Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
Fuente:
arXiv
Guardado en:
| Autores principales: | Korkidis, Giorgos, Pavlidou, Vasiliki |
|---|---|
| Formato: | Preprint |
| Publicado: |
2024
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Mass scaling relations for dark halos from an analytic universal outer density profile
por: Korkidis, Giorgos, et al.
Publicado: (2024)
por: Korkidis, Giorgos, et al.
Publicado: (2024)
Turnaround radius of galaxy clusters in N-body simulations
por: Korkidis, Giorgos, et al.
Publicado: (2019)
por: Korkidis, Giorgos, et al.
Publicado: (2019)
Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
por: Triantafyllou, Nikolaos, et al.
Publicado: (2024)
por: Triantafyllou, Nikolaos, et al.
Publicado: (2024)
The Density Profile of Dynamical Halos
por: Shields, Tristen, et al.
Publicado: (2025)
por: Shields, Tristen, et al.
Publicado: (2025)
Halo Radius (Splashback Radius) of Groups and Clusters of Galaxies on small scales
por: Kopylova, Flera G., et al.
Publicado: (2024)
por: Kopylova, Flera G., et al.
Publicado: (2024)
General-Relativistic Path Effects and the Local Hubble Expansion
por: Laaroua, Said
Publicado: (2025)
por: Laaroua, Said
Publicado: (2025)
Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos
por: Wang, Yikun, et al.
Publicado: (2026)
por: Wang, Yikun, et al.
Publicado: (2026)
The Non-universal Pseudo Phase-Space Density Profiles of Symphony Host Halos
por: Feng, Bocheng, et al.
Publicado: (2025)
por: Feng, Bocheng, et al.
Publicado: (2025)
Getting the tiger by the tail: Probing the turnaround radius of structures with outer halo density profiles
por: Grammatikos, Kyriakos, et al.
Publicado: (2018)
por: Grammatikos, Kyriakos, et al.
Publicado: (2018)
AtLAST -- Determination of Halo Mass Density Profiles at kpc Scales through Magnification Bias
por: González-Nuevo, Joaquín, et al.
Publicado: (2025)
por: González-Nuevo, Joaquín, et al.
Publicado: (2025)
On Direct Estimation of Density Parameters and Hubble Constant for $Λ$CDM Universe using Hubble Measurements
por: Pal, Srikanta, et al.
Publicado: (2022)
por: Pal, Srikanta, et al.
Publicado: (2022)
Beyond Linear Bias Expansions for AbacusSummit Halos at z = 8
por: Boone, Kyle K., et al.
Publicado: (2026)
por: Boone, Kyle K., et al.
Publicado: (2026)
Probabilistic Inference of Cosmological Density Parameters from Synthetic Hubble Expansion Data of Varying SNR Using Diverse Artificial Neural Network Architectures
por: Jin, Zijian, et al.
Publicado: (2025)
por: Jin, Zijian, et al.
Publicado: (2025)
What Prevents Resolving the Hubble Tension through Late-Time Expansion Modifications?
por: Zhou, Zhihuan, et al.
Publicado: (2025)
por: Zhou, Zhihuan, et al.
Publicado: (2025)
Fast Simulation of Cosmological Neutral Hydrogen based on the Halo Model
por: Hitz, Pascal, et al.
Publicado: (2024)
por: Hitz, Pascal, et al.
Publicado: (2024)
Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs
por: Tominaga, Hirobumi, et al.
Publicado: (2026)
por: Tominaga, Hirobumi, et al.
Publicado: (2026)
Darkness Visible: N-Body Simulations of Dark Matter Spikes in Hernquist Haloes
por: Kamermans, Jasper Leonora P. D., et al.
Publicado: (2024)
por: Kamermans, Jasper Leonora P. D., et al.
Publicado: (2024)
Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder
por: Breuval, Louise, et al.
Publicado: (2024)
por: Breuval, Louise, et al.
Publicado: (2024)
Constraining the Hubble Constant with a Simulated Full Covariance Matrix Using Neural Networks
por: Niu, Jing, et al.
Publicado: (2025)
por: Niu, Jing, et al.
Publicado: (2025)
Simulating Binary Primordial Black Hole Mergers in Dark Matter Halos
por: Aljaf, Muhsin, et al.
Publicado: (2024)
por: Aljaf, Muhsin, et al.
Publicado: (2024)
Tracing Primordial Gravitational Waves via non-Gaussian Signatures of Halo Bias
por: Abdelaziz, Mariam, et al.
Publicado: (2026)
por: Abdelaziz, Mariam, et al.
Publicado: (2026)
Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes
por: Freedman, Wendy L., et al.
Publicado: (2024)
por: Freedman, Wendy L., et al.
Publicado: (2024)
Radial Profiles of Radio Halos in Massive Galaxy Clusters: Diffuse Giants Over 2 Mpc
por: Rajpurohit, K., et al.
Publicado: (2025)
por: Rajpurohit, K., et al.
Publicado: (2025)
Ellipticities of Galaxy Cluster Halos from Halo-Shear-Shear Correlations
por: Liu, Zhenjie, et al.
Publicado: (2024)
por: Liu, Zhenjie, et al.
Publicado: (2024)
Universal Basic Mass Density inside Dark Matter Halos
por: Haddad, Fateen, et al.
Publicado: (2024)
por: Haddad, Fateen, et al.
Publicado: (2024)
Non-interacting holographic dark energy with Torsion via Hubble Radius
por: Yun, Yongjun, et al.
Publicado: (2025)
por: Yun, Yongjun, et al.
Publicado: (2025)
Signatures of Galactic Expansion in Gaia DR3: Implications for the JWST Early-Galaxy Puzzle
por: Karapetian, G. S., et al.
Publicado: (2025)
por: Karapetian, G. S., et al.
Publicado: (2025)
Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
por: Barua, Shubham, et al.
Publicado: (2025)
por: Barua, Shubham, et al.
Publicado: (2025)
Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
por: Bartlett, Deaglan J., et al.
Publicado: (2024)
por: Bartlett, Deaglan J., et al.
Publicado: (2024)
Constraints on Halo Gas Profiles from Joint kSZ and Galaxy Clustering Analysis of ACT DR6 and CMASS
por: Li, Shaohong, et al.
Publicado: (2026)
por: Li, Shaohong, et al.
Publicado: (2026)
A Correlation Between Black Hole Mass and Dark Matter Halo Concentration in Cosmological Simulations
por: Nino, John K.
Publicado: (2025)
por: Nino, John K.
Publicado: (2025)
Reconstruction of Dark Matter and Baryon Density From Galaxies: A Comparison of Linear, Halo Model and Machine Learning-Based Methods
por: Krywonos, Jordan, et al.
Publicado: (2025)
por: Krywonos, Jordan, et al.
Publicado: (2025)
Testing anisotropic Hubble expansion
por: Boubel, Paula, et al.
Publicado: (2024)
por: Boubel, Paula, et al.
Publicado: (2024)
Modified recombination and the Hubble tension
por: Mirpoorian, Seyed Hamidreza, et al.
Publicado: (2024)
por: Mirpoorian, Seyed Hamidreza, et al.
Publicado: (2024)
CMB Anomalies and the Hubble Tension
por: Giarè, William
Publicado: (2023)
por: Giarè, William
Publicado: (2023)
Galaxy Cluster Mass Estimation Through The Splashback Radius
por: Gabriel-Silva, Lucas, et al.
Publicado: (2025)
por: Gabriel-Silva, Lucas, et al.
Publicado: (2025)
Comparison of Halo Model and Simulation Predictions for Projected-Field Kinematic Sunyaev-Zel'dovich Cross-Correlations
por: Rodriguez, Michael Jacob, et al.
Publicado: (2025)
por: Rodriguez, Michael Jacob, et al.
Publicado: (2025)
Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
por: Burger, Pierre A., et al.
Publicado: (2024)
por: Burger, Pierre A., et al.
Publicado: (2024)
Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
por: Eroshenko, Yu. N., et al.
Publicado: (2024)
por: Eroshenko, Yu. N., et al.
Publicado: (2024)
On the Outskirts of Dark Matter Haloes
por: Chen, Alice, et al.
Publicado: (2022)
por: Chen, Alice, et al.
Publicado: (2022)
Ejemplares similares
-
Mass scaling relations for dark halos from an analytic universal outer density profile
por: Korkidis, Giorgos, et al.
Publicado: (2024) -
Turnaround radius of galaxy clusters in N-body simulations
por: Korkidis, Giorgos, et al.
Publicado: (2019) -
Searching for a signature of turnaround in galaxy clusters with convolutional neural networks
por: Triantafyllou, Nikolaos, et al.
Publicado: (2024) -
The Density Profile of Dynamical Halos
por: Shields, Tristen, et al.
Publicado: (2025) -
Halo Radius (Splashback Radius) of Groups and Clusters of Galaxies on small scales
por: Kopylova, Flera G., et al.
Publicado: (2024)