美文网首页
关于光子的 Doppler Shift

关于光子的 Doppler Shift

作者: optic_css | 来源:发表于2019-01-07 23:52 被阅读0次

    A breif introduction to the RDS

    __with some subtle method

      Let's assume that there are two frames (G1, G2, they respect the observer and the light source respectively) related with the velocity u, ie. Frame G1 is moving with the velocity V to frame G2.  All below is at G2's view.

    The relativistic particle m_{0} with the velocity as \vec{V}  [ v(x), v(y), v(z) ] respect to frame G1 thus have energy of relativisty as

    E_{r}= \frac{E_{r0}}{\sqrt{1-(\frac{v}{c} )^2} } ,

        from the Lorenz transform of the velocity,  the particle have

    v_{r} (i)= \frac{v(i) }{\sqrt{1-\frac{uv} {c^2}}},

        hence V_{r}=\sqrt{\sum_{i=x,y,z}v_{r }^2(i)}, substitude the Lorenz transform into V_{r}.

    1-(\frac{v_{r}}{c})^2=\frac{[1-(\frac{u}{c})^2][1-(\frac{v}{c})^2]}{1-\frac{uv}{c^2} } ,

        The energy (of course, the gross one),

    E_{r}= \frac{1-\frac{uv}{c^2}}{\sqrt{1-(\frac{u}{c})^2}} = \gamma E(1-\frac{uv}{c^2}).

        The reason to do this with out any restrict to v and v_r, is to let it fit all the particles, but not only for photon.

        from the quantum mechanics, the energy of photon is E=h\nu ,  besides the velocity of light is v=v_{r}=c (of course for all the frames).

        Hence,

    \nu _r=\gamma\nu  (1-\frac{uv}{c^2} ),

        When the dimentions go up to 3, have that

    \nu _r=\gamma\nu  (1-\frac{u cos\theta }{c} ).

        The equation above is what is called the "Relativistic Doppler Shift".

        You can form your own figure like below from this equation, and it is widely used in cosmo_......

    doppler shift.

        Referance: "Baidu.baike" , "Wikipedia_Relativity Theory".

    相关文章

      网友评论

          本文标题:关于光子的 Doppler Shift

          本文链接:https://www.haomeiwen.com/subject/jihurqtx.html