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"ABSTRAKParameter isoskalar SNM dan parameter isovektor PNM dari berbagai nilai radiusnukleon serta efek fitting pada prediksi daerah medium density dan low densityPNM, dengan menggunakan nilai b = 0:0005 dan b = 0:01 serta radius nukleon0, 0.66 fm, 0.76 fm, 0.83 fm, dan 0.99 fm telah berhasil diperoleh. Parameterisoskalar hasil fit menghasilkan nilai yang cocok dengan perhitungan DBHFuntuk semua radius nukleon yang digunakan, kecuali untuk radius 0.99 fm yangtidak memenuhi prediksi EOS SNM, menurut hasil eksperimen tumbukan ionberat. Sementara itu, efek fitting untuk parameter-parameter di luar daerah fittingwindow tidak sesuai dengan jangkauan eksperimen dari Danielewicz, dkk. Halini kemungkinan diakibatkan oleh keterbatasan jangkauan parameter, nilai b, danradius nukleon yang digunakan.

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ABSTRAKThe isoscalar parameter of SNM and isovector parameter of PNM from variousnucleon size as well as the effects of fitting on medium density and low densityprediction area of PNM have been investigated. To this end, we have chosen cutoffparameter b = 0:0005 and b = 0:01, with the nucleon radius of 0, 0.66, 0.76,0.83, and 0.99 fm. The obtained isoscalar parameters lead to a good agreement withthe result of the DBHF calculation for all nucleon radii used, except for rN = 0:99fm, which does not fulfill the SNM EOS prediction based on the results of heavyion collision. On the other hands, the effect of fitting by means of the parametersoutside the upper and lower bounds does not agree with the experimental result ofDanielwicz et al. It is suspected that this could happen due to the limitation of theparameter range, b, as well as the nucleon radius us"

"The book provides theoretical and phenomenological insights on the structure of matter, presenting concepts and features of elementary particle physics and fundamental aspects of nuclear physics.Starting with the basics (nomenclature, classification, acceleration techniques, detection of elementary particles), the properties of fundamental interactions (electromagnetic, weak and strong) are introduced with a mathematical formalism suited to undergraduate students. Some experimental results (the discovery of neutral currents and of the W± and Z0 bosons. The quark structure observed using deep inelastic scattering experiments) show the necessity of an evolution of the formalism. This motivates a more detailed description of the weak and strong interactions, of the Standard Model of the microcosm with its experimental tests, and of the Higgs mechanism. The open problems in the Standard Model of the microcosm and macrocosm are presented at the end of the book. For example, the CP violation currently measured does not explain the matter -antimatter asymmetry of the observable universe. The neutrino oscillations and the estimated amount of cosmological dark matter seem to require new physics beyond the standard model. A list of other introductory texts, work reviews and some specialized publications is reported in the bibliography."

"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."