Quintessential inflation

Abstract

We present an explicit observationally acceptable model for evolution from inflation to the present epoch under the assumption that the entropy and matter of the familiar universe are from gravitational particle production at the end of inflation. This eliminates the problem of finding a satisfactory coupling of the inflaton and matter fields. Since the inflaton potential $V(\varphi )$ may be a monotonic function of the inflaton $\varphi$, the inflaton energy could produce an observationally significant effective cosmological constant, as in quintessence.

6 pages, REVTeX, 1 figure

Cited by in corpus (450)

• Dynamics of dark energy
• The Cosmological Constant and Dark Energy
• f(R) theories
• The Cosmological Constant
• In the Realm of the Hubble tension $-$ a Review of Solutions
• k-Inflation
• Beyond the Cosmological Standard Model
• Inflation Dynamics and Reheating
• The Pre-Big Bang Scenario in String Cosmology
• Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A${}^{\ast }$
• How long before the end of inflation were observable perturbations produced?
• Quintessence arising from exponential potentials
• Dark Matter and Dark Energy
• Interacting quintessence solution to the coincidence problem
• Is there Supernova Evidence for Dark Energy Metamorphosis ?
• Quintessence as a run-away dilaton
• Fluid Dark Matter
• Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
• Cosmological Backgrounds of Gravitational Waves and eLISA/NGO: Phase Transitions, Cosmic Strings and Other Sources
• Oscillating Quintom and the Recurrent Universe
• Cosmology with the Laser Interferometer Space Antenna
• Primordial magnetogenesis
• The Cosmological Constant Problem and Quintessence
• Instant Preheating
• Cosmic anti-friction and accelerated expansion
• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Cosmological inflation in $F(R,\mathcal{G})$ gravity
• Black holes with scalar hair in light of the Event Horizon Telescope
• The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
• Production and detection of relic gravitons in quintessential inflationary models
• Gravitational Baryogenesis
• Quintessence and the Relic Density of Neutralinos
• Cosmology With Negative Potentials
• Cosmology with Mimetic Matter
• Gravitino Production After Inflation
• Recent Advances on Inflation
• Relic Gravity Waves from Braneworld Inflation
• An emergent universe from a loop
• Relating gravitational wave constraints from primordial nucleosynthesis, pulsar timing, laser interferometers, and the CMB: implications for the early universe
• Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter
• Inflation and Preheating in NO models
• Steep inflation: ending braneworld inflation by gravitational particle production
• de Sitter black hole with a conformally coupled scalar field in four dimensions
• Inflation, braneworlds and quintessence
• Quintessential Haloes around Galaxies
• Induced gravitational waves in a general cosmological background
• Beyond the Standard Models with Cosmic Strings
• Applications of scalar attractor solutions to Cosmology
• Ghosts, Instabilities, and Superluminal Propagation in Modified Gravity Models
• Gravitational Particle Production in Oscillating Background and Its Cosmological Implications
• Cosmological coincidence problem in interacting dark energy models
• Exhaustive Study of Cosmic Microwave Background Anisotropies in Quintessential Scenarios
• Dark energy, $\alpha$-attractors, and large-scale structure surveys
• Modeling Quintessential Inflation
• Reheating After Quintessential Inflation and Gravitational Waves
• Quintessential Inflation with $\alpha$-attractors
• On likely values of the cosmological constant
• Quintessence and Gravitational Waves
• Inflationary Magnetogenesis without the Strong Coupling Problem
• Electromagnetic response of a Gaussian beam to high-frequency relic gravitational waves in quintessential inflationary models
• Gravitational Wave Detection with High Frequency Phonon Trapping Acoustic Cavities
• Cosmological Particle Production: A Review
• Bouncing Loop Quantum Cosmology from $F(T)$ gravity
• Primordial Spectrum of Gauge Fields from Inflation
• Quintessence models in Supergravity
• Ultra High Energy Cosmic Rays and Inflation Relics
• Gravitational Effects on Inflaton Decay
• Spikes in the Relic Graviton Background from Quintessential Inflation
• Variable gravity Universe
• Ability of LIGO and LISA to probe the equation of state of the early Universe
• Quintessential Inflation on the Brane and the Relic Gravity Wave Background
• Probing the Universe through the Stochastic Gravitational Wave Background
• Emergent scale symmetry: Connecting inflation and dark energy
• Curvaton Reheating in Non-oscillatory Inflationary Models
• Inflation, dark matter and dark energy in the string landscape
• Confronting Braneworld Cosmology with Supernova data and Baryon Oscillations
• Instant Preheating in Quintessential Inflation with $\alpha$-Attractors
• Noninteracting dark matter
• Reheating from Tachyon Condensation
• Disformal Inflation
• From brane assisted inflation to quintessence through a single scalar field
• Laser-interferometric Detectors for Gravitational Wave Background at 100 MHz : Detector Design and Sensitivity
• Baryon asymmetry from electroweak tachyonic preheating
• Supernovae Ia Constraints on a Time-Variable Cosmological "Constant"
• Refining inflation using non-canonical scalars
• Baryogenesis from ultralight primordial black holes and strong gravitational waves from cosmic strings
• Energy-Momentum Tensor of Particles Created in an Expanding Universe
• Transition from quintessence to phantom phase in quintom model
• Thermal history of the plasma and high-frequency gravitons
• The Curvaton Hypothesis and the eta-problem of Quintessential Inflation, with and without Branes
• An Extended Matter Bounce Scenario: current status and challenges
• Non-minimal gravitational reheating during kination
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Cosmology from Rolling Massive Scalar Field on the anti-D3 Brane of de Sitter Vacua
• Ricci Reheating
• A k-essence Model Of Inflation, Dark Matter and Dark Energy
• Inflationary Phenomenology of Einstein Gauss-Bonnet Gravity Compatible with GW170817
• Super-Adiabatic Particle Number in Schwinger and de Sitter Particle Production
• Kination Dominated Reheating and Cold Dark Matter Abundance
• Quintessential Kination and Cold Dark Matter Abundance
• Curvaton reheating: an application to braneworld inflation
• MSLED: A Minimal Supersymmetric Large Extra Dimensions Scenario
• Runaway Quintessence, Out of the Swampland
• Gravitational particle creation for dark matter and reheating
• Inflation, quintessence, and the origin of mass
• Cosmological constant vs. quintessence
• Evolution and Dynamics of a Matter creation model
• The Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario
• Soundness of Dark Energy properties
• Inflation and Transition to a Slowly Accelerating Phase from S.S.B. of Scale Invariance
• Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO
• Low-scale Quintessential Inflation
• Hybrid cosmological attractors
• Stochastic backgrounds of relic gravitons: a theoretical appraisal
• Features in Dark Energy Equation of State and Modulations in the Hubble Diagram
• Primordial backgrounds of relic gravitons
• Towards inflation and dark energy cosmologies from modified Gauss-Bonnet theory
• Warm Quintessential Inflation
• Viability of the matter bounce scenario in Loop Quantum Cosmology for general potentials
• Chaplygin inspired Inflation
• Stochastic backgrounds of relic gravitons, T$\Lambda$CDM paradigm and the stiff ages
• Curing inflationary degeneracies using reheating predictions and relic gravitational waves
• Observational constraints on Gauss-Bonnet cosmology
• Gravitational reheating through conformally coupled superheavy scalar particles
• Cosmological constraints on slow-roll inflation: an update
• Constraints on Cosmic Quintessence and Quintessential Inflation
• Stochastic Gravitational Waves from Particle Origin
• Tracking quintessential inflation from brane worlds
• A Simple Model for Quintessential Inflation
• Gravitational waves from global cosmic strings in quintessential inflation
• Gravitational Production of Superheavy Dark Matter and Associated Cosmological Signatures
• Steep Inflation followed by Born-Infeld Reheating
• Tachyonic Quintessential Inflation
• Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
• Primordial Black Hole Archaeology with Gravitational Waves from Cosmic Strings
• Cosmological Signatures of Superheavy Dark Matter
• Hubble-induced phase transitions on the lattice with applications to Ricci reheating
• Gravitational reheating in quintessential inflation
• Rotating hairy black holes and thermodynamics from gravitational decoupling
• Unified Model of k-Inflation, Dark Matter & Dark Energy
• A review of Quintessential Inflation
• Recycling the universe using scalar fields
• A simple nonsingular inflationary quintessential model
• Primordial black holes and gravitational waves in nonstandard cosmologies
• Quintessential Baryogenesis
• Quintessential inflation in Palatini $f(R)$ gravity
• Dark energy: investigation and modeling
• Constraints on quintessence scalar field models using cosmological observations
• Compactification, Vacuum Energy and Quintessence
• Induced Gravitational Wave interpretation of PTA data: a complete study for general equation of state
• Field theory model giving rise to "quintessential inflation" without the cosmological constant and other fine tuning problems
• Higgs condensation as an unwanted curvaton
• Inconsistency of an inflationary sector coupled only to Einstein gravity
• Dark energy from primordial inflationary quantum fluctuations
• Palatini $R^2$ Quintessential Inflation
• Towards a model of Quintessential Inflation
• Precision cosmology and the stiff-amplified gravitational-wave background from inflation: NANOGrav, Advanced LIGO-Virgo and the Hubble tension
• Exact Solutions in Chiral Cosmology
• Aspects of Scalar Field Dynamics in Gauss-Bonnet Brane Worlds
• Dilatonic Interpretation of the Quintessence?
• Quintessential inflation: A tale of emergent and broken symmetries
• Implications of the NANOGrav result on primordial gravitational waves in nonstandard cosmologies
• Unification models with reheating via primordial black holes
• Accessibility of the Pre-Big-Bang Models to LIGO
• Growth of Dark Matter Perturbations during Kination
• Electroweak relaxation of cosmological hierarchy
• Accelerating dark energy models with anisotropic fluid in Bianchi type-$V{I}_0$ space-time
• Preheating in Quintessential Inflation
• Brane assisted quintessential inflation with transient acceleration
• Quintessential Affleck-Dine baryogenesis with non-minimal couplings
• New Constraints on Dark Matter Production during Kination
• Big Bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves
• Notes on teleparallel cosmology with nonminimally coupled scalar field
• String inspired explanation for the super-acceleration of our universe
• Probing Dark Energy models with neutrons
• Stochastic Gravitational Waves from Inflaton Decays
• Simple inflationary quintessential model II: Power law potentials
• Expansion history-dependent oscillations in the scalar-induced gravitational wave background
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• On exact solutions for quintessential (inflationary) cosmological models with exponential potentials
• Gravitational wave signals and cosmological consequences of gravitational reheating
• Trapped Quintessential Inflation
• Dark Fluid: Towards a unification of empirical theories of galaxy rotation, Inflation and Dark Energy
• Quintessential Inflation in a thawing realization
• Brane Cosmological Evolution With Bulk Matter
• Remarks on Dynamical Dark Energy Measured by the Conformal Age of the Universe
• Global Fluctuation Spectra in Big Crunch/Big Bang String Vacua
• DGP Cosmology with a Non-Minimally Coupled Scalar Field on the Brane
• Cosmological evolution of general scalar fields in a brane-world cosmology
• Self consistent estimates of magnetic fields from reheating
• Constraint on reheating after f(R) inflation from gravitational waves
• Hyperbolic Inflation in the Light of Planck 2015 data
• Initial conditions for quintessence after inflation
• Reheating constraints in quintessential inflation
• Challenges and Opportunities of Gravitational Wave Searches above 10 kHz
• The w = -1 crossing of the quintom model with slowly-varying potentials
• Introduction to Big Bang Nucleosynthesis and Modern Cosmology
• Boosting Ultraviolet Freeze-in in NO Models
• Warm Little Inflaton becomes Dark Energy
• The generality of inflation in closed cosmological models with some quintessence potentials
• On the viability of quintessential inflationary models from observational data
• Creating the Universe from Brane-Antibrane Annihilation
• Gravitational particle production in bouncing cosmologies
• Cold Dark Matter in non-Standard Cosmologies, PAMELA, ATIC and Fermi LAT
• A Study of an Einstein Gauss-Bonnet Quintessential Inflationary Model
• Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions
• Quintessential $\alpha$-attractor inflation: forecasts for Stage IV galaxy surveys
• Dumping inflaton energy density out of this world
• Hubble-induced phase transitions: Walls are not forever
• Analytic topological hairy dyonic black holes and thermodynamics
• Chaotic scalar fields as models for dark energy
• Slinky Inflation
• Probing Inflation and Dark Energy with Current Cosmological Observations
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• Cosmon inflation
• Unsuccessful cosmology with Modified Gravity Models
• Cosmic magnetism, curvature and the expansion dynamics
• Quintessential Kination and Thermal Production of Gravitinos and Axinos
• Quintessential inflation at low reheating temperatures
• Scale-invariant alternatives to general relativity. III. The inflation--dark-energy connection
• Have Pulsar Timing Arrays detected the Hot Big Bang? Gravitational Waves from Strong First Order Phase Transitions in the Early Universe
• Signatures of Non-thermal Dark Matter with Kination and Early Matter Domination: Gravitational Waves versus Laboratory Searches
• Hybrid Quintessential Inflation
• The transition of equation of state of effective dark energy in the DGP model with bulk contents
• Gravitational Waves from an Inflation Triggered First-Order Phase Transition
• The Stochastic Gravitational-Wave Background and the Inflation to Radiation Transition in the Early Universe
• $\alpha$ attractors in Quintessential Inflation motivated by Supergravity
• Trapped Quintessential Inflation in the context of Flux Compactifications
• New universal property of cosmological gravitational wave anisotropies
• Gravitational Baryogenesis after Anisotropic Inflation
• Dark energy from bulk matter
• Dynamical back-reaction of relic gravitons
• Mirror World and Superstring-Inspired Hidden Sector of the Universe, Dark Matter and Dark Energy
• From formation to evaporation: Induced gravitational wave probes of the primordial black hole reheating scenario
• Sensitivity of wide band detectors to quintessential gravitons
• Observational Constraints on Dynamical Dark Energy Models
• Symmetric and Asymmetric Reheating
• Crossing the phantom divide in brane cosmology with curvature corrections and brane-bulk energy transfer
• Late-time quantum backreaction of a very light nonminimally coupled scalar
• Lorentzian Quintessential Inflation
• Parametrising non-linear dark energy perturbations
• Reconstructing a model of quintessential inflation
• Beyond the Poles in Attractor Models of Inflation
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• Exponential potential for an inflaton with nonminimal kinetic coupling and its supergravity embedding
• Gravitational reheating and superheavy Dark Matter creation after inflation with non-minimal coupling
• Sensitivity of a VIRGO pair to stochastic GW backgrounds
• Baryogenesis in the paradigm of quintessential inflation
• Reheating through the Higgs amplified by spinodal instabilities and gravitational creation of gravitons
• A brief note on how to unify dark matter, dark energy, and inflation
• Post-inflationary phases stiffer than radiation and Palatini formulation
• Analytic three-dimensional primary hair charged black holes and thermodynamics
• Large-scale magnetic fields, curvature fluctuations and the thermal history of the Universe
• Inflation and late-time acceleration from a double-well potential with cosmological constant
• Quintessential Inflation from Lorentzian Slow Roll
• Spontaneous symmetry breaking in cosmos: The hybrid symmetron as a dark energy switching device
• Probing for the Cosmological Parameters with PLANCK Measurement
• Cosmological models in Weyl geometrical scalar-tensor theory
• Understanding gravitational particle production in quintessential inflation
• Unified Models of Inflation and Quintessence
• Brane Cosmology with a Non-Minimally Coupled Bulk-Scalar Field
• The phase-space view of non-local gravity cosmology
• The paradigm of warm quintessential inflation and spontaneous baryogenesis
• The Peebles -- Vilenkin quintessential inflation model revisited
• Cosmological constrains on minimally and non-minimally coupled scalar field models
• Dark matter and baryon-number generation in quintessential inflation via hierarchical right-handed neutrinos
• The unification of inflation and late-time acceleration in the frame of $k$-essence
• Dynamics of a Dark Matter Field with a Quartic Self-Interaction Potential
• Different reheating mechanisms in quintessence inflation
• Asymptotic behavior of w in general quintom model
• Unifying Inflation with early and late Dark Energy in Multi-Fields: Spontaneously broken scale invariant TMT
• Transition to Zero Cosmological Constant and Phantom Dark Energy as Solutions Involving Change of Orientation of Space-Time Manifold
• Curvaton scenario with low scale inflation revisited
• Heating up the cold bounce
• Acceleration of the Universe
• Unifying dark matter, dark energy and inflation with a fuzzy dark fluid
• Relic gravitons and high-frequency detectors
• Vacuum Structure and Gravitational Bags Produced by Metric-Independent Spacetime Volume-Form Dynamics
• Symmetry breaking and the onset of cosmic acceleration in scalar field models
• Dynamics of Quintessential Inflation
• Brane Cosmology with the Chameleon Scalar Field in Bulk
• Scaling solutions in quintessential inflation
• NO Curvatons or Hybrid Quintessential Inflation
• Cosmology from Moduli Dynamics
• Baryogenesis after Hyperextended Inflation
• Gradient expansion(s) and dark energy
• Inverse Power Law Quintessence with Non-Tracking Initial Conditions
• What is needed of a scalar field if it is to unify inflation and late time acceleration ?
• Gravitational decoupling for hairy black holes in asymptotically AdS spacetimes
• Dark energy and dark matter from an inhomogeneous dilaton
• Quintessential inflation with a trap and axionic dark matter
• Induced Gravity and the Attractor Dynamics of Dark Energy/Dark Matter
• Gravitational wave constraints on the observable inflation
• Post-inflationary thermal histories and the refractive index of relic gravitons
• Scalar particle production in a simple Horndeski theory
• Cosmic acceleration and de Sitter expansion in hybrid mass varying neutrino model
• Classical and quantum exact solutions for a FRW in chiral like cosmology
• A Model for Structure Formation Seeded by Gravitationally Produced Matter
• Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs
• Constraints on inflation in closed universe
• Generalized Galileon Model -- cosmological reconstruction and the Vainshtein mechanism --
• Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
• T-Model Inflation and Bouncing Cosmology
• Dynamical system analysis of Dirac-Born-Infeld scalar field cosmology in coincident $f(Q)$ gravity
• DESI constraints on $\alpha$-attractor inflationary models
• Interacting agegraphic quintessence dark energy in non-flat universe
• Cosmic backgrounds of relic gravitons and their absolute normalization
• Chameleonic inflation
• Embedding of FRW Cosmology in DGP Scenario with a Non-Minimally Coupled Scalar Field on the Brane
• Cosmology from pregeometry
• Observable Gravitational Waves from Hyperkination in Palatini Gravity and Beyond
• Tracking Curvaton(s)?
• Broken Scale Invariance, Gravity Mass, and Dark Energy in Modified Einstein Gravity with Two Measure Finsler Like Variables
• Quintessential inflation from a variable cosmological constant in a 5D vacuum
• Quintessence in the Weyl-Gauss-Bonnet model
• Decaying Massive Particle in Matter and Radiation Dominated Eras
• Braneworld inflation with effective α-attractor potential
• Viability of the Matter Bounce Scenario
• Tracking Quintessence and Cold Dark Matter Candidates
• Gravitational wave generation in hybrid quintessential inflationary models
• Low-scale inflation in a model of dark energy and dark matter
• On the possibility of braneworld quintessential inflation
• Inflation, space-borne interferometers and the expansion history of the Universe
• Waterfall stiff period can generate observable primordial gravitational waves
• Instant preheating in a scale invariant two measures theory
• Non-Oscillatory No-Scale Inflation
• Quintessential Inflation in Palatini Gravity
• Inflation, phase transitions and the cosmological constant
• Dark energy as a remnant of inflation and electroweak symmetry breaking
• Cosmological Imprints of SUSY Breaking in Models of Sgoldstinoless Non-Oscillatory Inflation
• A Quintessentially Geometric Model
• Curvaton Dynamics in Brane-worlds
• The Inflationary Energy Scale in Braneworld Cosmology
• Dark Energy as Double N-Flation--Observational Predictions
• Future evolution in a backreaction model and the analogous scalar field cosmology
• Testing $\alpha$-attractor quintessential inflation against CMB and low-redshift data
• Dynamical Evolution of Gravitational Leptogenesis
• Bifurcations in Ratra-Peebles quintessence models and their extensions
• Late time acceleration in Palatini gravity
• Quintessential early dark energy
• Thawing in a coupled quintessence model
• Dynamical Analysis of Scalar Field Cosmologies with Spatial Curvature
• Remarks on generalized scalar-tensor models of dark energy
• Upper limit on the amplitude of gravitational waves around 0.1Hz from the Global Positioning System
• Form invariant transformations between n-- and m-- dimensional flat Friedmann--Robertson--Walker cosmologies
• Relic gravitons from stiff curvature perturbations
• Inhomogeneous cosmologies with Q-matter and varying $\Lambda$
• Power suppression from disparate mass scales in effective scalar field theories of inflation and quintessence
• Cosmological Coincidence without Fine Tuning
• Reheating mechanism of Curvaton with Nonminimal Derivative Coupling to Gravity
• Resonance of Gaussian electromagnetic field to the high frequency gravitational waves
• Mirror World with Broken Mirror Parity, E(6) Unification and Cosmology
• Is the formation of primordial black holes from single-field inflation compatible with standard cosmology?
• Dynamical systems in perturbative scalar field cosmology
• Emergence of cosmological scaling behavior in asymptotic regime
• How an era of kination impacts substructure and the dark matter annihilation rate
• The Dapor-Liegener model of Loop Quantum Cosmology: A dynamical analysis
• Thermalization, Fragmentation and Tidal Disruption: The Complex Galactic Dynamics of Dark Matter Superfluidity
• Present and future of CosmoLattice
• Cosmological Gravitational Wave Background from Phase Transitions in Neutron Stars
• Cosmology from multimeasure multifield model
• Relationship between (2+1) and 3+1)--Friedmann--Robertson--Walker cosmologies
• Minimal dark matter in type III seesaw
• Optimal Location of Two Laser-interferometric Detectors for Gravitational Wave Backgrounds at 100 MHz
• Spectator dark matter in non-standard cosmologies
• Two models unifying warm inflation with dark matter and dark energy
• Scalar induced gravitational waves review
• Gravitational production of superheavy baryonic and dark matter in quintessential inflation: nonconformally coupled case
• Palatini approach and large-scale magnetogenesis
• A universal bound on the duration of a kination era
• Sculpting the Extra Dimensions: Inflation from Codimension-2 Brane Back-reaction
• Scalar-Gauss-Bonnet model, the coincidence problem and the gravitational wave speed
• Quantum induced w = -1 crossing of the quintessence and phantom models
• Anisotropic chiral cosmology: exact solutions
• Connecting Primordial Gravitational Waves and Dark Energy
• Dark energy in hybrid inflation
• New Source for QCD Axion Dark Matter Production: Curvature Induced
• Reheating constraints in Instant Preheating
• Bi-metric Universe with Matter
• Dark Energy, Dark Matter and Gravity
• Quintessence and Inflation from Symmetry Breaking Transition of the Internal Manifold
• Gauge Field Theory Vacuum and Cosmological Inflation without Scalar Field
• Quintessential inflation and nonlinear effects of the tachyonic trap mechanism
• False Vacuum Transitions - Analytical Solutions and Decay Rate Values
• Observational constraints to a unified cosmological model
• Gravitational production of dark matter in the Peebles-Vilenkin model
• Cosmological consequences of a scalar field with oscillating equation of state. III. Unifying inflation with dark energy and small tensor-to-scalar ratio
• Gauge Field Production and Schwinger Reheating in Runaway Axion Inflation
• Alternative LISA-TAIJI networks: Detectability of the Parity Violation in Stochastic Gravitational Wave Background
• Do current observations support transient acceleration of our universe?
• Time-dependent correlations of inflationary perturbations
• Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation
• Catalytic Creation of Bubble Universe Induced by Quintessence in Five Dimensions
• A Large Mass Hierarchy from a Small Non-minimal Coupling
• High frequency background gravitational waves from spontaneous emission of gravitons by hydrogen and helium
• Lagrangian description of fluid flow with pressure in relativistic cosmology
• Quintessential Inflation for Exponential Type Potentials: Scaling and Tracker Behavior
• Constraining the quintessential $\alpha$-attractor inflation through dynamical horizon exit method
• Pole inflation in Jordan frame supergravity
• Gauge Invariant Perturbation Analysis for Quintessence with an Exponential Potential
• A Note on Gravitational Particle Production in Supergravity
• The spectrum of Gravitational Waves, their overproduction in quintessential inflation and its influence in the reheating temperature
• Inflationary magnetogenesis and non-local actions: The conformal anomaly
• Gravitational waves induced by matter isocurvature in general cosmologies
• Scaling solutions for asymptotically free quantum gravity
• B-L-symmetric Baryogenesis with Leptonic Quintessence
• Connecting Inflation to the NANOGrav 15-year Data Set via Massive Gravity
• Accelerated expansion of a universe containing a self-interacting Bose-Einstein gas
• Prediction of the Expansion of the Universe made by Alexander Friedmann and the Effect of Particle Creation in Cosmology
• Dark Matter in a bi-metric universe
• Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
• Two-Field Quintessential Higgs model and the Swampland
• Gravitational waves from a curvature-induced phase transition of a Higgs-portal dark matter sector
• Interacting Models of Generalised Chaplygin Gas and Modified Chaplygin Gas with Barotropic Fluid
• Cosmic Acceleration Data and Bulk-Brane Energy Exchange
• Note on the reheating temperature in Starobinsky-type potentials
• Dark energy without fine tuning
• Gravitational particle production of superheavy massive particles in Quintessential Inflation: A numerical analysis
• Reheating constraints and the $H_0$ tension in Quintessential Inflation
• Witten-O'Raifeartaigh potential revisited in the context of Warm Inflation
• The Quantum Phase of Inflation
• Non-canonical 3-form dark energy
• On the Scale of Inflation
• Cosmological viability of a double field unified model from warm inflation
• Dark-matter particles and baryons from inflation and spontaneous CP violation in the early universe
• Reheating via gravitational particle production in simple models of quintessence or $\Lambda$CDM inflation
• Is the cosmological dark sector better modeled by a generalized Chaplygin gas or by a scalar field?
• Can Chameleon Field be identified with Quintessence ?
• The Spirit of Unification: The Wei of Physics
• The dark(er) side of inflation
• Hot Big Bang from inflation without the inflaton reheating
• Loop-corrected scalar potentials and late-time acceleration in f(R) gravity
• Implications of single field inflation in general cosmological scenarios on the nature of dark energy given the swampland conjectures
• Dynamical suppression of non-adiabatic modes
• Spontaneous baryogenesis and generation of gravitational waves in a new model of quintessential $\alpha$-attractor
• Non-perturbative reheating and Nnaturalness
• Probing Leptogenesis and Pre-BBN Universe with Gravitational Waves Spectral Shapes
• Gravitational reheating at strong coupling
• Kination cosmology from scalar fields and gravitational-wave signatures
• Non-minimally coupled quintessential inflation
• Manifestations of String Theory in Astrophysical Data and at the LHC
• On Gauge Choice of Spherically Symmetric 3-Branes
• Relic gravitons at intermediate frequencies and the expansion history of the Universe
• Modelling Quintessential Inflation in Palatini Modified Gravity
• Viscous absorption of ultra-high-frequency gravitons
• Supernova constraints on higher-dimensional cosmology with a phantom field
• A cross-epoch endpoint-consistency test of a single effective scaling from dark energy to inflation
• A Model of Gravitational Leptogenesis
• Differences between scalar field and scalar density solutions
• Quintessential Inflation in Palatini $F(R,X)$ gravity