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

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The discussion centers on understanding the implications of different values of the super-Hamiltonian, ##\mathcal H##, in the context of geodesic motion equations. Participants explore how dimensionless quantities relate to the Hamiltonian formulation and the significance of choosing specific values for ##\mathcal H##, particularly in relation to parameterization and the nature of geodesics. Clarifications are made regarding the dimensional consistency of equations and the role of reparameterization in eliminating certain terms. The conversation also touches on deriving geodesic equations using Hamilton's equations and the conditions under which ##\mathcal H## remains a constant of motion. Overall, the thread emphasizes the mathematical intricacies of the super-Hamiltonian approach to 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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