Darwin Lagrangian

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The Darwin Lagrangian (named after Charles Galton Darwin, grandson of the biologist) describes the interaction to order \frac{v^2}{c^2} between two charged particles in a vacuum and is given by[1]

 L = L_\text{f} + L_\text{int},

where the free particle Lagrangian is

 L_\text{f} = \frac{1}{2} m_1 v_1^2 + \frac{1}{8c^2} m_1 v_1^4 + \frac{1}{2} m_2 v_2^2 + \frac{1}{8c^2} m_2 v_2^4,

and the interaction Lagrangian is

 L_\text{int} = L_\text{C} + L_\text{D},

where the Coulomb interaction is

L_\text{C} = -\frac{q_1 q_2}{r},

and the Darwin interaction is

 L_\text{D} = \frac{q_1 q_2}{r} \frac{1}{2c^2} \mathbf v_1 \cdot \left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right] \cdot \mathbf v_2.

Here q1 and q2 are the charges on particles 1 and 2 respectively, m1 and m2 are the masses of the particles, v1 and v2 are the velocities of the particles, c is the speed of light, r is the vector between the two particles, and \hat{\mathbf r} is the unit vector in the direction of r.

The free Lagrangian is the Taylor expansion of free Lagrangian of two relativistic particles to second order in v. The Darwin interaction term is due to one particle reacting to the magnetic field generated by the other particle. If higher-order terms in v/c are retained, then the field degrees of freedom must be taken into account, and the interaction can no longer be taken to be instantaneous between the particles. In that case retardation effects must be accounted for.

Derivation of the Darwin interaction in a vacuum[edit]

The relativistic interaction Lagrangian for a particle with charge q interacting with an electromagnetic field is[2]

 L_\text{int} = -q\Phi + {q\over c} \mathbf u \cdot \mathbf A,

where u is the relativistic velocity of the particle. The first term on the right generates the Coulomb interaction. The second term generates the Darwin interaction.

The vector potential in the Coulomb gauge is described by[3] (Gaussian units)

 \nabla^2 \mathbf A - {1\over c^2} {\partial^2 \mathbf A \over \partial t^2} = -{4\pi \over c} \mathbf J_t

where the transverse current Jt is the solenoidal current (see Helmholtz decomposition) generated by a second particle. The divergence of the transverse current is zero.

The current generated by the second particle is

  \mathbf J = q_2 \mathbf v_2 \delta \left( \mathbf r - \mathbf r_2 \right),

which has a Fourier transform

  \mathbf J\left( \mathbf k \right) \equiv  \int d^3r \exp\left( -i\mathbf k \cdot \mathbf r \right) \mathbf J\left( \mathbf r \right) = q_2 \mathbf v_2 \exp\left( -i\mathbf k \cdot \mathbf r_2 \right).

The transverse component of the current is

\mathbf J_t\left( \mathbf k \right) = q_2 \left[ \mathbf 1 - \mathbf{\hat k} \mathbf{\hat k} \right] \cdot \mathbf v_2 \exp\left( -i\mathbf k \cdot \mathbf r_2 \right).

It is easily verified that

\mathbf k \cdot \mathbf J_t\left( \mathbf k \right) = 0,

which must be true if the divergence of the transverse current is zero. We see that

\mathbf J_t\left( \mathbf k \right)

is the component of the Fourier transformed current perpendicular to k.

From the equation for the vector potential, the Fourier transform of the vector potential is

  
 \mathbf A \left( \mathbf k \right)
 = {4\pi \over c} {q_2\over k^2} \left[ \mathbf 1 - \mathbf{\hat k} \mathbf{\hat k} \right] \cdot \mathbf v_2
\exp\left( -i\mathbf k \cdot \mathbf r_2 \right)

where we have kept only the lowest order term in v/c.

The inverse Fourier transform of the vector potential is

\mathbf A \left( \mathbf r \right)  
=\int { d^3 k \over \left ( 2 \pi \right ) ^3 } \; \mathbf A \left( \mathbf k \right) \;{ \exp \left ( i \mathbf k \cdot \mathbf r_1 \right )  } 
= {q_2\over 2c} {1 \over  r } \left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right] \cdot \mathbf v_2

where

\mathbf r = \mathbf r_1 - \mathbf r_2

(see Common integrals in quantum field theory ).

The Darwin interaction term in the Lagrangian is then

L_{D} = 
{q_1 q_2\over r} {1 \over 2c^2  } \mathbf v_1 \cdot 
\left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right]
\cdot \mathbf v_2

where again we kept only the lowest order term in v/c.

Lagrangian equations of motion[edit]

The equation of motion for one of the particles is

  {d \over dt} {\partial  \over \partial \mathbf v_1} L\left( \mathbf r_1 , \mathbf v_1 \right) = \nabla_1 L\left( \mathbf r_1 , \mathbf v_1 \right)
  {d \mathbf p_1 \over dt} = \nabla_1 L\left( \mathbf r_1 , \mathbf v_1 \right)

where p1 is the momentum of the particle.

Free particle[edit]

The equation of motion for a free particle neglecting interactions between the two particles is

{d \over dt} \left[ \left( 1   + {1\over 2} { v_1^2\over c^2 } \right)m_1\mathbf v_1 \right]=0
 \mathbf p_1 = \left( 1   + {1\over 2} { v_1^2\over c^2 } \right)m_1\mathbf v_1

Interacting particles[edit]

For interacting particles, the equation of motion becomes

  {d \over dt} \left[ \left( 1   + {1\over 2} { v_1^2\over c^2 } \right)m_1\mathbf v_1 +{q_1\over c}\mathbf A\left( \mathbf r_1 \right) \right]=
-\nabla {q_1 q_2 \over r}
+\nabla \left[ {q_1q_2 \over  r }{1\over 2c^2}
\mathbf v_1\cdot  
\left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right]
\cdot\mathbf v_2 \right]


 {d \mathbf{p}_1\over dt} 
= {q_1 q_2 \over r^2}{\hat{\mathbf r}}
+{q_1 q_2 \over r^2}{1\over 2c^2} 
\left\{ \mathbf v_1 \left( { {\hat{\mathbf r}}\cdot \mathbf v_2} \right) 
+  \mathbf v_2 \left( { {\hat{\mathbf r}}\cdot \mathbf v_1}\right)
- {\hat{\mathbf r}} \left[ \mathbf v_1 \cdot \left( \mathbf 1 +3 {\hat{\mathbf r}}{\hat{\mathbf r}}\right)\cdot \mathbf v_2\right]
 \right\}


 \mathbf p_1 =
\left( 1   + {1\over 2} { v_1^2\over c^2 } \right)m_1\mathbf v_1
+{q_1\over c}\mathbf A\left( \mathbf r_1 \right)


\mathbf A \left( \mathbf r_1 \right)  =  {q_2\over 2c} {1 \over  r }  
\left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right]
\cdot \mathbf v_2
\mathbf r =\mathbf r_1 - \mathbf r_2

Darwin Hamiltonian for two particles in a vacuum[edit]

The Darwin Hamiltonian for two particles in a vacuum is related to the Lagrangian by a Legendre transformation

  H = \mathbf p_1 \cdot \mathbf v_1 + \mathbf p_2 \cdot \mathbf v_2 - L.

The Hamiltonian becomes

 H\left( \mathbf r_1 , \mathbf p_1 ,\mathbf r_2 , \mathbf p_2 \right)=
\left( 1   - {1\over 4} { p_1^2\over m_1^2 c^2 } \right){ p_1^2 \over 2 m_1}
\; + \; \left( 1   - {1\over 4} { p_2^2\over m_2^2 c^2 } \right){ p_2^2 \over 2 m_2}
\; + \; {q_1 q_2 \over r }
\; - \; {q_1q_2 \over  r }{1\over 2m_1 m_2 c^2}
\mathbf p_1\cdot  
\left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right]
\cdot\mathbf p_2
  .

Hamiltonian equations of motion[edit]

The Hamiltonian equations of motion are

  \mathbf v_1 = {\partial H \over \partial \mathbf p_1}

and

  {d \mathbf p_1 \over dt} = -\nabla_1 H

which yield

  \mathbf v_1  =
\left( 1- {1\over 2} {p_1^2 \over m_1^2 c^2}  \right) {\mathbf p_1 \over m_1}
- {q_1 q_2\over 2m_1m_2 c^2} {1 \over  r }  
\left[\mathbf 1 + \mathbf{\hat r} \mathbf{\hat r}\right]
\cdot \mathbf p_2

and

  {d \mathbf p_1\over dt} = {q_1 q_2 \over r^2}{\hat{\mathbf r}}
\; + \; {q_1 q_2 \over r^2}{1\over 2m_1 m_2 c^2} 
\left\{ \mathbf p_1 \left( { {\hat{\mathbf r}}\cdot \mathbf p_2} \right) 
+  \mathbf p_2 \left( { {\hat{\mathbf r}}\cdot \mathbf p_1}\right)
- {\hat{\mathbf r}} \left[ \mathbf p_1 \cdot \left( \mathbf 1 +3 {\hat{\mathbf r}}{\hat{\mathbf r}}\right)\cdot \mathbf p_2\right]
 \right\}

Note that the quantum mechanical Breit equation originally used the Darwin Lagrangian with the Darwin Hamiltonian as its classical starting point though the Breit equation would be better vindicated by the Wheeler–Feynman absorber theory and better yet quantum electrodynamics.

See also[edit]

References[edit]

  1. ^ Jackson, John D. (1998). Classical Electrodynamics (3rd ed.). Wiley. ISBN 047130932X.  pp. 596-598
  2. ^ Jackson, pp. 580-581.
  3. ^ Jackson, p. 242.