Mathematical Principles of Theoretical Physics

(Rick Simeone) #1

2.6. PRINCIPLE OF HAMILTONIAN DYNAMICS (PHD) 103


whereψ= (ψ 1 ,ψ 2 )T, andψk=ψk^1 +iψ^2 k( 1 ≤k≤ 2 ). The Hamilton energyHof (2.6.51)
is in the form


H=



R^3

iψ†(~σ·∇)ψdx

(2.6.52)


=



R^3

[


∂ ψ 12
∂x^1

ψ 21 +

∂ ψ 22
∂x^1

ψ 11 +

∂ ψ^21
∂x^2

ψ^22 +

∂ ψ 11
∂x^2

ψ 21 +

∂ ψ 12
∂x^3

ψ 11 +

∂ ψ 21
∂x^3

ψ 11 +

∂ ψ^12
∂x^3

ψ^22

]


dx.

The Hamilton equations are


1
c

∂ ψk^1
∂t

=


δ
δ ψk^2

H,


1


c

∂ ψk^2
∂t

=−


δ
δ ψk^1

H,


fork= 1 , 2 ,

which, in view of for (2.6.52), are in the form:


(2.6.53)


1


c

∂ ψ 11
∂t

=


(


∂ ψ^12
∂x^1

+


∂ ψ^22
∂x^2

+


∂ ψ 11
∂x^3

)


,


1


c

∂ ψ 12
∂t

=


(


∂ ψ^22
∂x^1


∂ ψ^12
∂x^2

+


∂ ψ 12
∂x^3

)


,


1


c

∂ ψ 21
∂t

=


(


∂ ψ^11
∂x^1


∂ ψ^21
∂x^2


∂ ψ 21
∂x^3

)


,


1


c

∂ ψ 22
∂t

=


(


∂ ψ^21
∂x^1

+


∂ ψ^11
∂x^2


∂ ψ 22
∂x^3

)


.


It is readily to check that (2.6.53) and (2.6.51) are equivalent.


3.Dirac equations:

(2.6.54) ih ̄


∂ ψ
∂t

=−ihc ̄ (~α·∇)ψ+mc^2 α 0 ψ,

where~α,α 0 are as in (2.2.58),ψ= (ψ 1 ,ψ 2 ,ψ 3 ,ψ 4 )T, and


ψk=ψk^1 +iψk^2 for 1≤k≤ 4.

The Hamilton energy of (2.6.54) is defined by


(2.6.55) H=



R^3

[


−i ̄hcψ†(~α·∇)ψ+mc^2 ψ†α 0 ψ

]


dx.

It is clear that the expansions of (2.6.54) in terms of real and imaginary parts are in the form


h ̄

∂ ψk^1
∂t

=−


δ
δ ψk^2

H,


h ̄

∂ ψk^2
∂t

=


δ
δ ψk^1

H,


for 1≤k≤ 4 ,
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