Towards inflation in string theory
By S. Kachru, R. Kallosh, Andrei Linde, J. Maldacena, Liam McAllister, S. Trivedi. Journal of Cosmology and Astroparticle Physics, 2003
1,318 citations recorded by the source corpus.
I will discuss the development of inflationary theory and its present status, including recent progress in describing de Sitter space and inflationary universe in string theory.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/7f2a03a30a6fea3e127a4001bf3d11616c386cb8
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
In Nuclear and High Energy Physics
- Liam McAllister
- Eran Palti
- D. Baumann
- R. Kallosh
- Andrei Linde
- F. Quevedo
- Ralph Blumenhagen
- E. Silverstein
Citations in the corpus
- String loop corrections to Kähler potentials in orientifolds (2005, background): “A second interesting application of our results lies in the field of brane inflation, initiated in [6, 7, 8, 9] where an open string scalar plays the role of the inflaton field.”
- Planck2018 results (2018, background): “– D-brane inflationary models (Kachru et al. 2003; Dvali et al. 2001; Garcı́a-Bellido et al. 2002) provide a good fit to Planck and BK14 data for a large portion of their parameter space.”
- Inflation in realistic D-brane models (2004, methodology): “In this sense our scenario generalises the one in [9].”
- Pure de Sitter supergravity (2015, methodology): “The Kachru, Kallosh, Linde and Trivedi (KKLT) uplifting procedure for constructing de Sitter (dS) vacua in string theory was proposed in [3].”
- Emergence of spontaneously broken supersymmetry on an anti-D3-brane in KKLT dS vacua (2014, background): “The uplifting term was added in the next step in the KKLT construction in the form [1,2]”
- Cosmology with nilpotent superfields (2014, background): “as expected in the situation with warping [54].”
- Inflation and String Theory (2014, background): “throat region [41] as a source for inflation.”
- Axion inflation in type II string theory (2007, background): “[62, 63, 64], we will add an up-lift term of the form Vup = κ/Vα to V (S), where κ is a tunable constants and α is a rational number of order unity depending on the source of the up-lifting energy.”
- Loop corrections to volume moduli and inflation in string theory (2004, methodology): “Note that there is a slight difference to the model of KKLMMT.”
- D‐branes in Standard Model building, gravity and cosmology (2003, background): “There are, however, several problems with this type of inflationary scenarios [308].”
- Closer towards inflation in string theory (2003, background): “Recently, there was just such an attempt (KKLMMT) [ 3 ].”
- TOWARD REALISTIC INTERSECTING D-BRANE MODELS (2005, methodology): “This idea of brane inflation [221] has been applied to construct inflationary models arising from the collision of branes and anti-branes [221, 222, 223, 224, 225], as well as branes intersecting at angles [226, 227, 228].”