β -Delayed One and Two Neutron Emission Probabilities Southeast of Sn132 and the Odd-Even Systematics in

V. H. Phong¹,

S. Nishimura²,

G. Lorusso³

et al.

Abstract

math xmlns="http://www.w3.org/1998/Math/MathML" display="inline">mi>β/mi>/math>-Delayed One and Two Neutron Emission Probabilities Southeast of math xmlns="http://www.w3.org/1998/Math/MathML" display="inline">mrow>mmultiscripts>mrow>mi>Sn/mi>/ mrow>mprescripts>/mprescripts>none>/none>mrow>mn >132/mn>/mrow>/mmultiscripts>/mrow>/math> and the Odd-Even Systematics in math xmlns="http://www.w3.org/1998/Math/MathML" display="inline">mi>r/mi>/math>-Process Nuclide Abundances V. H. Phong et al.

Further monopole effects in neutron-rich Sb isotopes*

“…The rapid neutron-capture process (r-process) is responsible for approximately half of the elements heavier than Fe in our solar system [11]. Properties of neutron-rich nuclei near the N = 82 shell are important to understand the formation of the second r-process peak [12,13]. The calculations in N = 82 isotones have obtained strong evidence for the persistence of the N = 82 closed shell [14].…”

High-precision measurements of low-lying isomeric states in In120–124 with the JYFLTRAP double Penning trap

“…Neutron-rich indium isotopes around the doubly magic 132 Sn nucleus are a center of attention and they are extensively studied via a plethora of experimental methods, such as mass measurements [1][2][3][4], laser spectroscopy [5,6], decay spectroscopy [7][8][9][10][11][12][13][14][15][16][17][18], and transfer reactions [19]. It is because nuclei around the doubly magic core are relatively simple systems and they constitute a perfect testing ground for various theoretical approaches [20][21][22][23][24][25].…”