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two-body_problem [2013/11/09 20:36]
nikolaj
two-body_problem [2015/08/19 19:50]
nikolaj
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 ===== Two-body problem ===== ===== Two-body problem =====
-==== Definition ​==== +==== Set ==== 
-| @#FFBB00: $\langle \mathbb R^{2\times 3}, H\rangle \in \mathrm{it} $ ... Classical Hamiltonian system |+| @#FFBB00: definiendum ​| @#FFBB00: $\langle \mathbb R^{2\times 3}, H\rangle \in \mathrm{it} $ ... Classical Hamiltonian system |
  
-| @#55EE55: $ H({\bf r}_1,{\bf r}_2,{\bf p}_1,{\bf p}_2) = \frac{1}{m_1}\frac{1}{2}{\bf p}_1^2 + \frac{1}{m_2}\frac{1}{2}{\bf p}_2^2 + V(|{\bf r}_1-{\bf r}_2|) $ |+| @#55EE55: postulate ​  | @#55EE55: $ H({\bf r}_1,{\bf r}_2,{\bf p}_1,{\bf p}_2) = \frac{1}{m_1}\frac{1}{2}{\bf p}_1^2 + \frac{1}{m_2}\frac{1}{2}{\bf p}_2^2 + V(|{\bf r}_1-{\bf r}_2|) $ |
  
-==== Discussion ​====+----- 
 +=== Discussion ===
 == Equations of motion in suitable coordinates == == Equations of motion in suitable coordinates ==
-| @#DDDDDD: $ M \equiv m_1+m_2 $ | +| @#DDDDDD: range       | @#DDDDDD: $ M \equiv m_1+m_2 $ | 
-| @#DDDDDD: $ \mu \equiv m_1 m_2/M $ |+| @#DDDDDD: range       | @#DDDDDD: $ \mu \equiv m_1 m_2/M $ |
  
 The following choice of coordinates eliminates the singles out the center of mass, which the Hamiltonian is independent of. The following choice of coordinates eliminates the singles out the center of mass, which the Hamiltonian is independent of.
  
-| @#DDDDDD: $ {\bf r} \equiv {\bf r}_2 - {\bf r}_1 $ | +| @#DDDDDD: range       | @#DDDDDD: $ {\bf r} \equiv {\bf r}_2 - {\bf r}_1 $ | 
-| @#DDDDDD: $ {\bf R} \equiv (m_1\ {\bf r}_1 + m_2\ {\bf r}_2)/M $ | +| @#DDDDDD: range       | @#DDDDDD: $ {\bf R} \equiv (m_1\ {\bf r}_1 + m_2\ {\bf r}_2)/M $ | 
-| @#DDDDDD: $ {\bf p} \equiv (m_1\ {\bf p}_2 - m_2\ {\bf p}_1)/M $ | +| @#DDDDDD: range       | @#DDDDDD: $ {\bf p} \equiv (m_1\ {\bf p}_2 - m_2\ {\bf p}_1)/M $ | 
-| @#DDDDDD: $ {\bf P} \equiv {\bf p}_1 + {\bf p}_2 $ |+| @#DDDDDD: range       | @#DDDDDD: $ {\bf P} \equiv {\bf p}_1 + {\bf p}_2 $ |
  
-| @#DDDDDD: $ r \equiv |{\bf r}| $ |+| @#DDDDDD: range       | @#DDDDDD: $ r \equiv |{\bf r}| $ |
  
 ^ $ H({\bf r},{\bf R},{\bf p},{\bf R}) = \frac{1}{M}\frac{1}{2}{\bf P}^2 + \frac{1}{\mu}\frac{1}{2}{\bf p}^2 + V(r) $ ^ ^ $ H({\bf r},{\bf R},{\bf p},{\bf R}) = \frac{1}{M}\frac{1}{2}{\bf P}^2 + \frac{1}{\mu}\frac{1}{2}{\bf p}^2 + V(r) $ ^
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 == Scattering process == == Scattering process ==
-| @#DDDDDD: $ {\bf g} \equiv \frac{\partial}{\partial t}{\bf r} $ | +| @#DDDDDD: range       | @#DDDDDD: $ {\bf g} \equiv \frac{\partial}{\partial t}{\bf r} $ | 
-| @#DDDDDD: $ {\bf g}_{-\infty} \equiv \lim_{t\to-\infty}{\bf g} $ | +| @#DDDDDD: range       | @#DDDDDD: $ {\bf g}_{-\infty} \equiv \lim_{t\to-\infty}{\bf g} $ | 
-| @#DDDDDD: $ {\bf g}_{+\infty} \equiv \lim_{t\to+\infty}{\bf g} $ |+| @#DDDDDD: range       | @#DDDDDD: $ {\bf g}_{+\infty} \equiv \lim_{t\to+\infty}{\bf g} $ |
  
 Geometric considerations lead to the conclusion that there is a unit vector ${\bf \alpha}^V$, depending on the particle interaction potential $V$, with Geometric considerations lead to the conclusion that there is a unit vector ${\bf \alpha}^V$, depending on the particle interaction potential $V$, with
  
-| @#DDDDDD: $ S_{ij} \equiv \delta_{ij}-2\alpha_i^V\alpha_j^V $ |+| @#DDDDDD: range       | @#DDDDDD: $ S_{ij} \equiv \delta_{ij}-2\alpha_i^V\alpha_j^V $ |
 ^ $ {\bf g}_{+\infty} = S\ {\bf g}_{-\infty} $ ^  ^ $ {\bf g}_{+\infty} = S\ {\bf g}_{-\infty} $ ^ 
  
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 [[http://​en.wikipedia.org/​wiki/​Two-body_problem|Two-body problem]], [[http://​en.wikipedia.org/​wiki/​Rutherford_scattering|Rutherford scattering]],​ [[http://​en.wikipedia.org/​wiki/​Impact_parameter|Impact parameter]] [[http://​en.wikipedia.org/​wiki/​Two-body_problem|Two-body problem]], [[http://​en.wikipedia.org/​wiki/​Rutherford_scattering|Rutherford scattering]],​ [[http://​en.wikipedia.org/​wiki/​Impact_parameter|Impact parameter]]
  
-==== Parents ====+-----
 === Subset of === === Subset of ===
 [[Classical Hamiltonian system]] [[Classical Hamiltonian system]]
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