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Wayne Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy
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Page 1: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

Wayne Hu

Page 2: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

Page 3: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

(10120+1)-10120

(10120+2)-10120

Dystopian Future:Theory

Page 4: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

2016

2017

Dystopian Future:Observations

Page 5: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

Wayne Hu

Page 6: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Wayne HuChicago, January 2016

The Future of Cosmological Physics:Dark Energy

Wayne Hu

Goldstone Boson of SpontaneouslyBroken Time TranslationSymmetry

Page 7: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Accelerated Expansion

Page 8: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Accelerating Expansion: Distance-Redshift• Photons travel on null geodesics in the FRW spacetime

• D quantifies light travel time, whereas scale factor a=1/(1+z) quantifies the expansion or size of universe

Accelerating Expansion: Distance-RedshiftPhotons travel on null geodesics in the FRW spacetime

quantifies light travel time, whereas scale factor=1/(1+z) quantifies the expansion or size of universe

D =

∫dt

a=

∫da

aH=

∫dz

H

inferringdistance:standardcandles&rulers

Page 9: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Accelerating Expansion: Distance-Redshift• SNIa as standard candle: relative distance from high to low z• High z SNIa dimmer than expected, H more constant than expected in decelerating universe Riess et al (1998); Perlmutter et al (1998)

• Sound horizon as standard ruler: angular size in CMB islarger than expected in an open universe Boomerang, Maxima, DASI

Accelerating Expansion: Distance-Redshiftas standard candle: relative distance from high

SNIa dimmer than expected,SNIa dimmer than expected,SNIa dimmer H more constant expected in decelerating universe Riess et al (1998); Perlmutter et al (1998)

Sound horizon as standard ruler: angular size in than expected in an open universe Boomerang, Maxima, DASI

Page 10: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Accelerating Expansion: Distance-Redshift• Cosmological constant: energy density remains constant as Universe expands• Friedmann equation: H goes to a constant, spacetime approaches deSitter

Accelerating Expansion: Distance-RedshiftCosmological constant: energy density remains constant

Universe expandsFriedmann equation: H goes to a constant, spacetime

approaches deSitterH2 = 8πGρ/3

Page 11: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Simple ≠ Natural• Simplest possibility, consistent with all data to date, is a constant: Einstein’s Cosmological Constant• Particle physics provides sources for such a constant

• But the energy scales associated with particle physics scale cutoffs and transitions give energy densities (ρ ~ E4) at least ~60 orders of magnitude too large• For a bare CC to cancel these contributions would seem to require exquisite fine tuning

graviton

Zero Point Energy Phase Transitions

Page 12: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Coincidence• Coincidence problem: matter/radiation dilutes with expansion dark energy constant or slowly diluting only comparable today

-20 0 20

0

0.5

1

NowWE NBBPlanck

log(a)

Carroll (2001)

Page 13: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Distance-Redshift• [CMB-] BAO-SN and the inverse distance ladder

eBOSS Collab (2015)

%levelprecision

Page 14: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Sound Horizon• Standard ruler D(z*): sound horizon at recombination z* calibrated through measuring the ordinary matter content• In flat ΛCDM, angular size measures only remaining density, Λ

Planck 2013

sound horizon calibrated[baryon/photon, matter/radiation]

Page 15: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Checking for Cracks• Standard ruler D(z*): sound horizon at recombination z*

• Diffusion scale provides consistency check on sound horizon cali- bration: new physics at recombination, while BAO on acceleration

Planck 2013

consistency check

ü?

Page 16: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Falsifying ΛCDM• CMB determination of matter density controls all determinations

in the deceleration (matter dominated) epoch

• Planck: Ωmh2 = 0.1426± 0.0025→ 1.7%

• Distance to recombination D∗ determined to 141.7% ≈ 0.43%

(ΛCDM result 0.46%; ∆h/h ≈ −∆Ωmh2/Ωmh

2)[more general: −0.11∆w − 0.48∆ lnh− 0.15∆ ln Ωm − 1.4∆ ln Ωtot = 0 ]

• Expansion rate during any redshift in the deceleration epochdetermined to 1

21.7%

• Distance to any redshift in the deceleration epoch determined as

D(z) = D∗ −∫ z∗

z

dz

H(z)

• Volumes determined by a combination dV = D2AdΩdz/H(z)

• Structure also determined by growth of fluctuations from z∗

Page 17: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Value of Local Measurements• With high redshifts fixed, the largest deviations from the dark

energy appear at low redshift z ∼ 0

• By the Friedmann equation H2 ∝ ρ and difference between H(z)

extrapolated from the CMB H0 = 38 and 67 is entirely due to thedark energy density in a flat universe

• With the dark energy density fixed by H0, the deviation from theCMB observed D∗ from the ΛCDM prediction measures theequation of state (or evolution of the dark energy density)

pDE = wρDE

• Likewise current amplitude of structure, e.g. local clusterabundance, tests the smooth dark energy paradigm

Page 18: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

H0 is for Hints• Actual distance ladder measurements prefer larger value

Planck XVI

Page 19: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Dark Energy & H0

• •

Change the dark energy, change CMB inference for H0

But simultaneously change expansion rate at intermediate z

fr

actio

nal c

hang

e

z0.01

-0.1

0

0.1

-0.05

0.05

0.1 1 10

∆lnH74

67

∆w=-0.23

Page 20: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Local BAO • Locally DA = ∆z/H0, and the observed power spectrum is isotropic in h Mpc-1 space• Template matching the features yields the Hubble constant

Eisenstein, Hu & Tegmark (1998)k (Mpc–1)

0.05

2

4

6

8

0.1

Pow

er

h

Observedh Mpc-1

CMB provided

Page 21: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Cosmological Distances• Modes perpendicular to line of sight measure angular diameter distance

k (Mpc–1)0.05

2

4

6

8

0.1

Pow

er

Observedl DA-1

CMB provided

DA

Page 22: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Distance-Redshift• BAO-SN and the inverse distance ladder

eBOSS Collab (2015)

Page 23: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Cosmological Distances• Modes parallel to line of sight measure the Hubble parameter

k (Mpc–1)0.05

2

4

6

8

0.1

Pow

er

ObservedH/∆z

CMB provided

H

Page 24: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Acoustic Rings• Baryon oscillations appear as rings in a 2D power spectrum with modes parallel and perpedicular to the line of sight

0.02

0.02

0.04

0.06

0.08

0.10

0.12

0.14

0.04 0.06 0.08 0.10 0.12 0.14k⊥ (Mpc-1)

k (

Mpc

-1)

k⊥ (Mpc-1)

k (

Mpc

-1)

~10% peak to trough

Page 25: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Dark Energy• Predicts larger BAO (θ) angular and radial (z) scale; larger SN=H0DA relative luminosity distance; larger linear growth

frac

tiona

l cha

nge

z0.01

-0.1

0

0.1

-0.05

0.05

0.1 1 10

∆lnH∆lnBAOθ

∆ln(SN)

∆lnGrow∆lnBAOz

tensionwith data!

∆w=-0.23

Page 26: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Growth of Structure

Page 27: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Smooth Dark Energy and Sound Speed• Only cosmological constant is spatially smooth in all frames• Dark energy can be smooth relative to the dark matter if relativistic stresses support it against collapse• On scales below the sound horizon (Jeans scale), expansion history determines growth of structure: consistency relations

Tim

e

Space

ConstantDark Energy

dense

Newtonian

Page 28: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

• Peculiar velocities enhance parallel power and hence cause an anisotropy in the power spectrum which measures growth rate

Redshift Space Distortion

0.02

0.02

0.04

0.06

0.08

0.10

0.12

0.14

0.04 0.06 0.08 0.10 0.12 0.14k⊥ (Mpc-1)

k (

Mpc

-1)

Page 29: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Redshift Space Distortions• Redshift space distortions and the growth of structure

eBOSS Collab (2015)

Page 30: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

0.

700.

750.

800.

850.

900.

95

8(M/0

.27)

0.3

WL*

X-rays*

MaxBCG*

ACT

SPT Planck SZ

Planck prediction

Clusters CMBLSS

Growth and Clusters• Cluster abundance measurements vs Planck predictions

• Statistically discrepant at the ~3σ level

Planck 2013

Page 31: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Cluster Abundance• Cluster abundance, growth of structure, and the mass- observable scaling relation

Planck Collab (2015)

Page 32: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Halos and Shear

Page 33: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Cosmic Shear• Cosmic shear in DES galaxy ellipticities and CMB

Kirk et al (2015)

Page 34: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Current Status: Local Cracks• Tension between Planck high-z cosmology at local tests

Expansion rate (Hubble constant, not BAO) Growth (cluster abundance, cosmic shear, redshift space distortions)

New cosmological or astro physics? • In era of 1% precise cosmology, multiple probes and blind analyses required to assure 1% accuracy

• If new physics, a complex dark sector is required to break consistency between growth, distance and standards

• KICP is uniquely placed to resolve these observationally or theoretically

Page 35: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Beyond Smooth Dark Energy

Page 36: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Mercury or Pluto?General relativity says Gravity = Geometry

And Geometry = Matter-Energy

Could the missing energy required by acceleration be an incomplete description of how matter determines geometry?

Page 37: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Dynamical vs Lensing Mass• Newtonian potential: Ψ=δg00/2g00 which non-relativistic particles feel

• Space curvature: Φ=δgii/2gii which also deflects photons

• Most of the incisive tests of gravity reduce to testing the space curvature per unit dynamical mass

Page 38: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Dynamical vs Lensing Mass• Newtonian potential: Ψ=δg00/2g00 which non-relativistic particles feel

• Space curvature: Φ=δgii/2gii which also deflects photons

• But unlike the solar system, dark energy stress-energy unknown

Page 39: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Dark Energy as a Scalar Field• Dark energy picks out a preferred time slicing or foliation where spatial translational invariance unbroken • Symmetry limits the form of interactions and coupling with tensor gravity [EFT as organizing principle]• T=t+π(t,x) in a general slicing, introducing a (Stuckelberg) scalar

Space

ConstantDark Energy

Fielddense

T=const.

t=const.

π

Page 40: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Perturbative Subhorizon Regime• When dark energy field nonlinearity can be ignored: Most general scalar-tensor theory [Horndeski++] and/or Effective field theory leads to Theory with 4 free functions of time • Specifying perturbative “post Friedmann” phenomenology: Space curvature per unit dynamical mass (aka slip, dark energy anisotropic stress) Effective Newton constant G relating potentials to density fluctuations Tensor gravitational wave propagation speed and damping

• Linearization must break down: gravity well tested locally• Nonlinear interactions lead to screening mechanism

Page 41: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Perturbative Subhorizon Regime• When dark energy field nonlinearity can be ignored: Most general scalar-tensor theory [Horndeski++] and/or Effective field theory

leads to Theory with 4 free functions of time • Specifying perturbative “post Friedmann” phenomenology: Space curvature per unit dynamical mass (aka slip, dark energy anisotropic stress) Effective Newton constant G relating potentials to density fluctuations Tensor gravitational wave propagation speed and damping

• Linear instabilities: ghost (wrong sign kinetic terms, negative energy states) gradient instability (imaginary sound speed)

perturbative “post Friedmann” phenomenology: unit dynamical mass (aka slip,

dark energy anisotropic stress)G relating potentials to

propagation speed and damping

Page 42: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Perturbative Subhorizon Regime• When dark energy field nonlinearity can be ignored: Most general scalar-tensor theory [Horndeski++] and/or Effective field theory

leads to Theory with 4 free functions of time • Specifying perturbative “post Friedmann” phenomenology: Space curvature per unit dynamical mass (aka slip, dark energy anisotropic stress) Effective Newton constant G relating potentials to density fluctuations Tensor gravitational wave propagation speed and damping

• Linear instabilities: ghost (wrong sign kinetic terms, negative energy states) gradient instability (imaginary sound speed)

perturbative “post Friedmann” phenomenology: unit dynamical mass (aka slip,

dark energy anisotropic stress) Newton constant G relating potentials to

propagation speed and damping

Page 43: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Perturbative Subhorizon Regime• When dark energy field nonlinearity can be ignored: Most general scalar-tensor theory [Horndeski++] and/or Effective field theory leads to Theory with 4 free functions of time • Specifying perturbative “post Friedmann” phenomenology: Space curvature per unit dynamical mass (aka slip, dark energy anisotropic stress) Effective Newton constant G relating potentials to density fluctuations Tensor gravitational wave propagation speed and damping

• Linearization must break down: gravity well tested locally• Nonlinear interactions lead to screening mechanism

Page 44: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Nonlinear Screening Mechanisms• Scalar degree of freedom φ [where previously T(φ)] introduces changes to the Poisson equation(s)

• Where φ depends nonlinearly on matter sources

• Nonlinearity in Field: chameleon/symmetron Field gradients: kinetic screening Field second derivatives: Vainshtein/galileon• No superposition principle: structure must be simulated numerically with N-body simulations

∇2(Φ − Ψ)/2 = −4πGa2∆ρ

∇2Ψ = 4πGa2∆ρ − 1

2∇2φ

∇2φ = glin(a)a2 (8πG∆ρ − N [φ])

Page 45: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Hu, Huterer & Smith (2006)

Environment Dependent ForceFor large background field, gradients in the scalar prevent the

chameleon from appearing

Oyaizu, Lima, Hu (2008)

Page 46: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Common Building Blocks• Example: Vainshtein Mechanism & Galileon Symmetry

Bigr

avity Massive

Gravity

DGPBraneworld

Horndeski

Beyond Horndeski

CovariantGalileon

Vainshtein MechanismGalileon

Decoupling Limit

GLPV

Spatially CovariantGravity

f(R)

fab4

Fierz-Pauli

dRGT

Page 47: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Parameterizing the Future• General scalar-tensor and EFT akin parameterizes our current ignorance leaving future observations to guide us• Not a procedure to solve Original Λ problem: fine tuning of vacuum energy New Λ problem: why this finite value, why now Not fully general: additional modes, dimensions• Toward compelling alternative to Λ: Provide building blocks assembled into toy models Eliminate what cannot work • Dark energy theory is a boom, bust field always looking for next interesting idea• Case study: massive gravity++ Pros: degravitation, self-acceleration, Vainshtein mechanism, galileon non-renormalization, T from second metric Cons: instabilities, strong coupling, Cauchy breakdown...

Page 48: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Massive Multiverse

de Rham (2015)

Page 49: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Massive Multiverse

de Rham (2015)

Motloch et al (2015, 2016)

0 Π2

Π

0

Π2

Π

Χ

Η

Page 50: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

The Future of Cosmological Physics:Dark Energy

DESILSST

CMBS4WFIRST

EUCLID

DESLIGO

HETDEX

eBOSS

HSCSPT3G

GA

IALIGOLIGOLIGOLIGO

Page 51: The Future of Cosmological Physics: Dark Energy Hu Chicago, January 2016 The Future of Cosmological Physics: Dark Energy (10120+1)-10120 (10120+2)-10120 Dystopian Future: Theory

Stay Tuned... Josh FriemanMarch 2016

The Future of Cosmological Physics:Dark Energy

DESILSST

CMBS4WFIRST

EUCLID

DESLIGO

HETDEX

eBOSS

HSCSPT3G

GA

IALIGOLIGOLIGOLIGO


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