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Randall-Sundrum vs ADD Large Extra Dimensions
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Randall-Sundrum Speculative | ADD Large Extra Dimensions Speculative | |
|---|---|---|
| Proposed | 1999 | 1998 |
| Key figures | Lisa Randall, Raman Sundrum | Nima Arkani-Hamed, Savas Dimopoulos, Gia Dvali |
| In one sentence | Our universe is a 3-brane in a 5D Anti-de-Sitter bulk. The exponential warp factor explains why gravity is so weak. | The hierarchy problem is solved by allowing gravity to dilute into up to seven large extra dimensions. |
| Predictions |
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| Where it breaks |
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| Key unresolved problem | The moduli stabilization problem: nothing in the model pins down the gap between the two branes, so this distance is a free dial you set by hand rather than something the theory predicts. | The ruled-out problem: short-range gravity experiments and LHC collider searches have already excluded the simplest ADD large-extra-dimension scenarios, leaving no natural settings still standing. |
| Reader vote | No votes yet | No votes yet |
Randall-Sundrum
1999 · Speculative
ADD Large Extra Dimensions
1998 · Speculative
Proposed
1999
1998
Key figures
Lisa Randall, Raman Sundrum
Nima Arkani-Hamed, Savas Dimopoulos, Gia Dvali
In one sentence
Our universe is a 3-brane in a 5D Anti-de-Sitter bulk. The exponential warp factor explains why gravity is so weak.
The hierarchy problem is solved by allowing gravity to dilute into up to seven large extra dimensions.
Predictions
- Gravity weakens at very short distances (sub-millimeter scale)
- Kaluza-Klein graviton modes at TeV scale
- Telltale signatures at high-energy colliders like the LHC: resonance peaks where graviton modes decay into pairs of particles, or missing-energy events where gravitons escape the detector
- Deviations from Newton's law at the size of the extra dimensions
- Production of microscopic black holes at TeV colliders
- Kaluza-Klein graviton emission in scattering experiments
Where it breaks
- No KK gravitons or short-distance gravity deviations seen at LHC
- Original RS1 requires fine-tuning
- Sub-millimeter gravity tests have not seen deviations
- LHC has not produced microscopic black holes
- Simplest ADD scenarios excluded by collider searches
- Astrophysical constraints (supernova energy loss) further constrain it
Key unresolved problem
The moduli stabilization problem: nothing in the model pins down the gap between the two branes, so this distance is a free dial you set by hand rather than something the theory predicts.
The ruled-out problem: short-range gravity experiments and LHC collider searches have already excluded the simplest ADD large-extra-dimension scenarios, leaving no natural settings still standing.
Reader vote
No votes yet
No votes yet