Testing the Standard Model of Cosmology Using BAO data - KIAS

More documents

Recommendations

Info

Changing the strategy: • Instead of looking for w(z) and exact properties of dark energy at the current status of data, we can concentrate on a more reasonable problem: Λ OR NOT Λ
wz () =−0.7 wz ( ) =−1.3 2 2 3 H ( z) = H ⎡⎡ 0 ⎣⎣Ω 0m(1 + z) +Ω DE ⎧⎧ z 1 + wz ( ') ⎫⎫ Ω DE = (1 −Ω0m)exp ⎨⎨3 ∫ dz ' ⎬⎬ 0 ⎩⎩ 1 + z ' ⎭⎭ ⎤⎤ ⎦⎦ V. Sahni, A. Shafieloo, A. Starobinsky, PRD 2008
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: Y. Gong, JCAP (2005)
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

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?