Compare · Before the Universe
Loop Quantum Big Bounce vs String-Gas Cosmology
← Back to Loop Quantum Big BouncePick a variant from Cyclic & Bouncing Cosmologies
Loop Quantum Big Bounce Speculative | String-Gas Cosmology Speculative | |
|---|---|---|
| Proposed | 2001 | 1989 |
| Key figures | Abhay Ashtekar, Martin Bojowald, Parampreet Singh | Robert Brandenberger, Cumrun Vafa |
| In one sentence | A previous contracting universe bounced, quantum geometry prevented the collapse from becoming a singularity. | String-Gas Cosmology proposes that the Big Bang was the dynamics of a gas of fundamental strings, with cosmic structure emerging from string thermodynamics. |
| Predictions |
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| Where it breaks |
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| Key unresolved problem | The out-of-reach test: the bounce in loop quantum cosmology only shows up at Planck-scale densities, energies far beyond any experiment we can imagine building, so the prediction stays untestable for now. | The missing handoff: no one has fully worked out how the hot early string-gas phase, a dense tangle of vibrating strings, gives way to the ordinary expanding universe we see, so the link to observed physics is incomplete. |
| Reader vote | 100% · 1 vote | 0% · 0 votes |
Loop Quantum Big Bounce
2001 · Speculative
String-Gas Cosmology
1989 · Speculative
Proposed
2001
1989
Key figures
Abhay Ashtekar, Martin Bojowald, Parampreet Singh
Robert Brandenberger, Cumrun Vafa
In one sentence
A previous contracting universe bounced, quantum geometry prevented the collapse from becoming a singularity.
String-Gas Cosmology proposes that the Big Bang was the dynamics of a gas of fundamental strings, with cosmic structure emerging from string thermodynamics.
Predictions
- Quantum bounce at Planck density
- Modified CMB power spectrum at large angular scales
- Pre-Bang contracting universe phase
- The number of large spatial dimensions is constrained by string dynamics (predicts three)
- Specific spectrum of cosmological perturbations from string thermodynamics
- Distinct signatures in CMB power spectrum that differ from inflation
- Relationship between primordial gravitational waves and density perturbations
Where it breaks
- Effects only at Planck scale, not currently testable
- LQG itself is incomplete
- CMB corrections sub-dominant to cosmic variance
- String theory itself has not been experimentally verified
- Specific predictions are model-dependent and not yet decisive
- The mechanism for emerging from the high-temperature string gas phase is not fully worked out
Key unresolved problem
The out-of-reach test: the bounce in loop quantum cosmology only shows up at Planck-scale densities, energies far beyond any experiment we can imagine building, so the prediction stays untestable for now.
The missing handoff: no one has fully worked out how the hot early string-gas phase, a dense tangle of vibrating strings, gives way to the ordinary expanding universe we see, so the link to observed physics is incomplete.
Reader vote
100% · 1 vote
0% · 0 votes