Testing the Standard Model of Cosmology Using BAO data - KIAS

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C. Blake et. al, in prepration
(Present)t Standard Model of Cosmology Universe is Flat Universe is Isotropic Universe is Homogeneous (large scales) Dark Energy is Lambda (w=-1) Power-Law primordial spectrum (n_s=const) Dark Matter is cold All within framework of FLRW
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: Combining the information from supe
Page 37 and 38: Conclusion • BAO links the early

Testing the Standard Model of Cosmology Using BAO data - KIAS

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