Recent content by needved

  1. needved

    Graduate Eikonal approximation path integral solution in gravitational lensing

    Please, help here people. Im reading this article Wave Optics in Gravitational Lensing (T. T. Nakamura, 1999) . In the article start work with \begin{equation} (\nabla ^2 +\omega)\tilde\phi = 4\omega^2U\tilde\phi \end{equation} where $$\tilde\phi = F(\vec r)\tilde\phi_{0}(r)$$. Using...
  2. needved

    Finding Fourier coefficients for e^t

    Homework Statement i have this function \begin{equation} f(t) = e^t \end{equation} Homework Equations [/B] the Fourier seria have the form \begin{equation} f(t) = \sum C_{n} e^{int} \end{equation}The Attempt at a Solution } [/B] so i need to find the coeficients $c_{n}$ given by...
  3. needved

    Undergrad Why are spatial components equal to h_00 in weak field metric?

    In Schutz says When we have weak gravitaional fields then the line element *ds* is $$ ds^{2}=-(1+2\phi)dt^{2}+(1-2\phi)(dx^{2}+dy^{2}+dz^{2}) $$ so the metric is $$ {g_{\alpha\beta}} =\eta_{\alpha\beta}+h_{\alpha\beta}= \left( \begin{array}{cccc} -(1+2\phi) & 0 & 0 & 0\\ 0 & (1-2\phi) & 0 &...
  4. needved

    Undergrad Physical meaning of distance in retarded solutions to linearized Einstein equations

    Hi people, help here please When the Einstein equation are linearized the results are the weak field Einstein equations $$ \left ( -\frac{\partial^{2}}{\partial t^{2}} + \nabla^{2} \right ) \bar h^{\mu\nu}=-16\pi T^{\mu\nu} $$ a solution for this equations considering the source are the...
  5. needved

    High School Recovering length units in Schwarzschild geometry with c = G = 1

    Hi people :) I'm learning some of General Relativity topics but still I am a beginer, uh! i use the Schutz "A first course of general relativity", but i a little confused about the units, the author say it use c = G = 1 all around the book. Just right now i reading chapter 11: Schwarchild...