A few questions about the Lorentz factor

  • Context: Graduate 
  • Thread starter Thread starter kotreny
  • Start date Start date
  • Tags Tags
    Lorentz Lorentz factor
Click For Summary
SUMMARY

The discussion centers on the implications of the Lorentz factor (\(\gamma\)) in the context of faster-than-light (FTL) speeds and its mathematical properties. Participants explore the relationship between \(\gamma\) and hyperbolic functions, particularly rapidity, which offers a new perspective on motion. The conversation also touches on the geometric interpretations of relativistic concepts, including length contraction and energy-momentum relationships. Key mathematical insights include the integration of \(\gamma\) and its connection to arcsin, as well as the use of hyperbolic functions for relativistic calculations.

PREREQUISITES
  • Understanding of the Lorentz factor (\(\gamma\)) and its mathematical formulation.
  • Familiarity with hyperbolic functions (sinh, cosh, tanh) and their applications in physics.
  • Basic knowledge of calculus and integration techniques.
  • Concepts of special relativity, including time dilation and length contraction.
NEXT STEPS
  • Study the mathematical derivation of the Lorentz transformation equations.
  • Learn about rapidity and its advantages over traditional velocity measurements.
  • Explore the implications of complex numbers in the context of FTL travel and wormholes.
  • Investigate the relationship between energy and mass in relativistic physics, particularly through the lens of \(E=mc^2\).
USEFUL FOR

Students of physics, particularly those focusing on special relativity, mathematicians interested in the applications of hyperbolic functions, and anyone exploring advanced concepts in theoretical physics.

kotreny
Messages
46
Reaction score
0
I have only a rudimentary knowledge of the subject and would like more info about:

1)

The consequences of faster-than-light speed. I noticed that \gamma would then involve complex numbers, and seeing as complex analysis is definitely more than imaginary, I was wondering what it could mean, both mathematically and physically (wormholes?). Unfortunately, I haven't gone very far into math higher than calculus yet. Hopefully soon to change.

2)

\gamma bears more than a passing resemblance to the derivative of arcsin. Details?
 
Physics news on Phys.org
kotreny said:
\gamma bears more than a passing resemblance to the derivative of arcsin. Details?
You are nearly right. When I started high energy physics ~50 years ago, we did not have pocket calculators. We had only slide rules and trig tables. If you look up β in the sin(θ) column of the trig tables, then cos(θ) = 1/γ.

Consider β = 1/2. Look up sin(θ) = 1/2, and find cos(θ) = 0.86603, so γ = 1.155

Also if you set one side of a right angle triangle to the rest mass and the other side to the relativistic momentum (in energy units) then the hypotenous is the total energy.

So who needs pocket calculators?

Bob S
 
Last edited:
If you integrate \gamma=c/(c^2-v^2)^.5 wrt v, then you get c*arcsin(v/c), since c is constant.

Geometrically, this means if you have a point on a circle of radius c, with vertical component v, then the angle will be arcsin(v/c) in radians. Multiplying this by c will yield the arc length. \gamma is therefore dS/dv, S being arc traversed, measured in units of velocity.

That's about as far as I've gone. No idea what it means though; still learning the ropes. Don't forget to address 1)--suggesting some online resource or book would be helpful.
 
hello kotreny-

Please look at my thumbnail. I have drawn 3 triangles, all with the same included angle θ.
One triangle is your description, one shows the relationship between β γ and θ. the third shows the relation between total energy, momentum (in energy units), and rest mass. See also the trig relations.
Please review.

Bob S
 

Attachments

  • Relativistic_betagamma.jpg
    Relativistic_betagamma.jpg
    22.7 KB · Views: 830
It turns out that there are good reasons for using hyperbolic functions (sinh, cosh, tanh) instead of trig functions (sin, cos, tan). The relevant equations then become

\begin{array}{rl}<br /> \sinh \phi &amp; = \gamma \beta = \gamma v / c\\<br /> \cosh \phi &amp; = \gamma \\<br /> \tanh \phi &amp; = \beta = v/c \\<br /> \\<br /> p &amp; = m_0 c \, \sinh \phi \\<br /> E &amp; = m_0 c^2 \cosh \phi \\<br /> \end{array}​

The quantity \phi is called rapidity, and is another way to measure motion instead of velocity. At non-relativistic speeds, the rapidity approximates to v/c. The rapidity of light is infinite, relative to any inertial observer.
 
This is so cool. It makes more sense than ever.

Here's another one which I thought worth noting. The travel time, as seen by a stationary observer, for a continuously accelerated motion (from v=0 to v=0 again)...

t2 = 4.s/a + (s/c)2

...notice how it compares to the Newtonian version

t2 = 4.s/a

...thus differing only by the light-travel time component.

Really does make it all space-time rather than just space and time.
 
DrGreg said:
The quantity \phi is called rapidity, and is another way to measure motion instead of velocity. At non-relativistic speeds, the rapidity approximates to v/c. The rapidity of light is infinite, relative to any inertial observer.

You didn't mention the best thing of all about rapidity - it, unlike velocity, is additive.
 
Vanadium 50 said:
You didn't mention the best thing of all about rapidity - it, unlike velocity, is additive.
True.

Also the proper acceleration of an object is c \, d\phi / d\tau, where \tau is proper time.

The Lorentz transform is

\begin{array}{rcrcr}<br /> ct&#039; &amp; = &amp; ct \cosh \phi &amp; - &amp; x \sinh \phi \\<br /> x&#039; &amp;= &amp; -ct \sinh \phi &amp; + &amp; x \cosh \phi<br /> \end{array}​

remarkably similar to a rotation in Euclidean space.

Doppler blue shift is e^{\phi}. Doppler red shift is e^{-\phi}.

One drawback, though. Rapidity is a scalar, not a vector. Think of it as the angle between two worldlines in 4D spacetime.
 
Thank you for the reply, Dr Greg, but I have yet to thoroughly familiarize myself with the hyperbolic functions! :redface: I look forward to reviewing this thread in the near future.

Hello Bob, interesting thumbnail. I will definitely explore this connection more deeply once I am comfortable with the formulas involved. I can see why the triangles are similar.

This is digressing, but I just noticed yesterday that if space and time were expressed in the same units, then c would be a dimensionless ratio, and E=mc^2 would officially allow energy and mass to be expressed in the same units as well. Imagine: a unit for both space and time!


Again, could someone please give me more info about the mathematical results of faster-than-light speed? At least let me know if there's a proof that the complex numbers involved cannot have meaning. Thanks.
 
  • #10
I found another triangle that should be added to Bob's three. It puts a new perspective on length contraction.
The hypotenuse is L (the rest length), the opposite side is \betaL, and, interestingly, the adjacent is L*sqrt(1-\beta^2). It's easy to see that the triangle is similar.

My interpretation is this: Visualize a circle, tilted at an angle to you. The circle will look like an ellipse in your view, and by my calculation the minor axis will be the diameter times the cosine of the tilt angle. The length contraction would be calculated in exactly the same manner if the circle were moving relative to you. Also note that when an object is tilted, there is no change along the axis of revolution.
Could this mean that, somehow, space "tilts away" when there is motion? It also makes it easy to see that contraction of the other is observed in both frames of reference, because the "tilt" is the same in both perspectives, just in opposite directions.
 
  • #11
kotreny said:
I found another triangle that should be added to Bob's three. It puts a new perspective on length contraction.
The hypotenuse is L (the rest length), the opposite side is \betaL, and, interestingly, the adjacent is L*sqrt(1-\beta^2). It's easy to see that the triangle is similar.

My interpretation is this: Visualize a circle, tilted at an angle to you. The circle will look like an ellipse in your view, and by my calculation the minor axis will be the diameter times the cosine of the tilt angle. The length contraction would be calculated in exactly the same manner if the circle were moving relative to you. Also note that when an object is tilted, there is no change along the axis of revolution.
Could this mean that, somehow, space "tilts away" when there is motion? It also makes it easy to see that contraction of the other is observed in both frames of reference, because the "tilt" is the same in both perspectives, just in opposite directions.
Hi Kotreny-
You need to read this paper in Phys Rev
http://prola.aps.org/abstract/PR/v116/i4/p1041_1
Sorry, it is pay per view.
Bob S
 
  • #12
kotreny said:
This is digressing, but I just noticed yesterday that if space and time were expressed in the same units, then c would be a dimensionless ratio, and E=mc^2 would officially allow energy and mass to be expressed in the same units as well. Imagine: a unit for both space and time!

This is exactly what we do, actually. Typically we choose the units such that c = 1 (a dimensionless number). In these units, mass and energy have the same dimensions, as do time and distance. In fact, mass has the same units as 1/length.
 
  • #13
Ben Niehoff said:
This is exactly what we do, actually. Typically we choose the units such that c = 1 (a dimensionless number). In these units, mass and energy have the same dimensions, as do time and distance. In fact, mass has the same units as 1/length.
Theorists sometimes confuse the rest of us by setting many fundamental constants to "1" for convenience; like hbar=c=1. This makes it very hard to detemine the units of an equation.
Bob S
 

Similar threads

  • · Replies 101 ·
4
Replies
101
Views
7K
  • · Replies 23 ·
Replies
23
Views
2K
  • · Replies 13 ·
Replies
13
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 55 ·
2
Replies
55
Views
5K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 21 ·
Replies
21
Views
3K
  • · Replies 46 ·
2
Replies
46
Views
9K
  • · Replies 1 ·
Replies
1
Views
3K
  • · Replies 184 ·
7
Replies
184
Views
23K