Problem with dimensionless quantities in an equation requiring M^2 (Super Hamiltonian Formulation for Geodesic Motion)

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SUMMARY

The discussion centers on the interpretation of dimensionless quantities in the context of the Super Hamiltonian formulation for geodesic motion, specifically regarding the parameterization choices of the Hamiltonian, denoted as ##\mathcal H##. Participants clarify that while certain values of ##\mathcal H##, such as ##-½\mu^2##, have dimensions of [Mass]^2, others like ##+½## and ##-½## are dimensionless. The equations derived, including ##\big (\frac {dr}{d\tau} \big ) ^2## and ##\big (\frac {dr}{d\lambda} \big ) ^2##, illustrate the relationship between energy, angular momentum, and the geodesic paths in a gravitational field. The discussion emphasizes the importance of proper parameterization and the implications of Hamilton's equations in deriving geodesic equations.

PREREQUISITES
  • Understanding of Hamiltonian mechanics and Hamilton's equations.
  • Familiarity with geodesic motion in general relativity.
  • Knowledge of dimensional analysis in physics.
  • Proficiency in mathematical notation used in theoretical physics, particularly tensor calculus.
NEXT STEPS
  • Study the derivation of geodesic equations from Hamilton's equations in the context of general relativity.
  • Explore the implications of different parameterizations of the Hamiltonian in geodesic motion.
  • Investigate the role of dimensionless quantities in physical equations and their significance.
  • Review Box 25.3 and Box 25.6 from relevant texts for deeper insights into Hamiltonian formulations.
USEFUL FOR

The discussion is beneficial for theoretical physicists, graduate students in physics, and anyone studying general relativity and Hamiltonian mechanics, particularly those interested in the mathematical foundations of geodesic motion.

  • #31
TerryW said:
##\mathcal H = -\frac {1}{2} = \frac {1}{2}p_\mu p^\mu##

##p_\mu p^\mu = -1 = m^2 \textbf u^2##

But ##\textbf u^2 = -1 ##

So ##p_\mu p^\mu = -1 = -m^2##

So ##m^2 = 1, \quad \textbf p = \textbf u, \quad \frac {d}{d\lambda} = \frac {d}{d\tau} , \quad \lambda = \tau##
...
What does the ##~m~## in ##~m^2~## stand for?
 
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  • #32
m is the rest mass. Should have stuck to ##\mu##.
 
  • #33
TerryW said:
m is the rest mass. Should have stuck to ##\mu##.
So how can you get ##~m^2=-1~## as in post #30 ?

Take for example the trivial case ##~\lambda=\tau~## in Minkowski SR spacetime, where the geodesic is the straight line ##~x^\mu(\tau)=(\tau,0,0,0)~## . You get ## ~p^\mu=\frac{dx^\mu}{d\lambda}=u^\mu=\delta^\mu_0~## and ##~\mathcal H=-\frac 1 2~## . But how can you infer a mass from it?

Edit: Addition
##p^\mu=\frac{dx^\mu}{d\lambda}~## is the vector field on the curve of tangent vectors to it, whose components (in a given chart) are scaled by the parametrization ##~\lambda~##. It is proportional to ##~u^\mu~## , but the proportionality factor is not ##~\mu~## (except for the case where ##~\mathcal H=-\frac 1 2 \mu^2~## ), so in general it is not equal to the "mechanical 4-momentum" ##~\mu \mathbf u~## . Moreover, what sense does it make to talk of masses in the case of spacelike geodesics?
 
Last edited:
  • #34
I know that ##m^2 = -1 ## is problematical! It's just that the maths lead to that result.

I looked on the internet for some kind of discussion of what is happening in the spacelike realm of spacetime and didn't find anything useful. I have hazy memories of people postulating tachyons which accelerate when a retarding force is applied and decelerate when a positive force is applied (negative mass but not imaginary mass?).
 
  • #35
Hi TerryW

After 3 months on this thread, I give up.
I apologize for accepting the challenge (which turned out to be beyond my capabilities), since by doing so I possibly deprived you from getting a better help.

Thanks for your pleasant company :smile:

Regards,

JimWhoKnew
 
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  • #36
I actually feel that you’ve helped me a great deal with this problem and the exchange has improved my understanding of what parameterisation is all about and that ##\frac{d}{d\lambda}## is something more abstract than classical momentum.
So you’ve most certainly helped me more than you think you have!
Regards

TerryW
 
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