FIG 4 - uploaded by Fedor Simkovic
Content may be subject to copyright.
(Color online) The 0νββ matrix element as a function of maximum seniority included in the SM wave functions for 82 Se-82 Kr and of 128 Te-128 Xe. The contributions of seniority 6 and 10 states are appreciably smaller in agreement with the philosophy of the Random Phase Approximation. The data in the figure are taken from Caurier et al. [8].

(Color online) The 0νββ matrix element as a function of maximum seniority included in the SM wave functions for 82 Se-82 Kr and of 128 Te-128 Xe. The contributions of seniority 6 and 10 states are appreciably smaller in agreement with the philosophy of the Random Phase Approximation. The data in the figure are taken from Caurier et al. [8].

Source publication
Article
Full-text available
The methods used till now to calculate the neutrinoless double beta decay matrix elements are: the Quasiparticle Random Phase Approximation (QRPA), the Shell Model (SM), the angular momentum projected Hartee-Fock-Bogoliubov approach (HFB) and the Interacting Boson Model (IBM). The different approaches are compared specifically concerning the the an...

Contexts in source publication

Context 1
... [8,10,11]. However, contributions of the seniority six and ten admixtures to the neutrinoless double beta decay probability are suppressed according to the philosophy of the Random Phase Approach, that the ring diagrams are the leading ones (see also figure 4). ...
Context 2
... the RPA is approximately correct, since the ring diagrams give the most important ground state correlations. The contributions of seniority 6 and 10 to M 0ν are suppressed compared to the others (see figure 4). Figures 2 and 3 show the QRPA contributions of different angular momenta of the neutron pairs, which are changed in proton pairs with the same angular momenta. ...
Context 3
... radius parameter is chosen to be r 0 = 1.2 fm. Figure 4 shows for 82 Se and for 128 Te the influence of different seniority states in the SM [8]. A seniority zero pair corresponds to a zero angular momentum neutron pair, which can be changed into a zero seniority proton pair. ...
Context 4
... (see figures 1 and 4). But the SM results show also, that the seniority 6 and 10 configurations, which are not included in the QRPA ground state, contribute just a little to the total neutrinoless double beta decay matrix element (see figure 4). ...

Similar publications

Article
Full-text available
Background: The calculation of the hyperon binding energy in hypernuclei is crucial to understanding the interaction between hyperons and nucleons. Purpose: We assess the relative importance of two- and three-body hyperon-nucleon force by studying the effect of the hyperon-nucleon-nucleon interaction in closed shell \Lambda-hypernuclei from A=5 to...
Article
Full-text available
The relativistic particle-vibration coupling (RPVC) model is extended by the inclusion of spin- and isospin-flip excitation modes into the phonon space, introducing a new mechanism of dynamical interaction between nucleons with different isospin in the nuclear medium. Protons and neutrons exchange by collective modes which are formed by isovector $...
Article
Full-text available
Alpha emission from a nucleus is a fundamental decay process in which the alpha particle formed inside the nucleus tunnels out through the potential barrier. We describe alpha decay of $^{212}$Po and $^{104}$Te by means of the configuration interaction approach. To compute the preformation factor and penetrability, we use the complex-energy shell m...
Article
Full-text available
The radii of nucleon distribution and neutron skin in nuclei beyond the \beta-stability line are studied within the extended Thomas-Fermi approximation. We show that the growth of neutron skin in unstable nuclei does not obey the saturation condition because of the neutron coat. The neutron coat indicates the possibility of giant neutron halo which...
Article
Full-text available
The production of phi mesons in the collisions of 2.83 GeV protons with C, Cu, Ag, and Au at forward angles has been measured via the phi -> K+K- decay using the COSY-ANKE magnetic spectrometer. The phi meson production cross section follows a target mass dependence of A^0.56+/-0.02 in the momentum region of 0.6-1.6 GeV/c. The comparison of the dat...

Citations

... To explore the β-decay properties and get a better knowledge of the stellar dynamics, numerous attempts have been made previously. The calculations of Takahashi et al [10] based on gross theory, QRPA-based computations (e.g., [11][12][13][14]), and shell model calculations (e.g., [15]), are noticeable mentions. The gross theory computations failed to give structural information about each nucleus. ...
Article
Full-text available
Reliable and precise knowledge of the β-decay properties of neutron-rich nuclei is important for a better understanding of the r-process. We report the computation of β-decay properties of neutron-rich Cerium isotopes calculated within the proton-neutron quasiparticle random phase approximation (pn-QRPA) approach. A total of 34 isotopes of Ce in the mass range 120 A 157 were considered in our calculation. Pairing gaps are recognized amongst the key parameters in the pn-QRPA model to compute Gamow-Teller (GT) transitions. We employed two different values of the pairing gaps obtained from two different empirical formulae in our computation. The GT strength distributions changed considerably with change in the pairing gap values. This in turn resulted in contrasting centroid and total strength values of the GT distributions and led to differences in calculated half-lives using the two schemes. The traditional pairing gaps resulted in siginificant fragmentation of GT strength. However, the pairing gaps, calculated employing the formula based on separation energies of neutron and proton, led to computed half-lives in better agreement with the measured data.
... The neutrinoless DBDs occur in medium-mass nuclei that are often far from closed shells and, as a consequence, the calculations are mostly made in the proton-neutron quasiparticle random phase approximation (pn-QRPA), since this tool is computationally much simpler than the SM. As discussed in Ref. [8], the kind of correlations that these two methods include are not the same. The pn-QRPA deals with a large fraction of nucleons in a large single-particle space, but within a modest configuration space. ...
... The ground state defined in Eq. (2.27) is more accurate than the BCS ground state (a k |BCS = 0) since it contains terms with 0, 4, 8, . . . quasiparticles [8]. Nevertheless, in the present model we approximate the initial ground state in the (A, Z ) nucleus by the BCS vacuum and the states |J α in the intermediate (A, Z ∓ 1) nuclei as ...
... (3) The F strengths S {2} 00 deviate quite significantly from the sum rule strengths S {2} 00 -24% and 40%, respectively, within the spe spaces e expt j and e j in 48 Ca, 8 Note that the present calculations were done in a single-particle space consisting of the 2p-1 f -2s-1d shells for both protons and neutrons. and 14% in 96 Ru. ...
Article
A new model, based on the BCS approach, is especially designed to describe nuclear phenomena (A,Z)→(A,Z±2) of double-charge exchange (DCE). Although it was proposed and applied in the particle-hole limit, by one of the authors [Krmpotić, Fizika B 14, 139 (2005)], it has not yet been applied within the BCS mean-field framework, nor has its ability to describe DCE processes been thoroughly explored. It is a natural extension of the pn-QRPA model, developed by Halbleib and Sorensen [Nucl. Phys. A 98, 542 (1967)] to describe the single β decays (A,Z)→(A,Z±1), to the DCE processes. As such, it exhibits several advantages over the pn-QRPA model when used in the evaluation of the double beta decay (DBD) rates. For instance, (i) the extreme sensitivity of the nuclear matrix elements (NMEs) on the model parametrization does not occur; (ii) it allows us to study the NMEs, not only for the ground state in daughter nuclei, as the pn-QRPA model does, but also for all final 0+ and 2+ states, accounting at the same time for their excitation energies and the corresponding DBD Q values; (iii) together with the DBD-NMEs it also provides the energy spectra of Fermi and Gamow-Teller DCE transition strengths, as well as the locations of the corresponding resonances and their sum rules; (iv) the latter are relevant for both the DBD and the DCE reactions, since the underlying nuclear structure is the same; this correlation does not exist within the pn-QRPA model. As an example, detailed numerical calculations are presented for the (A,Z)→(A,Z+2) process in Ca48→Ti48 and the (A,Z)→(A,Z−2) process in Ru96→Mo96, involving all final 0+ states and 2+ states.
... Deficiencies of the pnQRPA formalism have been analyzed against the ISM formalism, e.g., in [199] by using a seniority-based scheme where the pnQRPA was considered to be a low-seniority approximation of the ISM. On the other hand, the ground-state correlations of the pnQRPA introduce higher-seniority components to the pnQRPA wave functions and the deficiencies stemming from the incomplete seniority content of the pnQRPA should not be so severe [200]. Schematic or G-matrix-based boson-exchange Hamiltonians have widely been used in the calculations. ...
... This decomposition has frequently been studied in the framework of the pnQRPA (see [589] for a review), but also in the ISM [590] and in the microscopic interacting boson model (IBM-2) [591]. The decomposition can also be probed by studying the angular momenta and parities of the neutron pairs that are changed into proton pairs in the 0νβ − β − decay [200]. The usual multipole decomposition (42) has been studied in the case of the deformed QRPA in [592]. ...
Article
Neutrino–nuclear responses associated with astro-neutrinos, single beta decays and double beta decays are crucial in studies of neutrino properties of interest for astro-particle physics. The present report reviews briefly recent studies of the neutrino–nuclear responses from both experimental and theoretical points of view in order to obtain a consistent understanding of the many facets of the neutrino–nuclear responses. Subjects discussed in this review include (i) experimental studies of neutrino–nuclear responses by means of single beta decays, charge-exchange nuclear reactions, muon- photon- and neutrino–nuclear reactions, and nucleon-transfer reactions, (ii) implications of and discussions on neutrino–nuclear responses for single beta decays, for astro-neutrinos, and for astro-neutrino nucleosynthesis, (iii) theoretical aspects of neutrino–nuclear responses for beta and double beta decays, for nuclear muon capture and for neutrino–nucleus scattering, and (iv) critical discussions on nucleonic and non-nucleonic spin–isospin correlations and renormalization (quenching or enhancement) effects on the axial weak coupling. Remarks are given on perspectives of experimental and theoretical studies of the neutrino–nuclear responses and on future experiments of double beta decays.
... In that work the pnQRPA was considered to be a low-seniority approximation of the ISM. But on the other hand, the ground-state correlations of the pnQRPA introduce higher-seniority components to the pnQRPA wave functions and the deficiencies stemming from the incomplete seniority content of the pnQRPA should not be so bad [108]. Also the renormalization problems of the two-body interaction are not so severe as in the ISM due to the possibility to use large single-particle model spaces. ...
Article
Full-text available
In this review the quenching of the weak axial-vector coupling strength, gA, is discussed in nuclear β and double-β decays. On one hand, the nuclear-medium and nuclear many-body effects are separated, and on the other hand the quenching is discussed from the points of view of different many-body methods and different β-decay and double-β-decay processes. Both the historical background and the present status are reviewed and contrasted against each other. The theoretical considerations are tied to performed and planned measurements, and possible new measurements are urged, whenever relevant and doable. Relation of the quenching problem to the measurements of charge-exchange reactions and muon-capture rates is pointed out.
... Other publications [106,130,186] have reported studies of the correlations included in the shell-model but not in the QRPA. Nuclear many-body states can be classified by a "seniority" quantum number s that labels the number of nucleons not in correlated neutronneutron and proton-proton J π = 0 + pairs. ...
... QRPA correlations in spherical nuclei include states with seniority s = 4, 8, 12 but not those with s = 6 and 10, and QRPA matrix elements could be too large for that reason. Although the contributions of states with s = 6 and 10 are relatively small in shell model calculations [186], Ref. [187] noted that when shell model states are forced to have the same seniority structure as QRPA states, the resulting shellmodel matrix elements grow, implying that the shortage of broken pairs in the QRPA makes its matrix elements too large. On the other hand, Ref. [188] observed that when the QRPA is applied within the small shell-model configuration space (which is not a natural space for the QRPA) the resulting matrix elements are similar to those of the shell model, suggesting that the shell-model matrix elements are about 50% too small. ...
Article
Full-text available
The nuclear matrix elements that govern the rate of neutrinoless double beta decay must be accurately calculated if experiments are to reach their full potential. Theorists have been working on the problem for a long time but have recently stepped up their efforts as ton-scale experiments have begun to look feasible. Here we review past and recent work on the matrix elements in a wide variety of nuclear models and discuss work that will be done in the near future. Ab initio nuclear-structure theory, which is developing rapidly, holds out hope of more accurate matrix elements with quantifiable error bars.
... This strongly hinders a reliable theoretical evaluation of the corresponding 0νββ-decay NMEs (for instance, it does not seem feasible in the near future to reliably treat this nucleus within the large-scale nuclear shell model (ISM), see, e.g., [14]). Recently, more phenomenological approaches like the pseudo-SU(3) model [30], the PHFB approach [15], the IBM [16], and the EDF [17] have been employed to calculate M 0ν for strongly deformed heavy nuclei (a comparative analysis of different approximations involved in some of the models can be found in [31]). The results of these models generally reveal a substantial suppression of M 0ν for 150 Nd as compared with the QRPA result of [11] where 150 Nd and 150 Sm were treated as spherical nuclei. ...
... The factor R l f l i , which includes the overlaps of single particle wavefunctions of the initial and final nuclei is given by (32) and the last term BCS f |BCS i in equation (31) corresponds to the overlap factor of the initial and final BCS vacua in the form given in [32]. The matrix element M 0ν is given within the QRPA in the intrinsic system by a sum of the partial amplitudes of transitions via all the intermediate states K π : ...
Article
Full-text available
A new generation of neutrinoless double beta decay experiments with improved sensitivity is currently under design and construction. They will probe inverted hierarchy region of the neutrino mass pattern. There is also a revived interest to the resonant neutrinoless double-electron capture, which has also a potential to probe lepton number conservation and to investigate the neutrino nature and mass scale. The primary concern are the nuclear matrix elements. Clearly, the accuracy of the determination of the effective Majorana neutrino mass from the measured 0\nu\beta\beta-decay half-life is mainly determined by our knowledge of the nuclear matrix elements. We review recent progress achieved in the calculation of 0\nu\beta\beta and 0\nu ECEC nuclear matrix elements within the quasiparticle random phase approximation. A considered self-consistent approach allow to derive the pairing, residual interactions and the two-nucleon short-range correlations from the same modern realistic nucleon-nucleon potentials. The effect of nuclear deformation is taken into account. A possibility to evaluate 0\nu\beta\beta-decay matrix elements phenomenologically is discussed.
Preprint
Full-text available
A new model, based on the BCS approach, is specially designed to describe nuclear phenomena $(A,Z)\rightarrow (A,Z\pm 2)$ of double-charge exchange (DCE). After being proposed, and applied in the particle-hole limit, by one of the authors (F. Krmpoti\'c [1]), so far it was never been applied within the BCS mean-field framework, nor has its ability to describe DCE processes been thoroughly explored. It is a natural extension of the pn-QRPA model, developed by Halbleib and Sorensen [2] to describe the single $\beta$-decays $(A,Z)\rightarrow (A,Z\pm 1)$, to the DCE processes. As such, it exhibits several advantages over the pn-QRPA model when is used in the evaluation of the double beta decay (DBD) rates. For instance, i) the extreme sensitivity of the nuclear matrix elements (NMEs) on the model parametrization does not occur, ii) it allows to study NMEs, not only for the fundamental state in daughter nuclei, as the pn-QRPA model does, but also for all final $0^+$ and $2^+$ states, accounting at the same time their excitation energies and the corresponding DBD Q-values, iii) together with the DBD-NMEs it provides also the energy spectra of Fermi and Gamow-Teller DCE transition strengths, as well as the locations of the corresponding resonances and their sum rules, iv) the latter are relevant for both the DBD and the DCE reactions, since the involved nuclear structure is the same; this correlation does not exist within the pn-QRPA model. As an example, detailed numerical calculations are presented for the $(A,Z)\rightarrow (A,Z+ 2)$ process in $^{48}$Ca $\rightarrow ^{48}$Ti and the $(A,Z)\rightarrow (A,Z- 2)$ process in $^{96}$Ru $\rightarrow ^{96}$Mo, involving all final $0^+$ states and $2^+$ states.
Article
We use the available experimental Gamow-Teller β− and β+/EC (electron-capture) decay rates between 0+ and 1+ ground states in neighboring even-even and odd-odd nuclei, combined with 2νββ half-lives, to analyze the influence of the nuclear environment on the weak axial-vector strength gA. For this purpose, the proton-neutron deformed quasiparticle random-phase approximation (pn-dQRPA), with schematic dipole residual interaction is employed. The Hamiltonian contains particle-hole (ph) and particle-particle (pp) channels with mass-dependent strengths. In deriving the equations of motion we use a self-consistent procedure in terms of a single-particle basis with projected angular momentum provided by the diagonalization of a spherical mean field plus the quadrupole-quadrupole interaction. Our analysis evidenced a quenched average effective value 〈gA〉≈0.7 with a root-mean-square deviation of σ≈0.3 for transitions from even-even emitters and σ≈0.6 for transitions from odd-odd emitters.
Article
In this paper, with restored isospin symmetry, we evaluated the neutrinoless double-β-decay nuclear matrix elements for Ge76, Se82, Te130, Xe136, and Nd150 for both the light and heavy neutrino mass mechanisms using the deformed quasiparticle random-phase approximation approach with realistic forces. We give detailed decompositions of the nuclear matrix elements over different intermediate states and nucleon pairs, and discuss how these decompositions are affected by the model space truncations. Compared to the spherical calculations, our results show reductions from 30% to about 60% of the nuclear matrix elements for the calculated isotopes mainly due to the presence of the BCS overlap factor between the initial and final ground states. The comparison between different nucleon-nucleon (NN) forces with corresponding short-range correlations shows that the choice of the NN force gives roughly 20% deviations for the light exchange neutrino mechanism and much larger deviations for the heavy neutrino exchange mechanism.
Article
We apply the proton-neutron deformed quasiparticle random-phase approximation (pn-dQRPA) to describe the low-lying (E≤6 MeV) 1+ Gamow-Teller (GT) strength functions in odd-odd deformed nuclei which participate as intermediate nuclei in two-neutrino double-β-decay (2νββ) transitions within the mass range A=70-176. In deriving equations of motion we use a single-particle basis with projected angular momentum, provided by the diagonalization of a spherical mean field furnished with a quadrupole-quadrupole interaction. The schematic residual Hamiltonian contains pairing and proton-neutron interaction terms in particle-hole (ph) and particle-particle (pp) channels, with constant strengths. By adopting constant particle-hole and particle-particle strengths we are able to describe the positions of the giant GT resonance and the measured half-lives of the 2νββ decays over the whole mass range A=70-176. At the same time we obtain a good agreement with the measured low-lying GT β- strength functions. By using the adopted ph and pp strengths, we predict the half-lives of a number of deformed 2νββ emitters and the low-lying GT strength functions of the corresponding odd-odd intermediate nuclei for their possible experimental tests in the future.