Titlebook: Discoveries at the Frontiers of Science; From Nuclear Astroph Johannes Kirsch,Stefan Schramm,Horst St?cker Book 2020 Springer Nature Switze

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What the Azimuthal Distribution of Heavy Mesons Tells Us About the Quark Gluon Plasma?,o a statistical equilibrium latest at the end of the QGP expansion and do therefore not carry information on the QGP properties during the expansion. We discuss here the interaction of the heavy quarks with the QGP partons and how this interaction influences the azimuthal distribution of the heavy m

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The Physics Case for the FAIR/NICA Energy Region,y. A transition from a baryon dominated to a meson dominated final state takes place around this beam energy. Ratios of strange particles to mesons show clear and pronounced maxima around this beam energy. The theoretical interpretation can be clarified by covering fully this energy region. In parti

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Quark Matter in Neutron Stars,ansition is modeled using both the Maxwell construction and the Gibbs construction. For the Maxwell construction, we find that all NSs with core densities beyond the phase transition density are unstable. Therefore, no quark matter cores would exist inside such NSs. The situation is drastically diff

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Binary Compact Star Mergers and the Phase Diagram of Quantum Chromodynamics,e Goethe University Frankfurt in 1990. During this time Walter Greiner gave his legendary 5-semester course on theoretical physics and I had the fortune to be able to attend his first lecture on .. Greiner’s fashion and manner of presenting the philosophical and mathematical backgrounds of theoretic

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,Generic Theory of Geometrodynamics from Noether’s Theorem for the , Symmetry Group,d spin-1 particles. Actually, we present a Hamilton–Lagrange–Noether formulation of the gauge theory of gravitation. It is based on the minimum set of postulates to be introduced, namely (i) the action principle and (ii) the form-invariance of the action under the (local) diffeomorphism group. The s