The Cosmological Constant Problem & Self-tuning Mechanism
Rong-Gen Cai
Institute of Theoretical Physics Chinese Academy of Sciences
The Cosmological Constant:
18
2R g R g GT
(A. Einstein, 1917)
The Static Universe; “Greatest Blunder”
The Old Cosmological Constant Problem:
Quantum Field Theory Vacuum Energy Density The Cosmological Constant
4 3 4~ ( ) ~ (10 )SUSYE Gev
QUESTION: Why ?0
4 19 4~ ( ) ~ (10 )QGE Gev
近年的天文观测支持 : 暴涨模型⊕暗物质 ⊕ 暗能量 22% 73% ⊕ 挑战 : 暴涨模型 ? 暗物质 ? 暗能量 ?
Inflation Model: A. Guth, 1981
Dark Matter:
Dark Energy:
0 /p 1 1/ 3
The New Cosmological Constant Problem:
3 4 29 3~ ~ (10 ) ~ 10 /ev g cm
QUESTION: 1) why ? 2) why ?
0
~
Dark Energy: Quintenssence ?
IF THE COSMOLOGICAL CONSTANT EXISTS:
Cosmological Event Horizon: Entropy: Finite Degrees of Freedom: Consistent With String Theory?
T. Banks, 2000: The Cosmological Constant is an Input of the Fundamental Theory!
To Solve Those Problems Including
the Cosmological Constant Problem
One Needs CRAZY Ideas
(M. S. Turner)
Brane World Scenario:
y
X 1) N. Arkani-Hamed et al, 1998 factorizable product
2) L. Randall and R. Sundrum, 1999 warped product in AdS_5
4 x nM T
14 2
4
x S /
x R
M Z
M
RS1:
RS2:
RS Brane Cosmology:
2 242 3 44 5
8 4( ) ( )
3 3 3H
M M a
where
24 53 3
5 5
25
4 5
4 4( )
3
3( )
4
M M
MM M
= 0
Fine-Tuning
The New Approach to the Cosmological Constant Problem in the Brane World Scenario
The Self-tuning Mechanism
The Case of Co-dimension one Brane
hep-th/0001197, hep-th/0001206
Consider the Following Action:
To incorporate the effects of SM quantum loops, one may consider the effective action:
The equations of motion:
Consider the following 5D metric with Poincare symmetry:
And the SM matters:
The equations of motion in the bulk:
where
Consider the delta function source on the brane and Z_2 symmetry, y ---> -y:
Key point: With the variable , the equations of motion are completely independent of the effective potential V_extremal.
Recalling the conformal coupling
It Pohibits both the de Sitter Symmetry and Anti-de Sitter Symmetry on the Brane
The Flat Domain Wall Solution is the Unique One, for any Value of the Brane Tension
Some Remarks:
1) There is a naked curvature singularity at
y
sysy
2 ( )a y
2) Finite 4D Planck Scale
The zero mode tensor fluctuations correspond to a massless 4D graviton with finite Planck scale
3) Why it works
The bulk action has a shift symmetry:
0 results in an associated conserved current:
However, the coupling to the brane tension breaks this symmetry.
The SM vacuum energy is converted into a current emerging on the brane and ending in the singularity region.
More general coupling to the brane tension:
with
* when a=2b=3/4, the action agrees with tree level string theory with phi as the dilaton.
A fine tuning is still needed!
hep-th/0002164
Here
Consider the Case: 0
One Solution with Assumption:
' '/ 3a 5 50, 0x x
,i ic dHere are integration constants.
1) Continuity at x_5=0 determines one of them, say, d_2.
2) The condition on the first derivatives at x_5=0 determines c_1 and c_2:
The Solution Does Exist for any Value of V and b.
At two singular points:
2 13 / 4, 3 / 4x c x c
Two more boundary conditions:
Here 1/ 3
IF cutting off the fifth dimension by defining
The boundary conditions then reduce to:
The Brane Contributions to the 4D Cosmological Constant:
As a result:
FINE TUNING
The Case of Co-dimension two Brane
hep-th/0302067, hep-th/0302129hep-th/0309042, hep-th/0309050
Consider
and action
The Maxwell Field Has the Solution
The Einstein’s Equations:
The Stress-Energy Tensor:
Here
A Static and Stable Solution is
provided
Now Add Brane to the System
with
The Stress-Energy Tensor of Branes:
Rewrite the metric of two-dim. sphere
Two branes at r=0 and r= infinity.
obeys the following equation:
This equation has the solution
where
This solution describes two-sphere, but a wedge is removed and opposite sides are identified.
By a coordinate transformation, the solution becomes
where
and
The geometry of extra two-dimensions
Finally
with
The brane is always flat for any tension.
THANK YOU