Relativistic Mean Field Study of Islands of Inversion in Neutron-Rich Z = 17–23, 37–40 and 60–64 Nuclei

Abstract

We study the extremely neutron-rich nuclei for Z = 17 − 23, 37 − 40 and 60 − 64 regions of the periodic table by using axially deformed relativistic mean field formalism with NL3* parametrization. Based on the analysis of binding energy, two neutron separation energy, quadrupole deformation and root mean square radii, we emphasized the speciality of these considered regions which are recently predicted islands of inversion.

Study of Reaction Cross Section of Light Mass Nuclei Using Glauber Formalisms

“…Measurements of nuclear reaction cross sections for 19,20,22 C suggest that the drip line nucleus 22 C has a halo structure [31,32]. The one and two neutron removal cross sections and the momentum distributions also support the halo behavior for 22 C. The nucleus 22 C has N = 16, which is a new magic number in neutron-rich nuclei [23,33], and it has a Borromean halo structure ( 21 C is unstable).…”

“…The advancement in radioactive ion beams (RIB) at intermediate energy made it possible to explore the nuclear chart, and it opened up new opportunities to investigate numerous exotic phenomena. The study of exotic nuclei, specially those around the drip-line, is of immense interest in present days [18][19][20]. Although, the drip line is well established at the doubly magic 24 O nucleus, the study of unbound oxygen isotopes [21] suggests the possibility of shifting the drip line.…”

Reaction and structure effects of light mass nuclei using Glauber model with relativistic and non relativistic simple effective interaction densities

“…The measurement of nuclear reaction cross-section for 19,20,22 C [27, 28] shows that the drip-line nucleus 22 C has a halo. The one and two neutron removal cross sections and momentum distribution also support the halo behavior of 22 C. The 22 C has N = 16 which is a new magic number in neutron-rich nuclei [20,29] and forms a Borromean halo structure ( 21 C is unstable).The direct time of flight mass measurement technique suggest 19 B, 22 C, 29 F and 34 Na are as Borromean dripline nuclei [30]. Another interesting phenomenon has been found in these days is the bubble structure of some nuclei like 22 O, 23 F, 34 Si, 36 S, 36 Ar, 46 Ar, 84 Se, 134 Ce, 174 Yb, 200 Hg etc.…”

“…The advancement in radioactive ion beam facility (RIB) in this energy range at various laboratories over the globe open up new opportunities to investigate some new exotic phenomenon. The study of such exotic nuclei specially those towards the dripline and the investigation of extended dripline are some of the current interest [17][18][19]. Although earlier the dripline is well established for 24 O which is a doubly magic nuclei.…”

“…Be,15 C,19 C,23 O and31 Ne halo nuclei are 942, 1065, 1215, 1327, The value of χ 2 is small for the Sph. RMF(NL3) density shows, the σ R obtained with this density reproduced better results as compare to the other cases.By looking deep into the table one can easily interpret that the values of reaction cross sections obtained for particular halo systems and other exotic nuclei shows better results with deformed RMF(NL3) and HF(SEI) densities.…”