Slide 1 Models of Our Universe: The Friedman Equation By Ashleigh Miller November 4, 2014 Southern Methodist University Dr. Cooley’s 3305 Modern Physics Class 1Modern Physics…
Slide 1Dark energy and the CMB Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto Slide 2 Why use…
Slide 1 1 Discovering New Physics with the LHC Nadia Davidson Supervisor: Elisabetta Barberio EPP Nobel Prize for Physics in 2010: Slide 2 2 Slide 3 3 The current model of…
The Cosmological Principle Viewed on sufficiently large distance scales, there are no preferred directions or preferred places in the Universe. Consequences of the Cosmological…
Making the most of the ISW effect Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto Outline What…
Dark energy and the CMB Robert Crittenden Work with S. Boughn, T. Giannantonio, L. Pogosian, N. Turok, R. Nichol, P.S. Corasaniti, C. Stephan-Otto Why use the CMB to study…