Compare · Before the Universe
String-Gas Cosmology vs Loop Quantum Big Bounce
← Back to String-Gas CosmologyCyclic & Bouncing Cosmologies· within family
String-Gas Cosmology Speculative | Loop Quantum Big Bounce Speculative | |
|---|---|---|
| Proposed | 1989 | 2001 |
| Key figures | Robert Brandenberger, Cumrun Vafa | Abhay Ashtekar, Martin Bojowald, Parampreet Singh |
| In one sentence | String-Gas Cosmology proposes that the Big Bang was the dynamics of a gas of fundamental strings, with cosmic structure emerging from string thermodynamics. | A previous contracting universe bounced, quantum geometry prevented the collapse from becoming a singularity. |
| Predictions |
|
|
| Where it breaks |
|
|
| Key unresolved problem | 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. | 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. |
| Reader vote | 0% · 0 votes | 100% · 1 vote |
String-Gas Cosmology
1989 · Speculative
Loop Quantum Big Bounce
2001 · Speculative
Proposed
1989
2001
Key figures
Robert Brandenberger, Cumrun Vafa
Abhay Ashtekar, Martin Bojowald, Parampreet Singh
In one sentence
String-Gas Cosmology proposes that the Big Bang was the dynamics of a gas of fundamental strings, with cosmic structure emerging from string thermodynamics.
A previous contracting universe bounced, quantum geometry prevented the collapse from becoming a singularity.
Predictions
- 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
- Quantum bounce at Planck density
- Modified CMB power spectrum at large angular scales
- Pre-Bang contracting universe phase
Where it breaks
- 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
- Effects only at Planck scale, not currently testable
- LQG itself is incomplete
- CMB corrections sub-dominant to cosmic variance
Key unresolved problem
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.
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.
Reader vote
0% · 0 votes
100% · 1 vote