Does BICEP2's observation rules out ekpyrotic cosmological model ?

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Discussion Overview

The discussion centers around the implications of the BICEP2 observation, specifically regarding its potential to rule out the ekpyrotic cosmological model (ECM) and its effects on string inflation models (SIM). Participants explore the significance of the observed parameters r and n_t in the context of these cosmological theories.

Discussion Character

  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants assert that the observation of n_t=0 definitively excludes the ekpyrotic cosmological model, which predicts n_t=2.
  • Others argue that the observed r=0.2 challenges many current string inflation models, such as KKLMMT, due to the requirement for a significant variation in the inflaton field.
  • A later reply references a paper that claims the BICEP2 data supports a scale-invariant primordial gravitational wave spectrum, suggesting that the ECM is ruled out at more than 5σ significance.
  • Another participant mentions a comment from Turok, indicating that while the ECM may be refuted, newer bouncing universe models based on the Higgs field could still be viable.

Areas of Agreement / Disagreement

Participants express differing views on the implications of the BICEP2 observations, with some asserting that it rules out certain models while others suggest that alternative models may still hold validity. The discussion remains unresolved regarding the broader implications for cosmological models.

Contextual Notes

There are limitations in the discussion regarding the assumptions underlying the interpretations of the BICEP2 data, as well as the dependence on specific definitions of the models in question. The mathematical steps leading to these conclusions are not fully resolved.

sufive
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Dear every specialists, I heard that BICEP2's observation r=A_t/A_s=0.2 n_t=0 indicate two things:

1) n_t=0 excludes ekpyrotic cosmological model (ECM) definitely because ECM predicts n_t=2

2) r=0.2 excludes almost all current string inflation model (SIM) such as KKLMMT because this observation requires inflaton field vary at leasts 10Mp while SIM do not allows such big range varyings

Who can tell me more about this two point of view
 
Physics news on Phys.org
http://arxiv.org/abs/1403.5463
The Tilt of Primordial Gravitational Waves Spectra from BICEP2
Cheng Cheng, Qing-Guo Huang
(Submitted on 21 Mar 2014)
In this paper we constrain the tilt of the spectra of primordial gravitational waves from Background Imaging of Cosmic Extragalactic Polarization (BICEP2) data only. We find r=0.21+0.04−0.10 and nt=−0.06+0.25−0.23 (at 68% C.L.) which implies that a scale-invariant primordial gravitational waves spectra is consistent with BICEP2 nicely. Our results provide strong evidence for supporting inflation model, and the alternative models, for example the ekpyrotic model which predicts n_t=2, are ruled out at more than 5σ significance.
Comments: 3 pages, 1 figure

This might also interest you, although it does not precisely address your two points:
http://arxiv.org/abs/1404.0745
Does the BICEP2 Observation of Cosmological Tensor Modes Imply an Era of Nearly Planckian Energy Densities?
Chiu Man Ho, Stephen D. H. Hsu
(Submitted on 3 Apr 2014)
BICEP2 observations, interpreted most simply, suggest an era of inflation with energy densities of order (1016GeV)4, not far below the Planck density. However, models of TeV gravity with large dimensions might allow a very different interpretation involving much more modest energy scales. We discuss the viability of inflation in such models, and conclude that existing scenarios do not provide attractive alternatives to single field inflation in four dimensions. Because the detection of tensor modes strengthens our confidence that inflation occurred, it disfavors models of large extra dimensions[/color], at least for the moment.
4 pages
 
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sufive said:
Dear every specialists, I heard that BICEP2's observation r=A_t/A_s=0.2 n_t=0 indicate two things:

1) n_t=0 excludes ekpyrotic cosmological model (ECM) definitely because ECM predicts n_t=2

2) r=0.2 excludes almost all current string inflation model (SIM) such as KKLMMT because this observation requires inflaton field vary at leasts 10Mp while SIM do not allows such big range varyings

Who can tell me more about this two point of view


Turok commented on this here:
http://www.perimeterinstitute.ca/news/new-window-big-bang
“It would conclusively refute the ekpyrotic and cyclic models we proposed a decade ago. However, more recent bouncing universe models based on the Higgs field might still be viable.”
 
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Jim Carrey on ekpyrotic Universe (start at about 3:00):
 
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