Testing the Standard Model of Cosmology Using BAO data - KIAS

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Dark Energy Reconstruction • Any uncertainties in matter density is bound to affect the reconstructed w(z). Assumptions from the early universe can affect reconstruction of the late universe. H(z) = ' ) ( d dz ! # " d L (z) 1+ z $ * &, % + -1 ω DE = 2(1 + ( 3 H 1− ( H z) Hʹ′ ) −1 H 0 2 3 ) Ω ) 0M (1 + z Shafieloo et al, MNRAS 2006 ; Shafieloo MNRAS 2007 Quite tricky to work with
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: Parameter estimation within a cosmo
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 and 36: (Present)t Standard Model of Cosmol
Page 37 and 38: Conclusion • BAO links the early

Testing the Standard Model of Cosmology Using BAO data - KIAS

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