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Published byΕυθαλία Μανωλάς Modified over 6 years ago
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The Cosmological Constant Problem & Self-tuning Mechanism
Rong-Gen Cai Institute of Theoretical Physics Chinese Academy of Sciences
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The Cosmological Constant:
(A. Einstein, 1917) The Static Universe; “Greatest Blunder”
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The Old Cosmological Constant Problem:
Quantum Field Theory Vacuum Energy Density The Cosmological Constant QUESTION: Why ?
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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:
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The New Cosmological Constant Problem:
QUESTION: 1) why ? 2) why ? Dark Energy: Quintenssence ?
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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!
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One Needs CRAZY Ideas To Solve Those Problems Including
the Cosmological Constant Problem One Needs CRAZY Ideas (M. S. Turner)
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Brane World Scenario: RS1: RS2: N. Arkani-Hamed et al, 1998
factorizable product 2) L. Randall and R. Sundrum, 1999 warped product in AdS_5 y RS1: RS2:
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RS Brane Cosmology: where = 0 Fine-Tuning
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The Self-tuning Mechanism
The New Approach to the Cosmological Constant Problem in the Brane World Scenario The Self-tuning Mechanism
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The Case of Co-dimension one Brane
hep-th/ , hep-th/ Consider the Following Action:
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To incorporate the effects of SM quantum loops,
one may consider the effective action:
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The equations of motion:
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Consider the following 5D metric
with Poincare symmetry: And the SM matters:
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The equations of motion in the bulk:
where Consider the delta function source on the brane and Z_2 symmetry, y ---> -y:
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Key point: With the variable , the equations of motion are completely independent of the effective potential V_extremal.
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the de Sitter Symmetry and Anti-de Sitter Symmetry on the Brane
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
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Some Remarks: 1) There is a naked curvature singularity at y
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2) Finite 4D Planck Scale The zero mode tensor fluctuations correspond to a massless 4D graviton with finite Planck scale
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3) Why it works The bulk action has a shift symmetry:
results in an associated conserved current:
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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.
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* when a=2b=3/4, the action agrees with tree level
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.
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A fine tuning is still needed!
hep-th/ Here
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Consider the Case:
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One Solution with Assumption:
are integration constants. Here 1) Continuity at x_5=0 determines one of them, say, d_2.
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The Solution Does Exist for any Value of V and b.
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.
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At two singular points:
Two more boundary conditions: Here
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IF cutting off the fifth dimension by defining
The boundary conditions then reduce to:
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The Brane Contributions to
the 4D Cosmological Constant: As a result:
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FINE TUNING
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The Case of Co-dimension two Brane
hep-th/ , hep-th/ hep-th/ , hep-th/ Consider and action
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The Maxwell Field Has the Solution
The Einstein’s Equations: The Stress-Energy Tensor:
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Here A Static and Stable Solution is provided
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Now Add Brane to the System
with The Stress-Energy Tensor of Branes:
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Rewrite the metric of two-dim. sphere
Two branes at r=0 and r= infinity. obeys the following equation:
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This equation has the solution
where
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By a coordinate transformation, the solution becomes
where and This solution describes two-sphere, but a wedge is removed and opposite sides are identified.
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The geometry of extra two-dimensions
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Finally with The brane is always flat for any tension.
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THANK YOU
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