Testing the Standard Model of Cosmology Using BAO data - KIAS

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Universe is Flat FLRW metric Shafieloo & Clarkson, PRD 2010
Conclusion • BAO links the early and late universe. It is currently providing us with more and more valuable information about the universe. • The current standard model of cosmology seems to work fine confronting with BAO data. • This does not mean all the other models are wrong. • It is important to analyze the data in a model independent way. • Challenging the standard model is more affordable and realistic than trying to reconstruct the underlying model of the universe. • Future data will break many degeneracies and probably we can distinguish between many models. We should wait and see how long the standard model can survive.
Page 1 and 2: Testing the Standard Model of Cosmo
Page 3 and 4: Standard Model of Cosmology Vanilla
Page 5 and 6: Beyond the Standard Model of Cosmol
Page 7 and 8: Parameter estimation within a cosmo
Page 9 and 10: Dark Energy Reconstruction • Any
Page 11 and 12: Late Universe and Dark Energy Model
Page 13 and 14: Y. Gong, JCAP (2005)
Page 15 and 16: wz () =−0.7 wz ( ) =−1.3 2 2 3
Page 17 and 18: To find cosmological quantities and
Page 19 and 20: Method of Smoothing A. Shafieloo, U
Page 21 and 22: h(z) Uncorrelated estimation of the
Page 23 and 24: Model Independent Reconstruction of
Page 25 and 26: Deriving h(z) from BAO Observable E
Page 27 and 28: Deriving h(z) from BAO
Page 29 and 30: Deriving h(z) from BAO Om diagnosti
Page 31 and 32: Alcock-Paczynski Measurement • An
Page 33 and 34: Combining the information from supe
Page 35: (Present)t Standard Model of Cosmol

Testing the Standard Model of Cosmology Using BAO data - KIAS

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