Swampland Conjecture and Inflation Model from Brane Perspective

Abstract

Over the past few decades, inflation models have been studied by researchers from different perspectives and conditions in order to introduce a model for the expanding universe. In this paper, we introduce a modified $f(R)$ gravitational model as ($R+\gamma R^p$) in order to examine a new condition for inflation models. Given that our studies are related to a modified $f(R)$ gravitational model on the brane, therefore we will encounter modified cosmological parameters. So, we first introduce these modified cosmological parameters such as spectral index, a number of e-folds and etc. Then, we apply these conditions to our modified $f(R)$ gravitational model in order to adapt to the swampland criteria. Finally, we determine the range of each of these parameters by plotting some figures and with respect to observable data such as Planck 2018.

21 pages, 15 captioned figures, Published in Physica Scripta

References in corpus (10)

• Disappearing cosmological constant in f(R) gravity
• On the Geometry of the String Landscape and the Swampland
• The Swampland: Introduction and Review
• The Weak Gravity Conjecture in three dimensions
• The Weak Gravity Conjecture and Effective Field Theory
• Brane assisted quintessential inflation with transient acceleration
• Beyond-one-loop quantum gravity action yielding both inflation and late-time acceleration
• Trans-Planckian Censorship and Inflation in Grand Unified Theories
• f(R) and Brans-Dicke Theories and the Swampland
• An Implication of "Gravity as the Weakest Force"

Cited by in corpus (15)

• Weak Gravity Conjecture from Conformal Field Theory: A Challenge from Hyperscaling Violating and Kerr-Newman-AdS Black Holes
• WGC and WCCC of black holes with quintessence and cloud strings in RPS space
• Pleasant behavior of swampland conjectures in the face of specific inflationary models
• Reissner-Nordström black holes surrounded by perfect fluid dark matter: testing the viability of weak gravity conjecture and weak cosmic censorship conjecture simultaneously
• Weak Cosmic Censorship and Weak Gravity Conjectures in CFT Thermodynamics
• Swampland dS conjecture in Mimetic $f(R,T)$ gravity
• WGC and WCC for charged black holes with quintessence and cloud of strings
• de Sitter Swampland Conjecture in String Field Inflation
• Swampland conjectures in hybrid metric-Palatini gravity
• Further Refining Swampland dS Conjecture in Mimetic f(G) Gravity
• Warm Inflation with Barrow Holographic Dark Energy
• Assessing WGC Compatibility in ModMax Black Holes via Photon Spheres Analysis and WCCC Validation
• Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
• Cosmic-Quantum Connections: Assessing the Viability of Weak Gravity and Weak Cosmic Censorship Conjectures in Kerr-Newman-Kiselev-Letelier Black Hole
• Stability of Extremal Black Holes and Weak Cosmic Censorship Conjecture in Kiselev Spacetime