Imagen de Portada

Dianoga SIDM: galaxy cluster self-interacting dark matter simulations

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Ragagnin, Antonio, Meneghetti, Massimo, Calura, Francesco, Despali, Giulia, Dolag, Klaus, Fischer, Moritz S., Giocoli, Carlo, Moscardini, Lauro
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Physics - Phenomenology
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
por: Despali, Giulia, et al.
Publicado: (2025)

The AIDA-TNG project. Abundance, radial distribution, and clustering properties of halos in alternative dark matter models
por: Romanello, Massimiliano, et al.
Publicado: (2025)

The Three Hundred: $M_{sub}-V_{circ}$ relation
por: Srivastava, Atulit, et al.
Publicado: (2023)

Accurately simulating core-collapse self-interacting dark matter halos
por: Fischer, Moritz S., et al.
Publicado: (2025)

Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions
por: Fischer, Moritz S., et al.
Publicado: (2023)

The Three Hundred Project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models
por: Giocoli, Carlo, et al.
Publicado: (2025)

Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
por: Fischer, Moritz S., et al.
Publicado: (2024)

Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
por: Despali, Giulia, et al.
Publicado: (2025)

SHH method for SIDM: An SIDM-hydro hybrid method for simulating self-interacting dark matter
por: Schon, Sarah, et al.
Publicado: (2025)

N-body simulations of dark matter-baryon interactions
por: Fischer, Moritz S., et al.
Publicado: (2025)

Properties of the diffuse gas component in filaments detected in the Dianoga cosmological simulations
por: Ilc, Samo, et al.
Publicado: (2024)

AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
por: Trobbiani, Leonardo, et al.
Publicado: (2025)

Merge and strip: dark matter-free dwarf galaxies in clusters can be formed by galaxy mergers
por: Ivleva, Anna, et al.
Publicado: (2024)

To collapse or not to collapse: Halo evolution with self-interacting dark matter mass segregation
por: Patil, Yashraj, et al.
Publicado: (2025)

Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures
por: Maggiore, Leonardo, et al.
Publicado: (2025)

Image simulations of highly magnified clumpy galaxies
por: Mini, Irene, et al.
Publicado: (2025)

DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
por: Harvey, David, et al.
Publicado: (2025)

SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales
por: Ando, Shin'ichiro, et al.
Publicado: (2024)

Galaxy-galaxy strong lensing cross-section with fuzzy dark matter model
por: Kawai, Hiroki, et al.
Publicado: (2024)

The dynamical evolution of the stellar clumps in the Sparkler galaxy
por: Giunchi, Eric, et al.
Publicado: (2025)

Interstellar dust production, destruction and effects of dust depletion in galaxies
por: Calura, Francesco
Publicado: (2025)

The AIDA-TNG project: gas distributions inside and around haloes
por: Zhang, Chi, et al.
Publicado: (2026)

Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations
por: Rihtaršič, Gregor, et al.
Publicado: (2023)

Self-interacting dark matter in the center of a Local Group dwarf galaxy and its satellites
por: Gutcke, Thales A., et al.
Publicado: (2025)

Accretion of self-interacting dark matter onto supermassive black holes
por: Sabarish, V. M., et al.
Publicado: (2025)

Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
por: Straight, Maria C., et al.
Publicado: (2025)

New applications of Graph Neural Networks in Cosmology
por: Farsian, Farida, et al.
Publicado: (2022)

On the tomographic cluster clustering as a cosmological probe
por: Romanello, Massimiliano, et al.
Publicado: (2024)

Multiple stellar population mass loss in massive Galactic globular clusters
por: Lacchin, Elena, et al.
Publicado: (2023)

AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
por: Giocoli, Carlo, et al.
Publicado: (2024)

Simulating realistic self-interacting dark matter models including small and large-angle scattering
por: Arido, Cenanda, et al.
Publicado: (2024)

Testing the isothermal Jeans model for self-interacting dark matter halos in the collapse phase
por: Li, Shubo, et al.
Publicado: (2026)

SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
por: Calura, F., et al.
Publicado: (2024)

The large cores of dark matter and globular clusters in AS1063. Possible evidence of self-interacting dark matter. Or not
por: Diego, Jose M.
Publicado: (2026)

The AIDA-TNG project: 3D halo shapes
por: Giocoli, C., et al.
Publicado: (2025)

Simulations of galaxy cluster mergers with velocity-dependent, rare and frequent self-interactions
por: Sabarish, V. M., et al.
Publicado: (2023)

The full iron budget in simulated galaxy clusters: The chemistry between gas and stars
por: Biffi, Veronica, et al.
Publicado: (2025)

How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
por: Villalba, Justo Antonio Gonzalez, et al.
Publicado: (2024)

Leo I: the classical dwarf spheroidal galaxy with the highest dark-matter density
por: Pascale, R., et al.
Publicado: (2025)

Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
por: Caro, Andrés, et al.
Publicado: (2024)