Recent content by travelingscienceman

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    Modern Cosmology Dodelson Problem 6.12b (Inflation)

    Thanks for your help once again! I was able to solve it after reevaluating ##\frac{d^2 a}{dt^2}## and got ##\frac{\ddot a a-\dot a^2}{a^3}##. And yeah it's 3P, messed up typing it in.
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    Modern Cosmology Dodelson Problem 6.12b (Inflation)

    Homework Statement Show that ##4\pi G(\dot \phi)^2=\epsilon a^2 H^2## Homework Equations Over dots mean derivative with respect to ##\eta##. $$\frac{1}{a}\frac{d}{d\eta}=\frac{d}{dt}$$ $$H=\frac{\dot a}{a^2}$$ $$\epsilon=\frac{-\dot H}{aH^2}$$ $$(\frac{\dot...
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    Modern Cosmology by Dodelson: Problem 6.12 a

    Thank you both. Today with a clear head I figured it out. $$H=\frac{\dot a}{a^2}$$ And so $$\epsilon=\frac{2\dot a^2 -\ddot a a}{\dot a^2}$$ Which made things much easier.
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    Modern Cosmology by Dodelson: Problem 6.12 a

    That helps but I am still having trouble. With ##\epsilon=\frac{-\dot H}{a H^2}## I just end up going in circles. But if I work with ##\epsilon=\frac{d}{dt}\frac{1}{H}## I get the following: $$\epsilon=\frac{d}{dt}\frac{1}{H}=\frac{\dot a^2 - \ddot a a}{\dot a^2}$$...
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    Modern Cosmology by Dodelson: Problem 6.12 a

    Homework Statement The general goal of the problem is to derive some useful identities involving the slow-roll parameters during inflation. For part a show that: $$\frac {d} {d\eta} (\frac {1} {aH})= \epsilon - 1$$ Homework Equations $$\epsilon \equiv \frac {d} {dt} (\frac {1} {H})= \frac...
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    What are the Top Research Interests in Inflation and Dark Energy?

    Hello all! I have a bachelors in computing but spent a couple of years studying physics at university and I finished last spring. I decided to take a break from school to study and hopefully do some research before heading back to graduate school. My research interests are inflation and...
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