[PDF] Top 20 A model for cosmological simulations of galaxy formation physics: multi-epoch validation
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A model for cosmological simulations of galaxy formation physics: multi-epoch validation
... star formation rate weighted oxygen abundance in each galaxy, which places an emphasis on star-forming gas as is done through metallicity estimates via nebular emission ... See full document
23
A model for cosmological simulations of galaxy formation physics
... the galaxy velocity dispersion and the mass loading is inversely proportional to that (see also Murray et ...wind model, where the wind velocity is de- rived from the escape velocity of the host ... See full document
39
Guo, Qi (2009): Galaxy Formation and Evolution in a LCDM Universe. Dissertation, LMU München: Fakultät für Physik
... given epoch (see Cooray & Sheth 2002 for a review) but provides no nat- ural way to link populations at different epochs (see Conroy & Wechsler (2008) for a recent attempt to remedy ...follow galaxy ... See full document
141
Spatially Resolved Star Formation in Cosmological Zoom-in Simulations: Understanding the Role of Feedback in Scaling Relations
... star formation cycles in the fiducial model across ∼ dex in Σ g in the Kennicutt-Schmidt, depletion time—stability, and star formation rate—gas velocity dispersion ...the model exhibits ... See full document
187
Understanding Galaxy Formation and Evolution with Realistic Simulations
... high-resolution cosmological zoom-in simulations from the Feedback in Realistic Environments (FIRE) project, which include physically motivated models of the multi-phase ISM, star formation, ... See full document
282
A unified model for AGN feedback in cosmological simulations of structure formation
... numerical model for black hole growth and its associated feedback pro- cesses that for the first time allows cosmological simulations of structure formation to self-consistently follow the ... See full document
28
Sijacki, Debora (2007): Non gravitational heating mechanisms in galaxy clusters. Dissertation, LMU München: Fakultät für Physik
... the formation and growth of cosmic structures is one of the most fascinat- ing and challenging fields of ...favoured cosmological model, the so-called ΛCDM cosmogony, dark matter structures grow ... See full document
160
Sawala, Till (2011): Simulations of Dwarf Galaxy Formation. Dissertation, LMU München: Fakultät für Physik
... we model the formation and evolution of dwarf galaxies in fully cosmological, smoothed particle hydrodynamical (SPH) ...a cosmological volume with periodic boundary conditions, in which the ... See full document
172
Galaxy formation near the epoch of reionization
... of cosmological initial conditions and collisionless evolution of structure formation through to the present, aimed at understanding the resulting properties of a metal-poor GCS formed under our ...Way-like ... See full document
207
How a Minimum Time Step and Formation of Initial Causal Structure in Space Time Is Linked to an Enormous Initial Cosmological Constant
... to formation of entropy, i.e. if Λ is an invariant cosmological “constant” and if Equation (10) holds, we can use the existence of nonzero initial entropy as the formation point of an ar- row of ... See full document
8
Sussing merger trees: the impact of halo merger trees on galaxy properties in a semi analytic model
... semi-analytic model for galaxy formation and ...numerical simulations of structure formation is non-trivial; different tree building algorithms can give differing merger ... See full document
14
Radio Galaxy Zoo: cosmological alignment of radio sources
... Both observational results (e.g. Tempel & Libeskind 2013; Zhang et al. 2013; Hirv et al. 2017) and tidal torque analytical models (e.g. Lee 2004; Codis, Pichon & Pogosyan 2015) suggest the alignment of ... See full document
11
How a Minimum Time Step and Formation of Initial Causal Structure in Space Time Is Linked to an Enormous Initial Cosmological Constant
... and Formation of Initial Causal Structure in Space-Time Is Linked to an Enormous Initial Cosmological ...Energy Physics, Gravitation and Cosmology, 4, ... See full document
8
Multi-Physics based Simulations of a Shock Absorber Sub-System
... to model a two chamber shock absorber in multi-physics ...AMESim model narrates standard shock absorber (OLEO Pneumatic) that can be modeled using Hydraulic Component Design ... See full document
7
On the influence of model physics on simulations of Arctic and Antarctic sea ice
... (1983–2007) simulations are per- formed with the global, ocean-sea ice models NEMO-LIM2 and NEMO-LIM3 driven by atmospheric reanalyses and cli- ...two simulations differ only in their sea ice component, ... See full document
13
Mad About Modern Physics Braintwisters, Paradoxes, and Curiosities pdf
... conventional physics arise: (1) If Newtonian gravitation and Kepler’s laws apply, they would dictate a decrease in star veloc- ity with increasing radius from the galactic nucleus, like the planets of the Solar ... See full document
311
Three-Dimensional Multi-Physics CFD Simulations of Sand Transfer around a Cube
... The number of sand particles in a desert is infinite. If all sand particles are traced, we must spend a huge amount of time for simulations. Thus, in the present study sand particles are treated as a lump ... See full document
6
Hubble’s Constant
... Bang cosmological model [3] [4] is its statement that the Cosmos began at some definite past time; in such a way that the expansion rate determines the age of the ... See full document
5
Physics in Discrete Spaces: On Some Cosmological Issues
... This article is an application of the theory of discrete spaces to cosmology. Its conclusions are necessarily speculative. An interesting aspect is that it gives possible solutions to many pending problems within a ... See full document
11
Accelerated cosmological expansion without tension in the Hubble parameter - Fast evolution of the Hubble parameter H(z)
... unchanged. By volume, weak gravity makes up most of the Universe. If inertia falls below its New- tonian value in weak gravity, then possibly the Hubble expansion is faster than what is expected in ΛCDM. For this reason, ... See full document
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