scholarly journals Nuclear moments put a new spin on the structure of 131In

Author(s):  
Adam Vernon ◽  
Ronald Fernando Garcia Ruiz ◽  
T. Miyagi ◽  
Cory Binnersley ◽  
Jon Billowes ◽  
...  

Abstract In spite of the high-density and strongly correlated nature of the atomic nucleus, experimental and theoretical evidence suggests that around particular 'magic' numbers of nucleons, nuclear properties are governed by a single unpaired nucleon1,2. A microscopic understanding of the extent of this behaviour and its evolution in neutron-rich nuclei remains an open question in nuclear physics 3-5. A textbook example is the electromagnetic moments of indium (Z = 49) 6, which are dominated by a hole with respect to the proton magic number Z = 50 nucleus. They exhibit a remarkably constant behaviour over a large range of odd-mass isotopes, previously interpreted as pure "single-particle behaviour". Here, we present precision laser spectroscopy measurements performed to investigate the validity of this simple single-particle picture. Observation of an abrupt change in the dipole moment at N = 82 reveals that while the single-particle picture indeed dominates at neutron magic number N = 82 2,7, it does not for previously studied isotopes. We present state-of-the-art nuclear theory developed to investigate the details of the nuclear forces that describe the experimental results. The emergence and disappearance of single-particle behaviour was reproduced from an ab initio theory, including challenging many-body correlations in these large, complex nuclei. The inclusion of time-symmetry-breaking mean fields is shown to be essential for a correct description of the nuclear electromagnetic properties within the Density Functional Theory framework. Until now, such time-odd channels have been poorly constrained, but are essential to provide accurate predictions of nuclear properties necessary for searches of new physics with neutrinos 8,9 and studies of fundamental symmetries 10,11. These findings are key to understand the microscopic origin of nuclear electromagnetism and the emergence of single-particle phenomena from complex nuclei.

2008 ◽  
Vol 23 (27n30) ◽  
pp. 2589-2592 ◽  
Author(s):  
G. SAXENA ◽  
D. SINGH ◽  
H. L. YADAV ◽  
A. HAGA ◽  
H. TOKI

Inspired by recent measurements indicating proton magic number at Z =14 in the vicinity of 42 Si , we have employed our relativistic mean-field (RMF) plus state dependent BCS approach for the study of even-even nuclei to obtain magic numbers and to look for nuclei exhibiting weakly bound structures and even halo formation. In our RMF+BCS approach the single particle continuum corresponding to the RMF is replaced by a set of discrete positive energy states for the calculations of pairing energy. It is found that in several nuclei the filling in of low lying single particle resonant state with large angular momentum, even before it becomes a bound state, helps to accommodate more neutrons but with extremely small increase in the binding energy. This gives rise to the occurrence of weakly bound system of neutron rich nuclei.


2007 ◽  
Vol 78 ◽  
pp. 012018 ◽  
Author(s):  
G I Fann ◽  
R J Harrison ◽  
G Beylkin ◽  
J Jia ◽  
R Hartman-Baker ◽  
...  

1971 ◽  
Vol 46 ◽  
pp. 356-363
Author(s):  
M. R. McNaughton

The conditions for superfluidity or ferromagnetism in neutron stars are presented and discussed (but not derived). It is suggested that present estimates relating to these are in error and that the predictions made contradict at least one of three sets of nuclear physics data cited in the text. This is due to neglecting the action of the exclusion principle.A comparatively simple method for calculating the strength of nuclear forces in the presence of many-body effects is outlined. Some preliminary results are presented together with projected future developments.


2016 ◽  
Vol 25 (05) ◽  
pp. 1641007 ◽  
Author(s):  
Manuel Pavón Valderrama

Effective field theories are the most general tool for the description of low energy phenomena. They are universal and systematic: they can be formulated for any low energy systems we can think of and offer a clear guide on how to calculate predictions with reliable error estimates, a feature that is called power counting. These properties can be easily understood in Wilsonian renormalization, in which effective field theories are the low energy renormalization group evolution of a more fundamental — perhaps unknown or unsolvable — high energy theory. In nuclear physics they provide the possibility of a theoretically sound derivation of nuclear forces without having to solve quantum chromodynamics explicitly. However there is the problem of how to organize calculations within nuclear effective field theory: the traditional knowledge about power counting is perturbative but nuclear physics is not. Yet power counting can be derived in Wilsonian renormalization and there is already a fairly good understanding of how to apply these ideas to non-perturbative phenomena and in particular to nuclear physics. Here we review a few of these ideas, explain power counting in two-nucleon scattering and reactions with external probes and hint at how to extend the present analysis beyond the two-body problem.


2010 ◽  
Vol 150-151 ◽  
pp. 984-987
Author(s):  
Shuai Qin Yu ◽  
Li Hua Dong ◽  
Yan Sheng Yin

The geometric structures and electronic properties of Si doped Fen (n=2-7) clusters have been systematically studied at the BPW91 level in density-functional theory (DFT). Calculated results show that an Si impurity does not change the ground-state structure of small iron clusters and prefers to occupy surface site bonding with iron atoms as many as possible. The second-order energy difference and the vertical ionization potential show that n=4 and 6 are magic numbers within the size range studied, but the maximum value occurs at n=4 for the energy gap between the highest occupied molecular orbital (HOMO) and the lowest unoccupied molecular orbital(LUMO). It is found that the hybridization intensity between Si and Fe atoms is relevant to the stability of clusters.


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