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Testing ab initio nuclear structure in neutron-rich nuclei: lifetime measurements of second 2+ states in 16C and 20O

To test the predictive power of ab initio nuclear structure theory, the lifetime of the second 2+ state in neutron-rich 20O, tau(2+_2 ) = 150(+80-30) fs, and an estimate for the lifetime of the second 2+ state in 16C have been obtained, for the first time. The results were achieved via a novel Monte Carlo technique that allowed us to measure nuclear state lifetimes in the tens-to-hundreds femtoseconds range, by analyzing the Doppler-shifted gamma-transition line shapes of products of low-energy transfer and deep-inelastic processes in the reaction 18O (7.0 MeV/u) + 181Ta. The requested sensitivity could only be reached owing to the excellent performances of the AGATA gamma-tracking array, coupled to the PARIS scintillator array and to the VAMOS++ magnetic spectrometer. The experimental lifetimes agree with predictions of ab initio calculations using two- and three-nucleon interactions, obtained with the valence-space in-medium similarity renormalization group for 20O, and with the no-core shell model for 16C. The present measurement shows the power of electromagnetic observables, determined with high-precision gamma spectroscopy, to assess the quality of first-principles nuclear structure calculations, complementing common benchmarks based on nuclear energies. The proposed experimental approach will be essential for short lifetimes measurements in unexplored regions of the nuclear chart, including r-process nuclei, when intense ISOL-type beams become available.

in 16 C have been obtained, for the first time. The results were achieved via a novel Monte Carlo technique that allowed us to measure nuclear state lifetimes in the tens-to-hundreds femtoseconds range, by analyzing the Doppler-shifted γ-transition line shapes of products of low-energy transfer and deep-inelastic processes in the reaction 18 O (7.0 MeV/u) + 181 Ta. The requested sensitivity could only be reached owing to the excellent performances of the AGATA γ-tracking array, coupled to the PARIS scintillator array and to the VAMOS++ magnetic spectrometer. The experimental lifetimes agree with predictions of ab initio calculations using two-and three-nucleon interactions, obtained with the valence-space in-medium similarity renormalization group for 20 O, and with the no-core shell model for 16 C. The present measurement shows the power of electromagnetic observables, determined with high-precision γ spectroscopy, to assess the quality of first-principles nuclear structure calculations, complementing common benchmarks based on nuclear energies. The proposed experimental approach will be essential for short lifetimes measurements in unexplored regions of the nuclear chart, including r-process nuclei, when intense ISOL-type beams become available.
Atomic nuclei are composed of protons and neutrons, which, in turn, are systems of quarks and gluons confined via the strong interaction, as described by Quantum Chromodynamics (QCD). Ideally, one would like to obtain the properties of nuclei solving QCD, but despite recent progress this is beyond current computational capabilities [1][2][3]. At the energy and momentum scales relevant for nuclear structure, chiral effective field theory (EFT), an effective theory based on the symmetries of QCD, provides a practical alternative [4][5][6]. In chiral EFT the degrees of freedom are nucleons and pions, and nuclear forces are given by a systematic expansion of two-(NN), three-(3N) and many-nucleon interactions that includes pion exchanges and contact terms.
In recent years, chiral EFT interactions have been combined with ab initio approaches that consider all nucleons in the solution of the nuclear many-body problem, in studies of mid-mass nuclei up to tin [7][8][9][10][11][12]. Theoretical results are typically compared to the simplest experimental observables, namely binding and excitation energies. First calculations of medium-mass nuclei with chiral NN+3N interactions predicted correctly the oxygen neutron dripline at 24 O [8,13], and later works reproduced well the excitation spectra of neutron-rich oxygen isotopes [8]. In neutron-rich calcium and nickel isotopes, the shell evolution was also satisfactorily predicted [14][15][16]. Tests of ab initio calculations against other observables include charge radii [17,18], beta decay lifetimes [19], and elastic proton scattering off 10 C [20]. Electromagnetic (EM) responses have also been studied in selected nuclei [21][22][23]. A general agreement between theory and experiment was found.
Electric and magnetic γ decays provide a more demanding, complementary test of theoretical approaches. So far, EM decays in light/medium-mass systems have only been explored in few cases [24][25][26][27][28][29]. In contrast to energies or beta decays, ab initio methods do not yet con-sistently describe all the data related to EM transitions. This calls for precision measurements of EM observables which are sensitive to the details of the calculations. Ideal cases are neutron-rich O and C isotopes. Here, ab initio approaches show a strong sensitivity of EM decays to 3N forces which significantly affect the lifetime of selected excited states, by changing the wave function composition [30].
In this paper, we focus on the lifetime determination of the second 2 + excitations, 2 + 2 , in 20 O and 16 C nuclei. We confront our results with predictions of the valencespace in-medium similarity renormalization group (VS-IMSRG) and of the no-core shell model (NCSM) of Ref. [30], both including NN and 3N forces. Previous experiments have only set limits on the lifetime of these 2 + 2 states, of the order of a few ps, and provided information on branching ratios in their decays [31][32][33][34]. In this work, we aim at a much more stringent test of ab initio calculations by measuring the 2 + 2 state lifetimes. In 20 O, the first-excited 2 + 1 state at 1674 keV decays with a lifetime of 10.4(9) ps [35]. The 2 + 2 state, of our interest, located at 4070 keV, was found to decay to the 2 + 1 state with 72(8)% branch [31], in parallel to the direct ground state branch for which contradicting B(E2) information is reported from intermediate-energy Coulomb excitation [36,37]. In 16 C, the 2 + 1 state at 1762 keV decays with a lifetime of 11.4(10) ps [33], while for the 2 + 2 state lifetime only the upper limit of 4 ps is known [32,33]. Theoretical predictions suggest that the lifetimes of these 2 + 2 states are in the tens-to-hundreds femtoseconds range. This poses an experimental challenge since such neutron-rich systems can only be produced, with sizable cross sections, in: i) relativistic heavy-ion fragmentation, for which the lower limit in lifetime determination is few hundreds femtoseconds, as shown by Morse et al. [38], ii) low-energy transfer and deepinelastic reactions, where the complex structure of the product velocity distribution, caused by large energy dissipations [39,40], does not allow to use standard Doppler Shift Attenuation Methods [41].
In this work, we have developed a technique which enables us to access tens-to-hundreds femtoseconds life- times in exotic neutron-rich nuclei, with low-energy transfer and deep-inelastic heavy-ion reactions our approach is a significant extension of the Doppler-Shift Attenuation Method to cases without well-defined reaction kinematics. It will be an essential and quite unique tool to determine short lifetimes in nuclei with large neutron excess, including r-process nuclei, when intense ISOLtype beams [42], currently under development, are available. The novelty of the method relies on the accurate reconstruction of the complex initial velocity distribution of the reaction product excited to a specific nucler state, including contributions from direct and dissipative processes. The Doppler-shifted γ-transition line shape is then simulated considering the precisely determined detection angle between the γ-ray and the reconstructed initial product velocity inside the target. It will be shown that the required sensitivity to the lifetimes could only be achieved by the excellent performances of our integral AGATA+PARIS+VAMOS detection system.
In the present study, 16 C and 20 O nuclei were populated in both direct transfer and deep-inelastic processes induced by an 18 O beam at 126 MeV on a 181 Ta target (6.64 mg/cm 2 ). The beam energy at the center of the target was ∼116 MeV, i.e., ∼50% above the Coulomb barrier, and projectile-like products had velocity v/c∼10%. The experiment was performed at GANIL with 31 High-Purity Ge detectors of the AGATA array [43,44], coupled to a scintillator array consisting of two large volume (3.5"×8") LaBr 3 detectors plus two clusters of the PARIS setup [45], which produced excellent time reference for the reaction. Reaction products were detected in the VAMOS++ spectrometer [46,47], placed at the reaction grazing angle of 45 • (opening angle ±6 • ) with respect to the beam direction and aligned with the center of AGATA. Relative to the VAMOS++ axis, AGATA covered the 115 • -175 • angular range, while the scintillators were placed at 90 • . More than 10 7 events were collected requiring coincidences between projectile-like products detected in VAMOS++ and γ rays in AGATA or PARIS. The VAMOS++ setting was optimized to detect 20 O within a large velocity range, including quasielastic and deep-inelastic processes. Other products with charge 5≤ Z ≤9 and mass number 11≤ A ≤21 were also detected. Identification plots of O and C ions are given in Fig. 1, together with the velocity distributions measured in VAMOS++ for the 2 + 2 states in 20 O and 16 C. In the case of 20 O, the velocity distribution shows a pronounced peak, corresponding to the direct population in a quasi-elastic process, while the tail, extending towards lower velocities, is associated with higher kinetic energy loss. The velocity distribution is similar in 16 C, although with a much larger contribution (∼ 32%) from dissipative processes.
Portions of γ-ray spectra obtained with AGATA by gating on 19 O, 20 O and 16 C ions, Doppler-corrected considering the product velocity vector measured in VA-MOS++, are shown in Fig. 2, panels a), b) and c), respectively. All visible γ rays correspond to known transitions (see level schemes on the right). A closer inspection reveals that some of the peaks are narrow and their energies agree, within uncertainty, with earlier studies. This is the case of transitions from relatively long-lived levels (τ >1 ps), emitted in flight outside the target, as for example the 1375-keV and 2371-keV lines in 19 O, the 1674-keV line in 20 O and the 1762-keV peak in 16 C [48].
In contrast, other lines, depopulating states with lifetimes shorter than 1 ps, exhibit rather large widths and tails. This indicates that the corresponding γ rays were partly emitted during the stopping process of the reaction product inside the target, i.e., at larger velocity than the one measured in VAMOS++. In these cases, the Doppler-broadened line shape can be used to determine the lifetime of the state.
The Monte Carlo simulation of the Doppler-shifted γtransition line shapes was performed in three steps [49]. First, we reconstruct, iteratively, the initial product velocity distribution inside the target, associated with the population of a given state (see Fig. 1). The procedure is based on the VAMOS++ measured velocity-angle distribution (the spectrometer response function is considered [47]), the reaction kinematics calculated for the selected state (including direct population and more dissipative processes), a random probability of reaction occurrence over the target thickness, and the slowing-down and straggling processes inside the target, from Ziegler et al. [50,51]. Second, we simulate the Doppler-shifted energy measured in AGATA for a transition emitted by the moving product nucleus, with lifetime and transition energy as parameters. Here, the angle between the product velocity at the emission point and the γ-ray direction is determined with precision of ∼1.5 • (i.e., 1 • for AGATA and 1 • for VAMOS++). Finally, we minimize the χ 2 surface, in lifetime-energy coordinates, by comparing the simulated and experimental transition line shapes, for three selected angular ranges (i.e., 120 • -140 • , 140 • -160 • and 160 • -180 • ), simultaneously. Figures 3(a)-(c) and (d)-(f) show the 2371-and 2779-keV lines from the decay of the 9/2 + and 7/2 + states in 19 O, with lifetimes τ >3.5 ps and τ = 92 (19) fs, respectively [52,53]. In Fig. 3 We now turn to the lifetime of the 2 + 2 states in 20 O and 16 C. Figures 3 (g)-(i) refer to the 2 + 2 → 2 + 1 decay in 20 O. A well-defined minimum is found in the χ 2 surface, yielding the values E γ = 2394.6 +1.0 −1.0 keV and τ = 150 +80 −30 fs. We note that the γ-ray energy agrees with the most precise value reported in literature, E γ = 2396(1) keV [31], while the present determination of the lifetime is the first obtained thus far. For the 2 + 2 → 2 + 1 decay, considering its 79(5)% branching ratio, here determined, one gets a partial lifetime of 190 +102 −40 fs. We stress that the above results rely on the AGATA excellent position resolution of the first γ interaction point, determined with the combined use of Pulse Shape Analysis [54,55] and the Orsay Forward Tracking algorithm [56]. Defining the γ direction from the front segment centers only, as in the case of conventional Ge arrays, gives χ 2 minima with much larger uncertainty (dashed lines in the insets of Fig. 3 (d)-(g)), making meaningless a comparison with theory. Figures 3 (j)-(k) report the analysis of the 2 + 2 state in 16 C, performed on the γ-ray spectrum integrated over the entire angular range, i.e., 120 • -180 • , due to the limited statistics. As a consequence, the 16 C χ 2 map, shown in Fig. 3(j), displays a wide valley, resulting in a very limited sensitivity when E γ < 2216 keV. For 2 + 2 →2 + 1 transition energies E γ > 2216 keV, the procedure provides a more definite value, which would indicate a lifetime τ < 180 fs. Considering the most precise energy measurement E γ = 2217(2) keV [33], there is a 78% probability for this scenario.
We performed calculations for 20 O by employing chiral NN interactions based on Ref. [57], and 3N interactions fitted on top, considering only few-body systems up to 4 He. First, the many-body perturbation theory (MBPT) valence-shell interactions from Ref. [8] were employed with an 16 O core. NN and normal-ordered 3N interactions are included up to third order, neglecting residual 3N interactions. Effective operators are used to calculate EM transitions [58,59]. The shell model diagonalizations were performed with the code ANTOINE [60]. The MBPT results reproduce well the 2 + 1 → 0 + lifetime in 20 O (τ = 11.7 ps vs. the experimental τ = 10.5(4) ps [35]), and this agreement does not depend significantly on the inclusion of 3N interactions. In turn, as shown in Fig. 4, the calculated partial lifetime of the 2 + 2 → 2 + 1 decay, τ = 275 fs (dashed blue line), agrees well with the present measurement only when 3N interactions are considered (B(M1)=0.015 µ 2 N , B(E2)=0.051 e 2 fm 4 , taking the experimental transition energy). When they are neglected, the 2 + 2 → 2 + 1 partial lifetime is about 60% . Black crosses and dashed lines indicate the χ 2 minimum and 1σ uncertainty for γ-detection angles defined by the AGATA front segment centers (precision ∼20 mm). In (a)-(c), simulated spectra for τ = 100 and 1000 fs (blue and red lines, respectively) are shown to demonstrate the absence of broadening and tails for decays from long-lived states. Panel j): χ 2 surface for the 16 C 2 + 2 → 2 + 1 transition. Panel k): 16 C 2 + 2 → 2 + 1 transition measured over the full AGATA angular range (histogram), compared with simulated spectra relative to the minimum of the χ 2 map, for Eγ = 2215 keV (τ =230 fs) and Eγ = 2217 keV (τ =50 fs).
longer (dashed green line) and the energy of the 2 + 2 state is more than 1 MeV lower (see also Ref. [8]). This change is driven by the dominant (d 5/2 ) 3 (s 1/2 ) 1 configuration, which is mostly missing in the NN calculation.
Second, we performed ab initio calculations with the VS-IMSRG [8,12,[61][62][63], based on the NN+3N interaction labeled EM1.8/2.0 in Ref. [64]. The treatment of 3N interactions improves that of the MBPT, by including approximately the interactions between valence nucleons [63]. In addition, we decouple valence-space operators consistent with the Hamiltonian as in Refs. [26,65], avoiding the use of effective charges or g-factors and producing effective two-body EM operators. In the IMSRG(2) approximation used here, all operators are truncated at the two-body level, which leads to reduced B(E2) values as discussed in Ref. [26]. VS-IMSRG transition energies are in very good agreement with experiment, giving 1629 keV and 2422 keV for the 2 + 1 →0 + and 2 + 2 →2 + 1 decays, respectively. This is at variance with the MBPT results, which overestimate the experimental energies by about 400 keV. The VS-IMSRG 2 + 2 → 2 + 1 partial lifetime in 20 O, τ = 249 fs (solid line), also agrees very well with the present measurement (see Fig. 4). B(M1)=0.0166 µ 2 N dominates over B(E2)=0.0684 e 2 fm 4 .
The good agreement with the experimental lifetime also suggests a small impact of meson-exchange currents, not included in this calculation.
In 10−20 C isotopes, Forssén et al. have performed NCSM calculations with NN+3N interactions [30]. Like in the VS-IMSRG, total energies and transition probabilities are obtained without effective charges or additional parameters. Consistently with the MBPT calculation on 20 O, Forssén et al. find the decay rates of the 2 + 2 , 3 + 1 and 4 + 1 excited states in 16 C sensitive to 3N forces, with transition strengths reduced up to a factor 7. For the 2 + 2 →2 + 1 decay, the NCSM finds that the B(M1)=0.063 µ 2 N dominates, yielding the partial lifetime τ = 81 fs. Figure 4 shows that the NCSM calculations are consistent with the experimental estimates for transition energy E γ ≥ 2216 keV − this scenario has 78% probability, as discussed above. The absence of a 3980-keV 2 + 2 →0 + decay branch in our data, for which we extract an upper limit of 13% (compatible with the previous value of ≤8.8% [33]) is also consistent with the NCSM NN+3N results.
Summarizing, we have measured, for the first time, the lifetime of the 2 + 2 state in 20 O, and an estimate is given for the 2 + 2 state in 16 C. To obtain such results, a novel Monte Carlo technique was developed to determine life- times in the tens-to-hundreds femtoseconds range, using low-energy transfer and deep-inelastic reactions. This technique will be essential for similar investigations in exotic neutron-rich nuclei produced with intense ISOLtype beams. Crucial in our work was the high precision provided by the AGATA γ-tracking array. The achieved results on transition probabilities agree well with predictions from MBPT and ab initio VS-IMSRG for 20 O, and NCSM calculations for 16 C, showing that 3N interactions are needed to accurately describe electromagnetic observables in neutron-rich nuclei. From a broader perspective, the present measurement demontrates that highprecision γ spectroscopy can benchmark first principles nuclear structure calculations. The work paves the way toward comprehensive tests of ab initio approaches, exploiting electromagnetic transitions in addition to standard comparisons based mostly on nuclear energies.
We thank S. R. Stroberg for very useful discussions. This work was supported by the Italian Istituto Nazionale