Recent content by StuckPhysicsStudent

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    Dodelson Cosmology 4.8 Temperature of Nonrelativistic Matter

    Well, it must depend on time since it is dependent on a. I am unsure exactly how it would depend on space, but regardless if I assume T does depend on both I get $$\frac{\partial f_{dm}}{\partial t}=-\frac{\dot{E}T-\dot{T}E}{T^2}e^{-E/T}$$ $$\frac{\partial f_{dm}}{\partial...
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    Dodelson Cosmology 4.8 Temperature of Nonrelativistic Matter

    Homework Statement Show that the temperature of non-relativistic matter scales as ##a^{-2}## in the absence of interactions. Start from the zero-order part of Eq. (4.68) and assume a form ##f_{dm} \propto e^{-E/T}=e^{-p^2/2mT}##. Note that his argument does not apply to electrons and protons...
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    How Can a Physics Student Master Advanced Theories Like Cosmology and QFT?

    Hey all. The title/name says it all. I am trying my best to improve my knowledge of Cosmology, GR, QFT, Statistical Field theory, and learn a bit about string theory. I have browsed through the site before and will be trying to soak up as much knowledge as possible.
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    Dodelson Cosmology 6.8 Inflation Klein Gordon Equation

    Homework Statement Show that Eq. (6.33) follows from Eq. (6.32) by changing variables from t to ##\eta##. Homework Equations (6.32) $$\frac{d^2\phi^{(0)}}{dt^2}+3H\frac{d\phi^{(0)}}{dt}+V'=0$$ (6.33) $$\ddot{\phi^{(0)}}+2aH\dot{\phi}^{(0)}+a^2V'=0$$ The Attempt at a Solution So...
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