This quantum world/Feynman route/Energy and momentum

From testwiki
Revision as of 15:08, 25 August 2008 by 217.86.167.205 (talk)
(diff) ← Older revision | Latest revision (diff) | Newer revision β†’ (diff)
Jump to navigation Jump to search

Template:Noprint

Energy and momentum

Observe that if dS does not depend on t (that is, dS/t=0 ) then

E=dSdt

is constant along geodesics. (We'll discover the reason for the negative sign in a moment.)

Likewise, if dS does not depend on π« (that is, dS/𝐫=0 ) then

𝐩=dSd𝐫

is constant along geodesics.

E tells us how much the projection dt of a segment dπ’ž of a path π’ž onto the time axis contributes to the action of π’ž. 𝐩 tells us how much the projection d𝐫 of dπ’ž onto space contributes to S[π’ž]. If dS has no explicit time dependence, then equal intervals of the time axis make equal contributions to S[π’ž], and if dS has no explicit space dependence, then equal intervals of any spatial axis make equal contributions to S[π’ž]. In the former case, equal time intervals are physically equivalent: they represent equal durations. In the latter case, equal space intervals are physically equivalent: they represent equal distances.

If equal intervals of the time coordinate or equal intervals of a space coordinate are not physically equivalent, this is so for either of two reasons. The first is that non-inertial coordinates are used. For if inertial coordinates are used, then every freely moving point mass moves by equal intervals of the space coordinates in equal intervals of the time coordinate, which means that equal coordinate intervals are physically equivalent. The second is that whatever it is that is moving is not moving freely: something, no matter what, influences its motion, no matter how. This is because one way of incorporating effects on the motion of an object into the mathematical formalism of quantum physics, is to make inertial coordinate intervals physically inequivalent, by letting dS depend on t and/or π«.

Thus for a freely moving classical object, both E and 𝐩 are constant. Since the constancy of E follows from the physical equivalence of equal intervals of coordinate time (a.k.a. the "homogeneity" of time), and since (classically) energy is defined as the quantity whose constancy is implied by the homogeneity of time, E is the object's energy.

By the same token, since the constancy of π© follows from the physical equivalence of equal intervals of any spatial coordinate axis (a.k.a. the "homogeneity" of space), and since (classically) momentum is defined as the quantity whose constancy is implied by the homogeneity of space, 𝐩 is the object's momentum.

Let us differentiate a former result,

dS(t,𝐫,λdt,λd𝐫)=λdS(t,𝐫,dt,d𝐫),

with respect to λ. The left-hand side becomes

d(dS)dλ=dS(λdt)(λdt)λ+dS(λd𝐫)(λd𝐫)λ=dS(λdt)dt+dS(λd𝐫)d𝐫,

while the right-hand side becomes just dS. Setting λ=1 and using the above definitions of E and 𝐩, we obtain

Edt+𝐩d𝐫=dS.

dS=mc2ds is a 4-scalar. Since (cdt,d𝐫) are the components of a 4-vector, the left-hand side, Edt+𝐩d𝐫, is a 4-scalar if and only if (E/c,𝐩) are the components of another 4-vector.

(If we had defined E without the minus, this 4-vector would have the components (E/c,𝐩).)

In the rest frame β„± of a free point mass, dt=ds and dS=mc2dt. Using the Lorentz transformations, we find that this equals

dS=mc2dtvdx/c21v2/c2=mc21v2/c2dt+m𝐯1v2/c2d𝐫,

where 𝐯=(v,0,0) is the velocity of the point mass in β„±. Compare with the above framed equation to find that for a free point mass,

E=mc21v2/c2𝐩=m𝐯1v2/c2.


Template:Noprint