The polarisation vectors of particles of arbitrary spin j are typically defined selecting a standard "representative" momentum p⋆ and then boosting into a general frame. A simple example is the case of spin j=1/2 massive particles, where p_\star=m(1,\boldsymbol 0), and u(p_\star)=\sqrt{2m}\begin{pmatrix}1\\0\\1\\0\end{pmatrix}
One can show that the boosted polarisation vector u(p)=L(\Lambda)u(p_\star) is given by u(p)=\begin{pmatrix}\sqrt{p\cdot\sigma\vphantom{\int}}\begin{pmatrix}1\\0\end{pmatrix}\\ \sqrt{p\cdot\bar\sigma\vphantom{\int}}\begin{pmatrix}1\\0\end{pmatrix} \end{pmatrix} and a similar expression for the s=-1/2 case.
In the case of spin j=1 massive particle, I've never seen any explicit expression for \varepsilon^\mu(p), not even a formal one (besides \varepsilon^\mu(p)=\Lambda \varepsilon^\mu(p_\star)). I expect that there should exist an expression similar to the j=1/2 case because, for one thing, \varepsilon^\mu\sim u^\dagger\sigma^\mu u (in a formal sense; more precisely, \frac12\otimes\frac12=1 in the sense of representations of the Lorentz group). My question is : what is the explicit form of \varepsilon^\mu for arbitrary p^\mu? I'm pretty sure that the result is well-known and can be found in many books, but I have failed to find it, so here I am.
For definiteness, let us consider p_\star=m(1,\boldsymbol 0) and \begin{equation} \varepsilon_+(p_\star)=\frac{1}{\sqrt{2}}\begin{pmatrix}0\\+1\\-i\\0\end{pmatrix}\qquad\quad \varepsilon_0(p_\star)=\begin{pmatrix}0\\0\\0\\1\end{pmatrix}\qquad\quad \varepsilon_-(p_\star)=\frac{1}{\sqrt{2}}\begin{pmatrix}0\\+1\\+i\\0\end{pmatrix} \end{equation} and the standard boost is chosen such that \Lambda p_\star=p.
Question: what is \varepsilon_\pm(p),\varepsilon_0(p)? Thanks in advance!
Answer
D\vphantom{asd}ear OP,
I hope you are doing ok. As usual, Weinberg's got you covered. See in particular equation 2.5.24: the standard boost that takes you from p_\star to p is \begin{equation} \begin{aligned} L^i{}_k&=\delta^i_k+(\gamma-1)\hat p_i\hat p_k\\ L^i{}_0&=\hat p_i\sqrt{\gamma^2-1}\\ L^0{}_0&=\gamma \end{aligned} \end{equation} where \hat p_i=p_i/|\boldsymbol p| and \gamma=\sqrt{1+\boldsymbol p^2/m^2}. This matrix satisfies \begin{equation} A(p)=LA(p_\star) \end{equation} for any vector A, such as p itself or the polarisation vectors \varepsilon_\sigma. I guess you can take it from here.
Sincerely, OP.
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