Growing Matter

Abstract

We investigate quintessence cosmologies with a matter component consisting of particles with an increasing mass. While negligible in early cosmology, the appearance of a growing matter component has stopped the evolution of the cosmon field at a redshift around six. In turn, this has triggered the accelerated expansion of the Universe. We propose to associate growing matter with neutrinos. Then the presently observed dark energy density and its equation of state are determined by the neutrino mass.

6 pages

References in corpus (22)

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• Cosmology and the Fate of Dilatation Symmetry
• The Supernova Legacy Survey: Measurement of Omega_M, Omega_Lambda and w from the First Year Data Set
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• Neutrino Dark Energy -- Revisiting the Stability Issue
• Non-linear Structure Formation in Cosmologies with Early Dark Energy
• Structure Formation and the Time Dependence of Quintessence
• Probing Quintessence with Time Variation of Couplings
• Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energy
• Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS
• Non-linear gravitational clustering in scalar field cosmologies

Cited by in corpus (141)

• Cosmology and Fundamental Physics with the Euclid Satellite
• Cosmology and fundamental physics with the Euclid satellite
• Varying constants, Gravitation and Cosmology
• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Dark Energy vs. Modified Gravity
• Non-minimal dark sector physics and cosmological tensions
• Planck 2015 results. XIV. Dark energy and modified gravity
• Hydrodynamical N-body simulations of coupled dark energy cosmologies
• Coupled and Extended Quintessence: theoretical differences and structure formation
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• Update on Coupled Dark Energy and the $H_0$ tension
• Models of coupled dark matter to dark energy
• Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
• Notes on $f(T)$ Theories
• Extended $f(R,L_m)$ gravity with generalized scalar field and kinetic term dependences
• Time dependent couplings in the dark sector: from background evolution to nonlinear structure formation
• Variable gravity: A suitable framework for quintessential inflation
• Variable gravity Universe
• Emergent scale symmetry: Connecting inflation and dark energy
• Testing modified gravity with Planck: the case of coupled dark energy
• How early is early dark energy?
• Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Effects of dark sectors' mutual interaction on the growth of structures
• The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models
• Unification of inflation and dark energy {\it à la} quintessential inflation
• Inflation, quintessence, and the origin of mass
• Clarifying the effects of interacting dark energy on linear and nonlinear structure formation processes
• Clarifying spherical collapse in coupled dark energy cosmologies
• Dark Energy in Practice
• A comparison of structure formation in minimally and non-minimally coupled quintessence models
• Early massive clusters and the bouncing coupled dark energy
• Structure formation in cosmologies with oscillating dark energy
• Primordial black holes from fifth forces
• Primordial dark matter halos from fifth forces
• Gravitational waves from global cosmic strings in quintessential inflation
• Clustering and redshift-space distortions in interacting dark energy cosmologies
• Dark energy: investigation and modeling
• Looking Beyond Lambda with the Union Supernova Compilation
• Quintessential inflation: A tale of emergent and broken symmetries
• Using dark energy to suppress power at small scales
• Very large scale structures in growing neutrino quintessence
• Eternal Universe
• The Imprint of f(R) Gravity on Non-Linear Structure Formation
• Cosmic Neutrino Background Detection in Large-Neutrino-Mass Cosmologies
• Quintessential Affleck-Dine baryogenesis with non-minimal couplings
• Classical and Quantum Solutions in Brans-Dicke Cosmology with a Perfect Fluid
• Doppelgänger dark energy: modified gravity with non-universal couplings after GW170817
• Steady accretion of an elastic body on a hard spherical surface and the notion of a four-dimensional reference space
• Unified early and late Universe cosmology through dissipative effects in steep quintessential inflation potential models
• Quintessential Inflation in a thawing realization
• The halo mass function in interacting Dark Energy models
• Neutrino lumps and the Cosmic Microwave Background
• A Dark Matter Trigger for Early Dark Energy Coincidence
• Relic gravitational waves from Quintessential Inflation
• Constraints on interacting dark energy models from galaxy Rotation Curves
• Model marginalized constraints on neutrino properties from cosmology
• Boosting Ultraviolet Freeze-in in NO Models
• Observational constraints on varying neutrino-mass cosmology
• Multiple Dark Matter as a self-regulating mechanism for dark sector interactions
• Structure Formation and Backreaction in Growing Neutrino Quintessence
• Scale-Dependent Growth from a Transition in Dark Energy Dynamics
• Dynamics of neutrino lumps in growing neutrino quintessence
• Cosmon inflation
• Mass varying neutrinos, symmetry breaking, and cosmic acceleration
• Hot big bang or slow freeze?
• Halo Formation from Yukawa Forces in the Very Early Universe
• Towards scaling cosmological solutions with full coupled Horndeski Lagrangian: the KGB model
• Dynamics of three-form dark energy with dark matter couplings
• Weak lensing predictions for coupled dark energy cosmologies at non-linear scales
• Cosmology of strongly interacting fermions in the early universe
• Neutrino Lumps in Quintessence Cosmology
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Conformally Coupled Tachyonic Dark Energy
• Surfing gravitational waves: can bigravity survive growing tensor modes?
• Model independent constraints on mass-varying neutrino scenarios
• Oscillating nonlinear large scale structure in growing neutrino quintessence
• Time variation of fundamental couplings and dynamical dark energy
• Modified gravity and coupled quintessence
• The general form of the coupled Horndeski Lagrangian that allows cosmological scaling solutions
• Neutrino Lump Fluid in Growing Neutrino Quintessence
• Coupled dark energy and dark matter from dilatation anomaly
• Observational constraints on the oscillating dark energy cosmologies
• Mass freezing in growing neutrino quintessence
• Isocurvature Perturbations of Dark Energy and Dark Matter from the Swampland Conjecture
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Linear Perturbation constraints on Multi-coupled Dark Energy
• Raytracing simulations of coupled dark energy models
• Mass Varying Neutrinos, Quintessence, and the Accelerating Expansion of the Universe
• Nonlinear matter spectra in growing neutrino quintessence
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems I - Linear theory revisited
• Exact cosmological solutions of models with an interacting dark sector
• Damped Neutrino Oscillations in a Conformal Coupling Model
• Supernova constraints on Multi-coupled Dark Energy
• Nonlinear growing neutrino cosmology
• Cosmology from pregeometry
• Stability of mass varying particle lumps
• Modifying Gravity at Low Redshift
• Spontaneous symmetry breaking in the late Universe and glimpses of early Universe phase transitions à la baryogenesis
• Investigating clustering dark energy with 3d weak cosmic shear
• The cosmological constant and higher dimensional dilatation symmetry
• Mass-varying neutrino in light of cosmic microwave background and weak lensing
• Neutrino generated dynamical dark energy with no dark energy field
• Nonbaryonic dark matter and scalar field coupled with a transversal interaction plus decoupled radiation
• Neutrino Dark Energy With More Than One Neutrino Species
• Relaxing neutrino mass bounds by a running cosmological constant
• Redshift space distortions in the presence of non-minimally coupled dark matter
• The kinematic Sunyaev-Zel'dovich effect of the large-scale structure (II): the effect of modified gravity
• The effect of interacting dark energy on local measurements of the Hubble constant
• Warping with dilatation symmetry and self-tuning of the cosmological constant
• Cosmic Degeneracies III: N-body Simulations of Interacting Dark Energy with Non-Gaussian Initial Conditions
• A new take on the inflationary quintessence
• Do Bound Structures Brake Cosmic Acceleration?
• Spherical collapse in coupled quintessence with a $\Lambda$CDM background
• Freezing Out Early Dark Energy
• Static structure of chameleon dark Matter as an explanation of dwarf spheroidal galactic core
• Gauge Issues in Extended Gravity and f(R) Cosmology
• Early dark energy constraints on growing neutrino quintessence cosmologies
• Observational Constraints on Early Coupled Quintessence
• Euclid preparation. Simulations and nonlinearities beyond $\Lambda$CDM. 1. Numerical methods and validation
• Tachyon field non-minimally coupled to massive neutrino matter
• Backreaction in Growing Neutrino Quintessence
• False Vacuum in the Supersymmetric Mass Varying Neutrinos Model
• The Matter Power Spectrum of Dark Energy Models and the Harrison-Zel'dovich Prescription
• Relaxing cosmological constraints on current neutrino masses
• Screening Mechanisms on White Dwarfs: Symmetron & Dilaton
• Slow-Roll Inflation in the Presence of a Dark Energy Coupling
• Early dark energy in the pre- and post-recombination epochs
• Dark energy from a renormalization group flow
• Observational constraints on the massive neutrinos induced late-time cosmic acceleration
• Bimodal/Schizophrenic Neutrino As a Bridge between Inflation and Dark Energy
• Coupling active and sterile neutrinos in the cosmon plus seesaw framework
• Phenomenology of Hybrid Scenarios of Neutrino Dark Energy
• Imprints of vector field non-standard couplings on solar neutrino flux
• Structural Implications of the Chameleon Mechanism on White Dwarfs
• The Two-Measure Theory and an Overview of Some of its Manifestations
• Cosmon as the Modulon: Non-Gaussianity from Dark Energy
• Interacting Quintessence and Growth of Structure
• Dark Energy Simulations
• Limits in late time conversion of cold dark matter into dark radiation
• Saving CNB assisted EDE model at the expense of quantum corrections?