Neutrino effects on the morphology of cosmic large-scale structure
arXiv:2002.08846 · doi:10.1103/PhysRevD.101.063515
Abstract
In this work, we propose a powerful probe of neutrino effects on the large-scale structure (LSS) of the Universe, i.e., Minkowski functionals (MFs). The morphology of LSS can be fully described by four MFs. This tool, with strong statistical power, is robust to various systematics and can comprehensively probe all orders of N-point statistics. By using a pair of high-resolution N-body simulations, for the first time, we comprehensively studied the subtle neutrino effects on the morphology of LSS. For an ideal LSS survey of volume Gpc/, neutrino signals are mainly detected from void regions with a significant level up to and for CDM and total matter density fields, respectively. This demonstrates its enormous potential for much improving the neutrino mass constraint in the data analysis of up-coming ambitious LSS surveys.
arXiv comment8 pages, 2 figures, published in PRD
References in corpus (64)
- A Universal Density Profile from Hierarchical Clustering
- Evidence for oscillation of atmospheric neutrinos
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- The Simons Observatory: Science goals and forecasts
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Precision Electroweak Measurements on the Z Resonance
- Massive neutrinos and cosmology
- Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
- A hierarchy of voids: Much ado about nothing
- Weighing Neutrinos with Galaxy Surveys
- Dark matter maps reveal cosmic scaffolding
- Measurement of Neutrino Oscillations with the MINOS Detectors in the NuMI Beam
- Beyond genus statistics: a unifying approach to the morphology of cosmic structure
- Robust Morphological Measures for Large-Scale Structure in the Universe
- Minimizing the stochasticity of halos in large-scale structure surveys
- An efficient implementation of massive neutrinos in non-linear structure formation simulations
- High Performance P3M N-body code: CUBEP3M
- Impact of massive neutrinos on nonlinear matter power spectrum
- Determining the neutrino mass with Cyclotron Radiation Emission Spectroscopy - Project 8
- Neutrino mass in cosmology: status and prospects
- Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters
- The evolution of the galaxy distribution
- Voids in massive neutrino cosmologies
- Massive Neutrinos Leave Fingerprints on Cosmic Voids
- Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
- MassiveNuS: Cosmological Massive Neutrino Simulations
- Probing Cosmology with Weak Lensing Minkowski Functionals
- Simulating nonlinear cosmological structure formation with massive neutrinos
- Grid Based Linear Neutrino Perturbations in Cosmological N-body Simulations
- Minkowski Functionals of SDSS galaxies I : Analysis of Excursion Sets
- The imprint of neutrinos on clustering in redshift-space
- Physical effects involved in the measurements of neutrino masses with future cosmological data
- The impact of massive neutrinos on the abundance of massive clusters
- The KATRIN Neutrino Mass Experiment
- Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N-body Scheme
- Non Gaussianity and Minkowski Functionals: forecasts for Planck
- Breaking degeneracies in modified gravity with higher (than 2nd) order weak-lensing statistics
- The effect of massive neutrinos on the matter power spectrum
- An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
- The halo model in a massive neutrino cosmology
- Constraining neutrino mass with weak lensing Minkowski Functionals
- Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
- Constraining neutrino mass with tomographic weak lensing peak counts
- DEMNUni: Massive neutrinos and the bispectrum of large scale structures
- Finding cosmic voids and filament loops using topological data analysis
- Cosmological neutrino simulations at extreme scale
- Large-Scale Structure of the Universe as a Cosmic Standard Ruler
- Higher-order massive neutrino perturbations in large-scale structure
- Differential Neutrino Condensation onto Cosmic Structure
- Breaking the Degeneracy: Optimal Use of Three-point Weak Lensing Statistics
- Measurement of the Cold Dark Matter-Neutrino Dipole in the TianNu Simulation
- The imprint of gravity on weak gravitational lensing II : Information content in cosmic shear statistics
- Using the topology of large-scale structure in the WiggleZ Dark Energy Survey as a cosmological standard ruler
- Neutrino Signatures on the High Transmission Regions of the Lyman-alpha Forest
- New probe of departures from general relativity using Minkowski functionals
- Investigating the degeneracy between modified gravity and massive neutrinos with redshift-space distortions
- Parity-odd Neutrino Torque Detection
- Cosmic neutrinos: dispersive and non-linear
- On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing
- Topology of large scale structure as test of modified gravity
- Breaking cosmic degeneracies: Disentangling neutrinos and modified gravity with kinematic information
- Forecasts on neutrino mass constraints from the redshift-space two-point correlation function
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- Fisher for complements: Extracting cosmology and neutrino mass from the counts-in-cells PDF
- Weakly non-Gaussian formula for the Minkowski functionals in general dimensions
- Probing massive neutrinos with the Minkowski functionals of large-scale structure
- Biased tracer reconstruction with halo mass information
- Sensitivity tests of cosmic velocity fields to massive neutrinos
- The effects of peculiar velocities on the morphological properties of large-scale structure
- Hybrid multi-fluid-particle simulations of the cosmic neutrino background
- Imprint of massive neutrinos on Persistent Homology of large-scale structure
- Improved Lyman Alpha Tomography using Optimized Reconstruction with Constraints on Absorption (ORCA)
- Probing the Anisotropy and Non-Gaussianity in the Redshift Space through the Conditional Moments of the First Derivative
- Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
- Numerical investigation of non-Gaussianities in the phase and modulus of density Fourier modes