Inflation, Swampland, and Landscape
arXiv:2112.04196 · doi:10.1142/S0217751X22500063
Abstract
In this paper, we evaluate a new refined de Sitter (dS) conjecture perspective. This conjecture provides interesting conditions in studying various inflationary models. Therefore we challenge refined dS conjecture with a general method for analyzing the potentials with the inflectional point near the top (V''= 0). We find the compatible spaces for our inflationary model that live out of swampland according to the latest observational data, such as Planck 2018.
arXiv comment15 pages, 3 figures, Accepted for publication in the International Journal of Modern Physics A (IJMPA)
References in corpus (53)
- Planck 2015 results. XIII. Cosmological parameters
- de Sitter Vacua in String Theory
- The Standard Model Higgs boson as the inflaton
- The String Landscape, Black Holes and Gravity as the Weakest Force
- On the Geometry of the String Landscape and the Swampland
- Encyclopaedia Inflationaris
- The Swampland: Introduction and Review
- The Trans-Planckian Problem of Inflationary Cosmology
- Distance and de Sitter Conjectures on the Swampland
- Quintessence: A Review
- BICEP2 / Keck Array x: Constraints on Primordial Gravitational Waves using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season
- Standard Model Higgs boson mass from inflation: two loop analysis
- De Sitter Space and the Swampland
- Higgs inflation at the critical point
- The landscape, the swampland and the era of precision cosmology
- Higgs inflation still alive
- Living beyond the edge: Higgs inflation and vacuum metastability
- The Weak Gravity Conjecture in three dimensions
- A Tower Weak Gravity Conjecture from Infrared Consistency
- Amplitudes' Positivity, Weak Gravity Conjecture, and Modified Gravity
- Meson spectroscopy from holomorphic probes on the warped deformed conifold
- Higgs inflation from Standard Model criticality
- Warm inflation as a way out of the swampland
- Infrared Consistency and the Weak Gravity Conjecture
- Cosmological window onto the string axiverse and the supersymmetry breaking scale
- Warm Inflation in the light of Swampland Criteria
- Uplifting Runaways
- Weak Gravity Conjecture in AdS/CFT
- The Weak Gravity Conjecture and Effective Field Theory
- Do We Live in the Swampland?
- Rescuing Single Field Inflation from the Swampland
- Avoiding the string swampland in single-field inflation: Excited initial states
- Quintessence Saves Higgs Instability
- Steep Eternal Inflation and the Swampland
- Computational Complexity of Vacua and Near-Vacua in Field and String Theory
- Phenomenological Consequences of the Refined Swampland Conjecture
- Chaotic inflation on the brane and the Swampland Criteria
- Inflation at the Tip
- Electroweak relaxation of cosmological hierarchy
- De Sitter Vacua in No-Scale Supergravity
- Primordial Black Holes and the String Swampland
- The swampland conjecture and the Higgs expectation value
- A Potential Mechanism for Inflation from Swampland Conjectures
- Strongly Coupled Quintessence
- f(R) and Brans-Dicke Theories and the Swampland
- Towards a proof of the Weak Gravity Conjecture
- On uplifts by warped anti-D3-branes
- New Scalar Field Quartessence
- Inflation from the internal volume in type IIB/F-theory compactification
- Two-field Cosmological -attractors with Noether Symmetry
- Gauss-Bonnet inflation and swampland
- Beyond Standard Inflationary Cosmology
- An Implication of "Gravity as the Weakest Force"
Cited by in corpus (5)
- Weak Cosmic Censorship and Weak Gravity Conjectures in CFT Thermodynamics
- Swampland dS conjecture in Mimetic gravity
- WGC and WCC for charged black holes with quintessence and cloud of strings
- de Sitter Swampland Conjecture in String Field Inflation
- Further Refining Swampland dS Conjecture in Mimetic f(G) Gravity