Primordial supersymmetric inflation

John Ellis; D. V. Nanopoulos; K. A. Olive; K. Tamvakis

doi:10.1016/0550-3213(83)90592-8

Primordial supersymmetric inflation

John Ellis, D. V. Nanopoulos, K. A. Olive, K. Tamvakis

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

113 Scopus citations

Abstract

We discuss the motivations for reconsidering cosmological inflation in supersymmetric theories as contrasted with conventional GUTs. Radiative corrections to the effective potential can be made arbitrarily small in supersymmetric GUTs, removing some of the obstacles to inflation. We analyze general renormalizable potentials at the tree level and show that the required fine-tuning of parameters becomes less acute if inflation takes place before the grand unified phase transition, a hypothesis we term primordial inflation. We show how the grand unified monopole problem can be solved in supersymmetric GUTs embodying primordial inflation.

Original language	English (US)
Pages (from-to)	524-548
Number of pages	25
Journal	Nuclear Physics, Section B
Volume	221
Issue number	2
DOIs	https://doi.org/10.1016/0550-3213(83)90592-8
State	Published - Jul 11 1983

Bibliographical note

Funding Information:
We thank Nicky Henderson for her rapid and efficient help with this paper. This work was supported in part by K.A.O.'s NATO/NSF postdoctoral fellowship.

Publisher link

10.1016/0550-3213(83)90592-8

Find It

Find It at U of M Libraries

Cite this

@article{ff65fa784acb4a9aad5cad435b8af446,

title = "Primordial supersymmetric inflation",

abstract = "We discuss the motivations for reconsidering cosmological inflation in supersymmetric theories as contrasted with conventional GUTs. Radiative corrections to the effective potential can be made arbitrarily small in supersymmetric GUTs, removing some of the obstacles to inflation. We analyze general renormalizable potentials at the tree level and show that the required fine-tuning of parameters becomes less acute if inflation takes place before the grand unified phase transition, a hypothesis we term primordial inflation. We show how the grand unified monopole problem can be solved in supersymmetric GUTs embodying primordial inflation.",

author = "John Ellis and Nanopoulos, {D. V.} and Olive, {K. A.} and K. Tamvakis",

note = "Funding Information: We thank Nicky Henderson for her rapid and efficient help with this paper. This work was supported in part by K.A.O.'s NATO/NSF postdoctoral fellowship.",

year = "1983",

month = jul,

day = "11",

doi = "10.1016/0550-3213(83)90592-8",

language = "English (US)",

volume = "221",

pages = "524--548",

journal = "Nuclear Physics B",

issn = "0550-3213",

publisher = "Elsevier",

number = "2",

}

TY - JOUR

T1 - Primordial supersymmetric inflation

AU - Ellis, John

AU - Nanopoulos, D. V.

AU - Olive, K. A.

AU - Tamvakis, K.

N1 - Funding Information: We thank Nicky Henderson for her rapid and efficient help with this paper. This work was supported in part by K.A.O.'s NATO/NSF postdoctoral fellowship.

PY - 1983/7/11

Y1 - 1983/7/11

N2 - We discuss the motivations for reconsidering cosmological inflation in supersymmetric theories as contrasted with conventional GUTs. Radiative corrections to the effective potential can be made arbitrarily small in supersymmetric GUTs, removing some of the obstacles to inflation. We analyze general renormalizable potentials at the tree level and show that the required fine-tuning of parameters becomes less acute if inflation takes place before the grand unified phase transition, a hypothesis we term primordial inflation. We show how the grand unified monopole problem can be solved in supersymmetric GUTs embodying primordial inflation.

AB - We discuss the motivations for reconsidering cosmological inflation in supersymmetric theories as contrasted with conventional GUTs. Radiative corrections to the effective potential can be made arbitrarily small in supersymmetric GUTs, removing some of the obstacles to inflation. We analyze general renormalizable potentials at the tree level and show that the required fine-tuning of parameters becomes less acute if inflation takes place before the grand unified phase transition, a hypothesis we term primordial inflation. We show how the grand unified monopole problem can be solved in supersymmetric GUTs embodying primordial inflation.

UR - http://www.scopus.com/inward/record.url?scp=0000555345&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0000555345&partnerID=8YFLogxK

U2 - 10.1016/0550-3213(83)90592-8

DO - 10.1016/0550-3213(83)90592-8

M3 - Article

AN - SCOPUS:0000555345

VL - 221

SP - 524

EP - 548

JO - Nuclear Physics B

JF - Nuclear Physics B

SN - 0550-3213

IS - 2

ER -

Primordial supersymmetric inflation

Abstract

Bibliographical note

Publisher link

Find It

Other files and links

Fingerprint

Cite this