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"Hamburan K+p dihitung dengan menggunakan kinematika relativik. Model potensial yang digunakan digambarkan sebagai model pertukaran meson dan hiperon. Penampang lintang differensial dan besaran-besaran spin dihitung. Perhitungan dibandingkan dengan yang menggunakan kinematika nonrelativistik untuk melihat efek relativistik pada energi bervariasi.

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Scattering of K+p is calculated using relativistic kinematics. The Model used is described as a potential model for meson and hiperon. Differential cross section and spin observables calculated. The calculations are compared with using non relativistics to see relativistic effects on energy range."

"Hamburan K−n dihitung dengan menggunakan teknik 3D yang dibandingkan dengan perhitungan partial wave untuk memecahkan persamaan Lippmann-Schwinger untuk matriks T. Interaksi yang dipakai melibatkan pertukaran meson dan hyperon sampai orde kedua. Perhitungan dibandingkan dengan yang menggunakan kinematika relativistik untuk melihat efek relativistik pada energi bervariasi. Besaran spin yang dihitung adalah penampang lintang diferensial, polarisasi, dan depolarisasi.

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Scattering of K−n is calculated using 3D technique which then is compared with the partial wave calculations to solve the Lippmann-Schwinger equation for matrix T. The interaction being used involves the exchange of mesons and hyperon up to second order. The calculations are compared with those using relativistic kinematics to see relativistic effects on various energies. The spin observables are differential cross section, polarization and depolarization."

"Hamburan K+p dimodelkan sebagai pertukaran satu hadron. Hadron yang dipertukarkan berupa meson skalar σ; meson vektor ρ dan ω; hyperon Λ dan Σ; dan resonans Σ∗ (1385). Besaran yang dihitung adalah spin-averaged differential cross section yang dihitung menggunakan kinematika relativistik serta menggunakan teknik tiga dimensi sehingga tanpa ekspansi gelombang parsial. Penelitian dilakukan untuk melihat kontribusi suku rescattering pada hamburan K+p. Kontribusi suku rescattering dengan melibatkan semua pertukaran partikel dihitung pada energi 700 MeV - 3400 MeV. Kemudian, kontribusi suku rescattering untuk tiap pertukaran partikel dihitung pada energi 700 MeV - 2200 MeV dan energi 5 GeV - 10 GeV.

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K+p scattering is modeled as one-hadron exchange. The hadrons being exchanged are scalar meson σ; vector meson ρ and ω; hyperon Λ and Σ; and resonance Σ∗ (1385). Spin-averaged differential cross section is calculated using relativistic kinematics and three-dimensional technique thus without partial wave expansion. The research was conducted to see the contributions of rescattering terms on K+p scattering. Rescattering terms contributions involving all exchanged particles are calculated for energies 700 MeV - 3400 MeV. Furthermore, rescattering terms contributions for each exchanged particles are calculated for energies 700 MeV - 2200 MeV and energies 5 GeV - 10 GeV."

"Hamburan K⁺n dihitung dalam basis ruang momentum tiga dimensi (3D). Sebagai input digunakan interaksi yang dijabarkan sebagai pertukaran meson dan hiperon antar kaon dan nukleon. Dua tipe perhitungan dikerjakan, tipe satu menggunakan kinematika nonrelativistik dan tipe dua memakai kinematika relativistik. Perhitungan tipe dua dibandingkan terhadap perhitungan tipe satu untuk melihat efek relativistik pada energi yang bervariasi.

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K+n scattering is calculated in three-dimensional (3D) momentum space basis. As input interaction described as meson and hyperon exchange between kaon and nucleon is taken. Two types of calculations are carried out, type one uses nonrelativistic kinematics and type two takes relativistic kinematics. Calculations of type two are compared to those of type one to see some relativistic effects at various energies."

"[ABSTRAKFenomena halo neutron dalam nuklir digambarkan adanya kemunculan 'ekor' danadanya 'ruang kosong' antara core dan ekor pada distribusi neutron akibat energiikat yang lemah. Metode analisa halo yang dikembangkan oleh V. Rotival dkk [Phys.Rev. C79, 054308 (2009)] untuk menghitung besaran-besaran halo berdasarkan mo-del Hartree-Fock-Bogoulibov (HFB) pada isotop Cr dan isotop Sn menjadi salah sa-tu alternatif untuk mempelajari fenomena halo. Berbeda dengan Rotival dkk, kamimenggunakan model Relativistic Mean Field (RMF) pada penelitian ini. Berbedadengan hasil perhitungan berdasarkan model HFB, kami fokus mengamati perilakuspektrum single particle energy level 1g9~2 terhadap kemunculan halo pada isotopCr. Selain itu, pada penelitian ini kami juga memperlajari dampak dari suku crosscoupling meson ! − , suku-suku tensor dan suku pertukaran elektromagnetik padamodel RMF terhadap kemunculan halo pada isotop Cr dan isotop Sn. Hasil perhi-tungan prediksi kemunculan halo berdasarkan model RMF lebih besar dibandingkandengan hasil perhitungan berdasarkan model HFB (`NhaloeRMF > `NhaloeHFB):

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ABSTRACTIn neutron halo phenomenon, the neutron density displays an unusually extended'tail' and 'empty space' between the core and the tail due to weak binding energy.New analysis method of the halo was developed by V. Rotival, et al.[Phys. Rev. C79,054308 (2009)] in Cr-isotopes and Sn-isotopes, its usually applied with Hartree-Fock-Bogoliubov (HFB) model. Unlike them, we use the model of the Relativistic MeanField (RMF) in this research. We observed dierent behavior at the level 1g9~2 in linewith appearance of halo in Cr-isotopes. Moreover, in this research we also studiedthe eects of cross coupling meson ! − , tensor, and electromagnetic exchange inRMF model appearance of halo in Cr-isotopes and Sn-isotopes. The prediction ofthe existence of halo based on RMF model is greater than the prediction based onHFB model (`NhaloeRMF > `NhaloeHFB):, In neutron halo phenomenon, the neutron density displays an unusually extended'tail' and 'empty space' between the core and the tail due to weak binding energy.New analysis method of the halo was developed by V. Rotival, et al.[Phys. Rev. C79,054308 (2009)] in Cr-isotopes and Sn-isotopes, its usually applied with Hartree-Fock-Bogoliubov (HFB) model. Unlike them, we use the model of the Relativistic MeanField (RMF) in this research. We observed dierent behavior at the level 1g9~2 in linewith appearance of halo in Cr-isotopes. Moreover, in this research we also studiedthe eects of cross coupling meson ! − , tensor, and electromagnetic exchange inRMF model appearance of halo in Cr-isotopes and Sn-isotopes. The prediction ofthe existence of halo based on RMF model is greater than the prediction based onHFB model (`NhaloeRMF > `NhaloeHFB):]"

"Hamburan kaon-nukleon diformulasikan dalam basis momentum-spin tiga dimensi. Interaksi yang dipakai berdasarkan model potensial Yukawa dengan faktor spin-orbit. Dalam penelitian ini, kami memasukkan unsur kinematika relativistik ke dalam hamburan, dan kemudian menyelidiki efek relativistik pada hamburan kaon-nukleon untuk nilai energi yang bervariasi.

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Kaon-nucleon scattering is formulated in three-dimensional momentum-spin basis. The interaction being used is based on Yukawa potential model with spin-orbit factor. In this research, we use relativistic kinematics into scattering, and then invistigate some relativistic effects on kaon-nucleon scattering for varies energy."

"[ABSTRAKPrediksi dari posisi proton dan neutron dripline dipelajari dalam model ModiedRelativistic Mean Field (MRMF) menggunakan tujuh buah variasi parameter set.Posisi proton dan neutron dripline diprediksi dengan menggunakan energi separasidan energi partikel tunggal. Dalam model MRMF ini, dapat dilihat pengaruhkopling isovektor-isoskalar, tensor dan electromagnetic exchange terhadap prediksiproton dan neutron dripline. Hasil perhitungan menunjukkan bahwa prediksi protondripline pada isoton N = 28 tidak dipengaruhi oleh ketiga faktor tersebut. Selainitu, proton dripline pada isoton N = 28 tidak memiliki korelasi yang kuat terhadapsifat bulk inti. Prediksi neutron dripline pada isotop Ca dan isotop Pb dipengaruhioleh ketiga faktor tersebut yang ditandai dengan berbedanya prediksi pada setiapvariasi parameter set. Neutron dripline pada isotop Ca memiliki korelasi yang kuatterhadap skin. Namun, pada isotop Pb tidak terlihat korelasi yang kuat terhadapskin. Pada daerah superheavy, isoton N = 258 memiliki hasil prediksi proton driplineyang dipengaruhi oleh ketiga faktor, terutama tensor dan electromagnetic exchange,serta memiliki korelasi yang kuat terhadap skin, jari-jari muatan, dan ketebalanpermukaan.

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ABSTRACTStudy of prediction of proton and neutron dripline in Modied Relativistic Mean Field(MRMF) model using seven variations of parameter set. The position of protonand neutron dripline predicted use energy separation and energy single particle method.In this MRMF model, can be seen the eects of coupling isovector-isoscalar,tensors, and electromagnetic exchange on prediction of proton and neutron dripline.The result of these calculation show that prediction of proton dripline in isotone N= 28 not inuenced by all these factors. Moreover, proton dripline in isotone N = 28do not have a strong correlation with nucleus bulk properties. Prediction of neutrondripline in isotope Ca and isotope Pb inuenced by all these factors characterizedby dierent predictions on each variations of parameter set. Neutron dripline atisotope Ca have a strong correlation with skin. However, at isotope Pb does notlook strong correlation with skin. In the superheavy region, isotone N = 258 hasthe predicted outcome of protons which is inuenced by all these factors, notablytensors and electromagnetic exchange and having a strong correlation with skin,charge radius, and surface thickness., Study of prediction of proton and neutron dripline in Modied Relativistic Mean Field(MRMF) model using seven variations of parameter set. The position of protonand neutron dripline predicted use energy separation and energy single particle method.In this MRMF model, can be seen the eects of coupling isovector-isoscalar,tensors, and electromagnetic exchange on prediction of proton and neutron dripline.The result of these calculation show that prediction of proton dripline in isotone N= 28 not inuenced by all these factors. Moreover, proton dripline in isotone N = 28do not have a strong correlation with nucleus bulk properties. Prediction of neutrondripline in isotope Ca and isotope Pb inuenced by all these factors characterizedby dierent predictions on each variations of parameter set. Neutron dripline atisotope Ca have a strong correlation with skin. However, at isotope Pb does notlook strong correlation with skin. In the superheavy region, isotone N = 258 hasthe predicted outcome of protons which is inuenced by all these factors, notablytensors and electromagnetic exchange and having a strong correlation with skin,charge radius, and surface thickness.]"