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Ignacy Sawicki Université de Genève Understanding Dark Energy.

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Presentation on theme: "Ignacy Sawicki Université de Genève Understanding Dark Energy."— Presentation transcript:

1 Ignacy Sawicki Université de Genève Understanding Dark Energy

2 Making Sense of the Sky 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Image credit: NASA and ESA

3 Making Sense of the Sky 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Redshift

4 Ordering by redshift 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Image credit: Ivo Labbé

5 Use Standard Candles to Map 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

6 Use Standard Candles to Map 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

7 First Attempt at Model  Copernican Principle: here is not special Universe grossly homogeneous and isotropic  Gravity is General Relativity  Matter non-relativistic 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

8 First Attempt at Model: FAIL 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick From D. Huterer Dimmer

9 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick (stars 0.4%, gas 4.6%) Planck 2015

10 Is the Universe fooling us? 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

11 Is the Universe fooling us? 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Acceleration detected at 64σ

12 But is it actually Λ? 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Alternatives to Λ must be dynamical: search for time- and scale-dependence

13 ΛCDM as Null Hypothesis 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Planck 2015 Background close to ΛCDM

14 CMB is Gravitational Collapse 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick gravitational collapse Initial conditions (inflation) Galaxy formation Vacuum in quasi-de Sitter (nearly) scale invariant Gaussian fluctuations Planck 2015

15 Dark Energy Changes Growth 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick ΛCDM Dynamic al DE Snowmass Report 1309:5385

16 Use Structure to Probe Gravity/DE 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick SDSS/BOSS SDSS/BOSS DR10

17 Redshift-Space Distortions 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Real space Redshift space Samushia et al. (2013)/BOSS Kaiser (1985)

18 Redshift-Space Distortions  Galaxy velocities tend to be lower than ΛCDM would imply 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Ruiz & Huterer (2014)

19 Weak Lensing 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

20 Is everything OK with ΛCDM? 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Weak Lensing (CFHTLeNS, Heymans 2012) + Distances Clusters (Planck 2013) CMB (Planck 2013) + Distances Probability Density

21 CMB Lensing: Smooths Peaks 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Planck: Ade et al. (2015)

22 The Takeaway  Dark energy is not going away  ΛCDM fits, but maybe first tensions are beginning to appear Power seems to be lacking in many probes of growth  It could well end up being other physics Massive neutrinos can have similar physics  Caveat emptor: All cosmological probes sensitive only to gravity; cannot say anything direct about composition 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

23 Watch this Space! 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Credit: D. Huterer

24 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick THANK YOU!

25 w is not an observable 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick Kunz (2007)

26 Scale-Dependent Growth Rate 18 September 2015 XXXV Physics in Collisions 2015, University of Warwick

27 BAO : SDSS vs Euclid Distance-redshift relation moves P(k) EUCLID expected SDSS today 0.7<z<2.0 0.15<z<0.5

28 Measuring shear in next generation wide field cosmic shear surveys


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