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Free Evolution
As we mentioned in the previous chapter, the “free evolution” approach is by far the most commonly used today in Numerical Relativity codes. It...
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Stellar Evolution
In principle, there are the following stages in stellar evolution:...
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Stellar Evolution
This chapter includes the work done for the Nobel Prizes awarded to S. Chandrasekhar and W. A. Fowler in 1983.Their work relates to stellar...
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Long-Term Evolution of the Saturnian System
Here we present the current state of knowledge on the long-term evolution of Saturn’s moon system due to tides within Saturn. First we provide some...
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Colour evolution and infrared physics
We give a complete account of how soft gluon, massless quark, evolution equations in colour space originate, from a factorization into a hard cross...
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Stellar Evolution, SN Explosion, and Nucleosynthesis
Massive stars evolve toward the catastrophic collapse of their innermost core, producing core-collapse supernova (SN) explosions as the end products....
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Dynamical evolution of spinodal decomposition in holographic superfluids
We study the nonlinear dynamical evolution of spinodal decomposition in a first-order superfluid phase transition using a simple holographic model in...
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Galaxy Evolution in Mass-Selected Samples
I summarize the recent results from the HDFS and K20 surveys that allow to trace the evolution of massive galaxies up to z≃ 3. I show that the...
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Quantum speed of evolution of neutral mesons
We investigate the quantum-mechanical time-evolution speed limit for neutral K and B mesons, both single as well as correlated, within the framework...
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The Evolution of Evolved Galaxies
The plethora of high redshift multifrequency surveys currently under way, that were extensively illustrated at this meeting will shortly provide us...
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The Size Evolution of High-Redshift Galaxies
It is appropriate in a conference on the growth of galaxies to examine what we know about the evolution of galaxy sizes. Quantifying galaxy size...
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Darwinian Evolution, Hypercycles and Game Theory
Adaptation and evolution are quasi synonymous in popular language, it is hence little surprising that the theory of Darwinian evolution is infused...
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Evolution und Emergenz
Im Jahr 1900 ist viel los. Erst stellt Max Planck in Berlin sein Quantum der Wirkung vor, das mit Sicherheit eine minimale Größe hat – kleiner kann...
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The Near-Infrared View of Galaxy Evolution
Near-infrared surveys provide one of the best opportunities to investigate the cosmic evolution of galaxies and their mass assembly. We briefly...
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Multi-collinear splitting kernels for track function evolution
Jets and their substructure play a central role in many analyses at the Large Hadron Collider (LHC). To improve the precision of measurements, as...
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Evolution of colour correlated double parton distributions: a quantitative study
Double parton distributions satisfy the same evolution equations as ordinary single-parton densities, provided that the colours of the two partons...
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Volcanic and Tectonic Constraints on the Evolution of Venus
Surface geologic features form a detailed record of Venus’ evolution. Venus displays a profusion of volcanic and tectonics features, including both...
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The Galaxy Evolution Explorer (GALEX)
The Galaxy Evolution Explorer (GALEX) is a Space Ultraviolet Imaging and Spectroscopic Survey Small Explorer mission that will map the star formation...
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Scaling and Evolution of Stellar Magnetic Activity
Magnetic activity is a ubiquitous feature of stars with convective outer layers, with implications from stellar evolution to planetary atmospheres....
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Evolution of Heterogeneous Systems
In this chapter we apply the ideas and methods developed in previous chapters to the dynamics of heterogeneous systems and obtain the celebrated...