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Assisted inflation via tachyon condensation.

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Assisted inflation via tachyon condensation. / Mazumdar, Anupam; Panda, Sudhakar; Lorenzana, Abdel-Perez.
In: Nuclear Physics B, Vol. 614, No. 1-2, 29.10.2001, p. 101-116.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Mazumdar, A, Panda, S & Lorenzana, A-P 2001, 'Assisted inflation via tachyon condensation.', Nuclear Physics B, vol. 614, no. 1-2, pp. 101-116. https://doi.org/10.1016/S0550-3213(01)00410-2

APA

Mazumdar, A., Panda, S., & Lorenzana, A-P. (2001). Assisted inflation via tachyon condensation. Nuclear Physics B, 614(1-2), 101-116. https://doi.org/10.1016/S0550-3213(01)00410-2

Vancouver

Mazumdar A, Panda S, Lorenzana A-P. Assisted inflation via tachyon condensation. Nuclear Physics B. 2001 Oct 29;614(1-2):101-116. doi: 10.1016/S0550-3213(01)00410-2

Author

Mazumdar, Anupam ; Panda, Sudhakar ; Lorenzana, Abdel-Perez. / Assisted inflation via tachyon condensation. In: Nuclear Physics B. 2001 ; Vol. 614, No. 1-2. pp. 101-116.

Bibtex

@article{fa1a27c221fd40a394906cb5a3c25f29,
title = "Assisted inflation via tachyon condensation.",
abstract = "In this paper we propose a new mechanism of inflating the Universe with non-BPS D4-branes which decay into stable D3-branes via tachyon condensation. In a single brane scenario the tachyon potential is very steep and unable to support inflation. However, if the universe lives in a stack of branes produced by a set of noninteracting unstable -branes, then the associated set of tachyons may drive inflation along our 3 spatial dimensions. After tachyon condensation the Universe is imagined to be filled with a set of parallel stable D3-branes. We study the scalar density perturbations and reheating within this setup.",
author = "Anupam Mazumdar and Sudhakar Panda and Abdel-Perez Lorenzana",
note = "In this pioneering paper we have shown how our Universe emerges from the condensation of higher dimensional defects from string theory. This is amongst the first few papers which has embedded inflation within string theory. It has generated a wave of research developing its novel approach. 128 citations (SPIRES). RAE_import_type : Journal article RAE_uoa_type : Physics",
year = "2001",
month = oct,
day = "29",
doi = "10.1016/S0550-3213(01)00410-2",
language = "English",
volume = "614",
pages = "101--116",
journal = "Nuclear Physics B",
publisher = "ELSEVIER SCIENCE BV",
number = "1-2",

}

RIS

TY - JOUR

T1 - Assisted inflation via tachyon condensation.

AU - Mazumdar, Anupam

AU - Panda, Sudhakar

AU - Lorenzana, Abdel-Perez

N1 - In this pioneering paper we have shown how our Universe emerges from the condensation of higher dimensional defects from string theory. This is amongst the first few papers which has embedded inflation within string theory. It has generated a wave of research developing its novel approach. 128 citations (SPIRES). RAE_import_type : Journal article RAE_uoa_type : Physics

PY - 2001/10/29

Y1 - 2001/10/29

N2 - In this paper we propose a new mechanism of inflating the Universe with non-BPS D4-branes which decay into stable D3-branes via tachyon condensation. In a single brane scenario the tachyon potential is very steep and unable to support inflation. However, if the universe lives in a stack of branes produced by a set of noninteracting unstable -branes, then the associated set of tachyons may drive inflation along our 3 spatial dimensions. After tachyon condensation the Universe is imagined to be filled with a set of parallel stable D3-branes. We study the scalar density perturbations and reheating within this setup.

AB - In this paper we propose a new mechanism of inflating the Universe with non-BPS D4-branes which decay into stable D3-branes via tachyon condensation. In a single brane scenario the tachyon potential is very steep and unable to support inflation. However, if the universe lives in a stack of branes produced by a set of noninteracting unstable -branes, then the associated set of tachyons may drive inflation along our 3 spatial dimensions. After tachyon condensation the Universe is imagined to be filled with a set of parallel stable D3-branes. We study the scalar density perturbations and reheating within this setup.

U2 - 10.1016/S0550-3213(01)00410-2

DO - 10.1016/S0550-3213(01)00410-2

M3 - Journal article

VL - 614

SP - 101

EP - 116

JO - Nuclear Physics B

JF - Nuclear Physics B

IS - 1-2

ER -