scholarly journals Ground-State Properties of Mg Isotopes in and Beyond the Island of Inversion through Reaction Cross Sections

2015 ◽  
Author(s):  
Shin Watanabe ◽  
Kosho Minomo ◽  
Mitsuhiro Shimada ◽  
Shingo Tagami ◽  
Masaaki Kimura ◽  
...  
Keyword(s):  
Cross Sections ◽  
Ground State ◽  
Reaction Cross ◽  
Island Of Inversion ◽  
Ground State Properties ◽  
Mg Isotopes ◽  
Reaction Cross Sections

QUASI-CLASSICAL TRAJECTORY STUDY OF THE REACTION PROBABILITY AND CROSS SECTION OF THE REACTION LiH + H

2013 ◽  
Vol 12 (01) ◽  
pp. 1250093 ◽  
Author(s):  
YULIANG WANG ◽  
JINCHUN ZHANG ◽  
BAOGUO TIAN ◽  
KUN WANG ◽  
XIAORUI LIANG ◽  
...  
Keyword(s):  
Cross Section ◽  
Cross Sections ◽  
Ground State ◽  
Collision Energy ◽  
Energy Surface ◽  
Classical Trajectory ◽  
Reaction Cross ◽  
Reaction Probability ◽  
Title Reaction ◽  
Reaction Cross Sections

Based on the new accurate potential energy surface of the ground state of LiH2 system. Quasi-classical trajectory (QCT) calculations were carried out for the reaction LiH + H . The reaction probability of the title reaction for J = 0 has been calculated. The reaction cross sections were calculated as functions of the collision energy in the range 0.1–2.5 eV. The results were found to be well consistent with the previous real wave packet (RWP) and QCT results.

A Search for Isotope Effects in Chemiluminescent Reactions of Metastable Ca*( 3Pj, 1D2 ) Atoms with CH3I and CD3I Molecules

1999 ◽  
Vol 54 (3-4) ◽  
pp. 191-194 ◽  
Author(s):  
B. Pranszke ◽  
P. Kierzkowski ◽  
A. Kowalski
Keyword(s):  
Cross Sections ◽  
Ground State ◽  
Isotope Effects ◽  
Reaction Cross ◽  
Isotopic Substitution ◽  
Methyl Group ◽  
Total Collision ◽  
Reaction Cross Sections

Chemiluminescent reactions of calcium atoms in the metastable 3Pj and 1D2 states with CH3I and CD3I were studied in a beam-gas arrangement. Calcium monoiodide spectra associated with transitions from the electronic A 2Π, B 2Σ+ and C 2Π states to the X 2Σ+ ground state were recorded. Total collision and chemiluminescence cross sections were measured. It was found that isotopic substitution in the methyl group does not change the reaction cross sections and the chemiluminescence spectra.

scholarly journals Density distributions, form factors and reaction cross sections for exotic 11Be and 15C nuclei

2019 ◽  
Vol 12 (24) ◽  
pp. 10-24
Author(s):  
Ahmed N. Abdullah
Keyword(s):  
Cross Sections ◽  
Single Particle ◽  
Ground State ◽  
Form Factors ◽  
Reaction Cross ◽  
Exotic Nuclei ◽  
Wave Functions ◽  
Proton Form ◽  
Proton Form Factors ◽  
Reaction Cross Sections

The ground state proton, neutron and matter densities of exotic 11Be and 15C nuclei are studied by means of the TFSM and BCM. In TFSM, the calculations are based on using different model spaces for the core and the valence (halo) neutron. Besides single particle harmonic oscillator wave functions are employed with two different size parameters  Bc and Bv.  In BCM, the halo nucleus is considered as a composite projectile consisting of core and valence clusters bounded in a state of relative motion. The internal densities of the clusters are described by single particle Gaussian wave functions.  Elastic electron scattering proton form factors for these exotic nuclei are analyzed via the plane wave born approximation (PWBA). As the calculations in the BCM do not distinguish between protons and neutrons, the calculations of the proton form factors are restricted only by the TFSM. The reaction cross sections for these exotic nuclei are studied by means of the Glauber model with an optical limit approximation using the ground state densities of the projectile and target, where these densities are described by single Gaussian functions. The calculated reaction cross sections at high energy are in agreement with the experimental data.

scholarly journals New candidate for deformed halo nucleus in Mg isotopes through analysis of reaction cross sections

2014 ◽  
Vol 66 ◽  
pp. 03095 ◽  
Author(s):  
S. Watanabe ◽  
K. Minomo ◽  
S. Tagami ◽  
M. Shimada ◽  
M. Kimura ◽  
...  
Keyword(s):  
Cross Sections ◽  
Halo Nucleus ◽  
Reaction Cross ◽  
Mg Isotopes ◽  
Reaction Cross Sections

Calculation the Cross Sections for 6Li(α,p)9Be Reaction by Reverse Reaction

2014 ◽  
Vol 4 (2) ◽  
pp. 546-554
Author(s):  
Firas Mahmood Hady
Keyword(s):  
Cross Sections ◽  
Alpha Particle ◽  
Ground State ◽  
Proton Energy ◽  
High Probability ◽  
Threshold Energy ◽  
Reaction Cross ◽  
Light Elements ◽  
Q Value ◽  
Reaction Cross Sections

In this study light elements 6Li , 9Be , 10Be for 6Li(α , p)9Be reaction with proton energy from ( 27.5) MeV to ( 67.5 ) MeVwith threshold energy (2.3626) MeV are used according to the available data of reaction cross sections. The Q-value isequale (2.125MeV) and parity of ( 9Be =3/2+) ,(B =3+) and (Li = 1+) for the ground state .The more recent cross sectionsdata of 6Li(α,p)9Be reaction is reproduced in fine steps and by using (Matlab-7.6-2008a) program and get the equationfrom 3-degree for plotted. We deduced that the high probability to produced 9Be by bombard 6Li by alpha particle

Formation of α clusters in dilute neutron-rich matter

Science ◽  
2021 ◽  
Vol 371 (6526) ◽  
pp. 260-264 ◽  
Author(s):  
Junki Tanaka ◽  
Zaihong Yang ◽  
Stefan Typel ◽  
Satoshi Adachi ◽  
Shiwei Bai ◽  
...  
Keyword(s):  
Cross Sections ◽  
Cluster Formation ◽  
Reaction Cross ◽  
Skin Thickness ◽  
Neutron Skin ◽  
Heavy Nuclei ◽  
Α Decay ◽  
Neutron Skin Thickness ◽  
Reaction Cross Sections ◽  
Α Particles

The surface of neutron-rich heavy nuclei, with a neutron skin created by excess neutrons, provides an important terrestrial model system to study dilute neutron-rich matter. By using quasi-free α cluster–knockout reactions, we obtained direct experimental evidence for the formation of α clusters at the surface of neutron-rich tin isotopes. The observed monotonous decrease of the reaction cross sections with increasing mass number, in excellent agreement with the theoretical prediction, implies a tight interplay between α-cluster formation and the neutron skin. This result, in turn, calls for a revision of the correlation between the neutron-skin thickness and the density dependence of the symmetry energy, which is essential for understanding neutron stars. Our result also provides a natural explanation for the origin of α particles in α decay.

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