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"This second volume follows the successful Lect. Notes Phys. 818 (Vol.1), and comprises six extensive lectures covering the following topics, microscopic cluster models, neutron halo and break-up reactions, break-up reaction models for two- and three-cluster projectiles, clustering effects within the di-nuclear model, nuclear alpha-particle condensates, and clusters in nuclei: experimental perspectives."

"This book brings together various aspects of the nuclear fission phenomenon discovered by Hahn, Strassmann and Meitner almost 70 years ago. Beginning with an historical introduction the authors present various models to describe the fission process of hot nuclei as well as the spontaneous fission of cold nuclei and their isomers. The role of transport coefficients, like inertia and friction in fission dynamics is discussed. The effect of the nuclear shell structure on the fission probability and the mass and kinetic energy distributions of the fission fragments is presented. The fusion-fission process leading to the synthesis of new isotopes including super-heavy elements is described."

"Keberadaan partikel hyperon di dalam bintang neutron diteliti dengan menggunakan model medan rata-rata relativistik. Dengan mengasumsikan adanya hyperon di dalam bintang neutron akan berdampak kepada persamaan keadaan dan sifat-sifat bintang neutron seperti jari-jari, massa, transisi fase dan lain-lain. Pada kajian ini akan dibahas bagaimana pengaruh konstanta kopling 𝜍∗ meson terhadap persamaan keadaan bintang neutron dan bagaimana pengaruhnya terhadap transisi fase bintang neutron untuk tekanan yang anisotropik dengan menggunakan model medan rata-rata relativistik dan parameter set BSP yang kemudian dikomparasikan dengan parameter set GM1. Diperoleh hasil dengan memvariasikan konstanta kopling 𝑔𝜍∗Λ 𝑔𝜍𝑁 berdampak kepada persamaan keadaan bintang neutron dan hubungan massa dan jari-jari bintang neutron.

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The existence hyperon in neutron stars has been studied by using relativistic mean field model. By assuming the hyperon in neutron stars will affect the equation of state and properties of neutron stars such as radius, mass, phase transitions, and others. In this study, we will discuss how 𝜍∗ meson coupling constant affecting equation of state and phase transition in neutron stars for anisotropic pressure by using relativistic mean field model and BSP parameter set which later will be compared with GM1 parameter set. It can be seen that by varying 𝑔𝜍 ∗Λ/𝑔𝜍𝑁 coupling constant affecting the equation of state and mass-radius relation of neutron stars."

"To achieve this goal, the present text concentrates mainly on equilibrium thermodynamics, first, the fundamental ideas of strong interaction thermodynamics are introduced and then the main concepts and methods used in the study of the physics of complex systems are summarized. Subsequently, simplified phenomenological pictures, leading to critical behavior in hadronic matter and to hadron-quark phase transitions are introduced, followed by elements of finite-temperature lattice QCD leading to the important results obtained in computer simulation studies of the lattice approach. Next, the relation of the resulting critical behavior to symmetry breaking/restoration in QCD is clarified before the text turns to the study of the QCD phase diagram. The presentation of bulk equilibrium thermodynamics is completed by studying the properties of the quark-gluon plasma as new state of strongly interacting matter. The final chapters of the book are devoted to more specific topics which arise when nuclear collisions are considered as a tool for the experimental study of QCD thermodynamics."