in his popular book on relativity, _Relativity: A Clear Explanation That Anyone Can Understand_, he used light flashes, emitted from each end of a moving train. I haven't been able to find an online reference that contains his description of the scenario.
 
  • #76
The flashing lights, etc. are in his book "Relativity"
 
  • #77
Remember that assumptions of constant c and the preservation of laws of physics in all inertial time frames leads to a mathematical "proof" of the Lorentz transforms. They are equivalent statements.

Many college textbooks actually derive the "relatvistic mass" equation by itself based on the Lorentz transforms.
 
  • #78
Energy-Momentum Relation:

E2 = (m0c2)2 + (pc)2

Substitute mc2 for E (energy-mass equivilence)

Substitute mv for p (relation between mass, velocity, and momentum)

it should look like this:

(mc2)2 = (m0c2)2 + (mvc)2

Subtract (mvc)2 over..

(mc2)2 - (mvc)2 = (m0c2)2

m2c4 - m2v2c2 = m02c4

Factor out (mc2) on the left..

(mc2) (c2 - v2) = (m0c2)2

Factor out a c2 from the second set of parenthesis above...

(mc2) (c2) (1 - v2 / c2) = m02c4

Take the square root of both sides...

mc2 * √(1 - v2 / c2) = m0c2

"c2"s cancel out and then divide the √(1 - v2 / c2) over..

m = m0 / √(1 - v2 / c2) [relativistic mass-invariant mass relation]

m: relativistic mass
m0: rest mass (invariant mass)
v: velocity
c: the speed limit of the universe
p: momentum
E: energy
 
  • #79
pa0+pb0=pa1+pb1

γ(va0).ma.va0+γ(vb0).mb.vb0=γ(va1).ma.va1+γ(vb1).mb.vb1

This is the general expression for the relativistic momentum conservation with two particles, where 'ma' and 'mb' are the rest masses of the particles.
To understand the relativistic momentum definition, we need to see why this expression is valid for moving systems, upon the multiplication of the factor γ(v). So it is important to bear in mind the relation between time and proper time, as we can deduce from the basic experiment of a light ray in a moving mirror:

Δt2-Δx2/c2=Δζ2

Δζ/Δt=√(1-v2/c2)=γ(v) →

γ(v)/Δt=1/Δζ (proper time)

Now, using the speed "diferential definition" (Δx/Δt), and applying the relation whith proper time above to the expression of momentum conservation along the 'x' coordinate, we get:

ma.Δxa0/Δζa+mb.Δxb0/Δζb=ma.Δxa1/Δζa+mb.Δxb1/Δζb

Applying the Lorentz transformation Δx=γ(V)(Δx'-V.Δt'), we obtain (canceling the commun term γ(V)):

ma.Δx'a0/Δζa-ma.Δx'a0V.Δt'/Δζa+mb.Δx'b0/Δζb-mb.Δx'b0V.Δt'/Δζb=ma.Δx'a1/Δζa-ma.Δx'a1V.Δt'/Δζa+mb.Δx'b1/Δζb-mb.Δx'b1V.Δt'/Δζb

Applying again the relation between proper time and time we have:

γ(v'a0).ma.v'a0+γ(v'b0).mb.v'b0-γ(v'a0).ma.V-γ(v'b0).mb.V=γ(v'a1).ma.v'a1+γ(v'b1).mb.v'b1-γ(v'a1).ma.V-γ(v'b1).mb.V

In this expression, if the equality

γ(v'a0).ma+γ(v'b0).mb=γ(v'a1).ma+γ(v'b1).mb

holds (this is the relatIvistic "condition" tor relativistic momentum conservation), then we have the momentum conservation:

γ(v'a0).ma.v'a0+γ(v'b0).mb.v'b0=γ(v'a1).ma.v'a1+γ(v'b1).mb.v'b1

p'a0+p'b0=p'a1+p'b1

With respect to the transversal components (x and y), the result is analogous and imediate...
 

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