### Abstract

To accommodate the observed accelerated expansion of the universe, one popular idea is to invoke a driving term in the Friedmann-Lemaître equation of dark energy which must then comprise 70% of the present cosmological energy density. We propose an alternative interpretation which takes into account the entropy and temperature intrinsic to the horizon of the universe due to the information holographically stored there. Dark energy is thereby obviated and the acceleration is due to an entropic force naturally arising from the information storage on the horizon surface screen. We consider an additional quantitative approach inspired by surface terms in general relativity and show that this leads to the entropic accelerating universe.

Original language | English (US) |
---|---|

Pages (from-to) | 273-277 |

Number of pages | 5 |

Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |

Volume | 696 |

Issue number | 3 |

DOIs | |

State | Published - Jan 31 2011 |

### Fingerprint

### Keywords

- Acceleration
- Gravity
- Thermodynamics

### ASJC Scopus subject areas

- Nuclear and High Energy Physics

### Cite this

*Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics*,

*696*(3), 273-277. https://doi.org/10.1016/j.physletb.2010.12.025

**Entropic accelerating universe.** / Easson, Damien; Frampton, Paul H.; Smoot, George F.

Research output: Contribution to journal › Article

*Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics*, vol. 696, no. 3, pp. 273-277. https://doi.org/10.1016/j.physletb.2010.12.025

}

TY - JOUR

T1 - Entropic accelerating universe

AU - Easson, Damien

AU - Frampton, Paul H.

AU - Smoot, George F.

PY - 2011/1/31

Y1 - 2011/1/31

N2 - To accommodate the observed accelerated expansion of the universe, one popular idea is to invoke a driving term in the Friedmann-Lemaître equation of dark energy which must then comprise 70% of the present cosmological energy density. We propose an alternative interpretation which takes into account the entropy and temperature intrinsic to the horizon of the universe due to the information holographically stored there. Dark energy is thereby obviated and the acceleration is due to an entropic force naturally arising from the information storage on the horizon surface screen. We consider an additional quantitative approach inspired by surface terms in general relativity and show that this leads to the entropic accelerating universe.

AB - To accommodate the observed accelerated expansion of the universe, one popular idea is to invoke a driving term in the Friedmann-Lemaître equation of dark energy which must then comprise 70% of the present cosmological energy density. We propose an alternative interpretation which takes into account the entropy and temperature intrinsic to the horizon of the universe due to the information holographically stored there. Dark energy is thereby obviated and the acceleration is due to an entropic force naturally arising from the information storage on the horizon surface screen. We consider an additional quantitative approach inspired by surface terms in general relativity and show that this leads to the entropic accelerating universe.

KW - Acceleration

KW - Gravity

KW - Thermodynamics

UR - http://www.scopus.com/inward/record.url?scp=78651075243&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=78651075243&partnerID=8YFLogxK

U2 - 10.1016/j.physletb.2010.12.025

DO - 10.1016/j.physletb.2010.12.025

M3 - Article

AN - SCOPUS:78651075243

VL - 696

SP - 273

EP - 277

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 3

ER -