Deep excursion beyond the proton dripline. I. Argon and chlorine isotope chains
The proton-unbound argon and chlorine isotopes have been studied by measuring trajectories of their decay-in-flight products by using a tracking technique with micro-strip detectors. The proton () and two-proton () emission processes have been detected in the measured angular correlations “heavy-fragment”+ and “heavy-fragment”++, respectively. The ground states of the previously unknown isotopes Cl and Cl have been observed for the first time, providing the separation energies of and MeV, respectively. The relevant systematics of and separation energies have been studied theoretically in the core+ and core++ cluster models. The first-time observed excited states of Ar allow to infer the -separation energy of 6(34) keV for its ground state. The first-time observed state in Ar with MeV can be identified either as a ground or an excited state according to different systematics.
The location of the driplines — the borderlines separating particle-stable and particle-unstable isotopes — is one of the fundamental questions of nuclear science. The unbound states with small decay energy can have lifetimes which are long enough to be treated as quasistationary states. Thus they may be considered as stationary states in many theoretical applications. This naturally leads us to the question: what are the limits of nuclear structure existence? In other words, how far beyond the driplines the nuclear structure phenomena fade and are completely replaced by the continuum dynamics? This question represents a motivation for studies of nuclear systems far beyond the driplines.
The proton and neutron driplines have been accessed for nuclides in broad ranges of (number of protons) and (number of neutrons) of the nuclear chart. However, even in these regions the information about the nearest to the dripline unbound isotopes is scarce and often missing. Thus the fundamental question about the limits of the nuclear structure existence remains poorly investigated. For example, if we consider the proton dripline within (- and -shell nuclei), the most extensively investigated case in that region is the fluoride isotope chain. Here our knowledge extends three mass units beyond the proton dripline: the F and F nuclides are well studied, and considerable spectroscopic information is available now for F Goldberg et al. (2010) in addition.
This paper continues our analysis of the data on reactions with a relativistic Ar beam populating particle-unstable states Mukha et al. (2015); Golubkova et al. (2016); Xu et al. (2018). The article Mukha et al. (2015) was focused on Ar and Cl isotopes which were reported for the first time. It was also found that the decay mechanism of Ar is likely to belong to a transition region between true and sequential decay mechanisms. Such a “transition regime” exhibits strong sensitivity of observed kinematic variables to the values of parameters defining the decay mechanism: -decay energy , ground state (g.s.) resonance energy in the core+ subsystem , and its width . The practical implementations of this fact, including opportunity of a precise determination of from the correlation data, were recently elaborated in Ref. Golubkova et al. (2016). In paper Xu et al. (2018) a detailed consideration of the data from Mukha et al. (2015) was given.
In present work we report on the byproduct data of the same experiment which resulted in Refs. Mukha et al. (2015); Golubkova et al. (2016); Xu et al. (2018), which include observation of Cl and Cl ground states and several (presumably excited) states in Ar and Ar. In order to clarify the situation with the observed states, we have performed systematic studies of separation energies in the chlorine and argon isotope chains. The depth of the performed “excursion beyond the proton dripline” in the argon and chlorine isotope chains is similar now in extent to that for the fluorine isotope chain, the best-studied case in the whole nuclei region.
In the experiment, described in detail in Refs. Mukha et al. (2015); Xu et al. (2018), the Ar beam was obtained by the fragmentation of a primary 885 AMeV Ar beam at the SIS-FRS facility at GSI (Germany). The prime objective of the experiment was study of decays of Ar isotopes. The scheme of the measurements is shown in Fig. 1 (a). We briefly repeat the general description of the experiment and the detector performance given in Ref. Xu et al. (2018) in detail.
The FRS was operated with an ion-optical settings in a separator-spectrometer mode, when the first half of the FRS was set for separation and focusing of the radioactive beams on a secondary target in the middle of the FRS, and the second half of FRS was set for detection of heavy-ion decay products. The 620 AMeV Ar ions with the intensity of 50 ions were transported by the first half of the FRS in order to bombard a Be secondary target located at the middle focal plane S2. At the first focal plane S1 of the FRS, an aluminum wedge degrader was installed in order to achieve an achromatic focusing of Ar at the secondary target. In the previously reported data Xu et al. (2018) the Ar nuclei were produced via one-neutron () knockout from the Ar ions. The decay products of unbound Ar were tracked by a double-sided silicon micro-strip detector array placed just downstream of the secondary target, see Fig. 1 (b). The projectile-like particles, outgoing from the secondary target, were analyzed by the second half of the FRS, which was operated as a magnetic spectrometer. The magnet settings between the S2 and S4 focal planes were tuned for the transmission of the targeted heavy ion (HI) fragments (e.g., S) down to S4, the last focal plane. In addition to Ar, the studies of decay properties of the stopped Ar ions were performed by using the OTPC detector at S4 Lis et al. (2015).
A double-sided silicon micro-strip detector (DSSD) array consisted out of four large-area DSSDs Stanoiu et al. (2008) was employed to measure hit coordinates of the two protons and the recoil heavy ions, resulting from the in-flight decays of the studied precursors. The high-precision position measurement by DSSDs allowed for reconstruction of all fragment trajectories, which let us to derive the decay vertex together with an angular HI- and HI-- correlations. For example, the trajectories of measured S++ coincidences were a basis for the analysis and the concluded spectroscopic information on Ar Xu et al. (2018).
However, a number of by-product results were obtained in a similar way from the data recorded in the same experiment. Namely, excited states of Ar were populated by various inelastic mechanisms, and Ar spectrum was populated in two-neutron () knockout reaction. The unbound Ar and Ar states were detected in triple S++ and S++ coincidences, respectively, see the respective angular correlation plots in Figs. 2 and 3. The relative angles there and everywhere below are presented in milliradian units (mrad). Also the states of Cl and Cl can be populated both in the fragmentation of Ar and as the result of proton emission from the corresponding Ar isotopes. These mechanisms have lower cross sections, and the obtained results have less statistics, see the respective angular -HI correlation plots in Figs. 9 and 6. In spite of poor statistics with few events registered, we have obtained several nuclear-structure conclusions from the experimental data.
ii.1 How nuclear-structure information can be obtained from proton-ion angular correlations
Before the data analysis presentation, we remind the reader, how nuclear-structure information concerning the nuclei involved in a or decay can be obtained by measuring only the trajectories of the decay products, without measuring their kinetic energies. This approach has been successfully tested in analyses of , decays of the known states in Na, Ne and has been described in details in Ref. Mukha et al. (2010).
For the discussion of decays given below, let us consider three different mechanisms. These cases are illustrated in Fig. 4. The upper panels schematically show the nuclear states involved in decay of nucleus with mass number , the lower panels show the corresponding momentum correlations , where HI corresponds to the nucleus. In the first case (a) of prompt decay, sequential emission should be energetically forbidden. As both emitted protons should share -decay energy , their energy spectra are broad and centered around the value of ; consequently, the momentum-correlation plot should have the shape of an arc, with a radius corresponding to the value and with most of the counts lying in the peak indicated by the dark spot in the lower panel of Fig. 4 (a). Note that all momentum-correlation plots in Fig. 4 are symmetric with the respect to the line since the protons and are indistinguishable.
The case (b) represents the sequential emission of two protons through a narrow resonance in the intermediate nucleus with . The proton energies are fixed here, and the correlation plot should yield double peaks as indicated by the black dots in the lower panel of Fig. 4 (b).
The third -decay mechanism is 2p emission from several broad continuum parent states via a low-lying state in , see Fig. 4 (c). This mechanism should reveal a peak in the -HI energy with the corresponding broad distribution along the narrow “slice” as shown in the lower part of Fig. 4 (c).
In the present method, we measure only total HI momentum and relative -HI angles in the transverse direction. We register trajectories of all decay products directly downstream from the secondary-reaction target. Fig. 5 (b) shows the kinematics plot for the simple case of isotropic and mono-energetic single-proton emission from a high-energy heavy ion. Fig. 5 (c) shows the corresponding distribution of laboratory -HI opening angles, . The angular spectrum exhibits a sharp peak corresponding to the proton emitted almost orthogonal to the HI momentum vector. Thus the maximum value of is directly related to the decay energy of the emitted proton. In the same way, the momentum correlations for decays (Fig. 5) can be replaced by the corresponding correlations. If the initial and final states of emission are narrow, the width of a peak in the angular distribution is governed mostly by the angular straggling of the proton in the secondary-reaction target. If those states are broad, the width results from a convolution of the state’s width with the proton angular straggling.
The cases, sketched in Figs. 4 and 5 represent ideal cases. In reality, several proton branches may be present, representing more than one of the cases, shown schematically in Fig. 5 (a), and leading to a complicated spectra with several peaks. One can, however, clean up the spectra and enhance e.g. transitions with the small -values by gating on the small angles of and plotting the spectrum of under this condition.
Another tool of data analysis is a kinematic variable
describing 3-body HI++ angular correlations. Since is related to the energy sum of both emitted protons and, therefore, to the of the parent state by the relation Mukha et al. (2012), one can obtain an indication of the parent state and its -decay energy by studying the distribution of . In a case of the decay from the same state, two protons share , and such events should be located along a root-mean-square arc in an angular correlation plot . By gating on a particular arc, the decay events from a certain -precursor can be selected. The distributions are very useful in the analysis of -decay data since they produce the spectra with less peaks and allow to gate on a specific excitation-energy regions.
In all cases, detailed Monte-Carlo simulations are required in order to interpret the angular spectra quantitatively by taking into account the corresponding response of the experimental setup. For example, the angular correlation for fixed energy decay must be first calculated. This predicted angular correlation is then compared to the measured one. The resonance energy is obtained by the best-fit where the probability that the two distributions are identical has maximum value. In the same way, limits for the width of a resonance can be obtained.
The above-described analysis procedure, where the states observed in a -precursor were investigated by comparing the measured angular and correlations with the Monte Carlo (MC) simulations of the respective detector response, has been published in Refs. Mukha et al. (2010, 2012). We follow this procedure in the present work, and the applied detector calibrations are taken from the previous Ar analysis of the same experiment Xu et al. (2018).
ii.2 The data analysis: unknown states in Ar and Cl
We begin from the analysis of the relatively simple case of the measured S++ correlations presented by the and plots in Figs. 3 and 6(b), respectively. These Ar-related correlations comprise just seven 2p-decay events, each being measured in triple S+p+p coincidence. Each detected event provides two and one values. Most of them are very well focused around the locations at mrad or mrad. These values correspond to the 1p-decay of the Cl state with of about 1.6 MeV and to the 2p-decay of the Ar state with of about 5.5 MeV. A cross-check of this conclusion is illustrated in Fig. 6(a) where the angular correlations projected from the S++ correlation plot [in Fig. 6(b)] are compared with the “inclusive” distribution obtained from the measured double-coincidence events. One may see that the “inclusive” spectrum consists of relatively enhanced peaks (1–3). The peaks (1) and (2) have the best-fits at the 1p-decay energies of 1.60(8) and 3.9(1) MeV, respectively. They have been assigned as the first- and second-emitted protons from the 5.5 MeV state in Ar, and their sum decay energy gives the total -decay energy of 5.50(18) MeV.
The data-fitting procedure is illustrated on the example of the (1) peak at mrad in the correlation in Fig. 7. This is the same procedure described in details in Refs. Mukha et al. (2010); Xu et al. (2018). The best-fit simulations obtained for the in-flight decay of Cl with the 1p-decay energy of 1.60 MeV describe the data quantitatively, and the figure inset shows that the probability of the data matching simulations is about 1. The full width at half maximum of the probability distribution provides the evaluation of the uncertainty.
There are two additional events in the decay patten of the 5.5 MeV state in Fig. 6 (b) corresponding to the inclusive peaks (3) and (4) in Fig. 6 (a). As the inclusive peak (3) is much enhanced, we may speculate that it may be an evidence on the second state in Cl, which is also fed by the other unspecified reaction channels, illustrated in Fig. 4(c). The best-fit 1p-decay energy of the peak (3) is 3.20(6) MeV.
In addition, there are indications on S++ correlations at of 97 and 112 mrad, which may correspond to the -decays of Ar with of about 7.2 and 9.5 MeV, respectively. Both of the indicated states have the second-emitted proton energy of 1.6 MeV, which corresponds to the lowest assigned state in Cl.
The derived decay scheme and levels of Ar and Cl are shown in Fig. 8.
We argue below in Section III, that our empirical assignments are backed by the isobaric mirror symmetry systematics and that the most probable interpretation of the measured decay-product correlations is the observation of Cl ground state with =-1.60(8) MeV and the Ar excited state with =-5.50(18) MeV.
ii.3 The data analysis: unknown states in Ar and Cl
The -decay pattern of Ar, derived from the S++ data, is more complicated. Several separated regions with events, corresponding to the same -decay energy, can be distinguished at the low angles in Fig. 2, which indicate different states in Ar. The tentatively selected arcs are labeled by the Roman numerals (i)–(iv). The same event groups can be found in the angular correlation plot in Fig. 9 (c) derived for the assumed Ar -decays. Its projections on the and axes are shown in the panels (b) and (a) in Fig. 9, respectively. The (S-) projection indicates some structures centered at the angles mrad, which point to possible low-energy states in Cl. The projection indicates several -decay patterns in Ar with the centre-of-gravity values at mrad.
The obtained statistics of the measured triple coincidences is low, and the non-selective projections do not allow for a quantitative analysis. Thus we have used the slice projections gated by the selected areas (i-v) in Fig. 9 (a). These gated projections are shown in Fig. 10 in the panels (i-v), respectively. Two additional projections gated at very large values are shown in the panels (vi,vii). In analogy to the Ar analysis, the “inclusive” distribution obtained from the measured double-coincidence events is shown in the lowest panel of Fig. 10. This inclusive distribution display the same low-energy peak (1) at around 26 mrad as well as the peaks (4,5), though evidence on the Fig. 9(c)-indicated peaks at 37 and 43 mrad (marked as (2) and (3), respectively) is weak.
Similarly to the Cl case, the MC simulations of the well-distinguished peaks (1,4,5) in the lowest panel of Fig. 10 by the experimental-setup response have resulted in assigning of the unknown Cl states with the -decay energies of 0.48(2), 2.00(5) and 3.0(2) MeV, respectively. On the basis of the performed analysis, the 0.48(2) MeV peak is assumed to be the ground state of Cl. Such an assignment is supported by the observed S++ correlations where one of the emitted protons has relatively large energy and another proton’s energy is peaked at around 0.5 MeV, see Fig. 10(vii). This is a typical situation for a final-state interaction due to the Cl g.s. resonance, see illustration in Fig. 4(c).
By using the parameters of the Cl g.s. one may obtain the 2-decay energy of the lowest-energy state in Ar observed in the S++ correlations, see Fig. 10(i). We have fitted the projection (i) by a sequential proton decay of Ar via the g.s. of Cl, and the obtained value of 2-decay energy is 0.95(5) MeV. Though the pattern centered at mrad has low statistics, it is very important for an overall interpretation of the data, as it highly likely corresponds to the Ar first excited state. Thus we may lay the first piece into the puzzle of the Ar excitation spectrum and its -decay scheme whose complete reconstruction is shown in Fig. 11 and which is explained in a step-by-step way below.
Namely, the gated projections in Fig. 10 (ii) and (iii) exhibit the same peak (3) at 43 mrad, which point to the sequential 2p decays of these Ar states via the same state in Cl. The peak (3) is best-fitted by assuming the 1p decay of the Cl state with =1.35(5) MeV. Then the Ar states corresponding to the complementary bumps in the structures (ii) and (iii) have the fitted 2p-decay energies of 1.58(6) and 2.12(7) MeV, respectively. One should note that the projection (ii) provides very broad and statistically poor signal from the corresponding Ar state, which makes the assignment very tentative, see Fig. 11.
Next, the gated projections in Fig. 10 (iv) and (v) reveal events matching the same 2.00 MeV peak (4) in the inclusive spectrum in the lowest panel in Fig. 10. They point to the sequential 2p decays of two more states in Ar via the 2.00 MeV state in Cl. In particular, the fit of the peak at 48 mrad which is complementary to the peak (4) in the projection (v) yields its energy of 1.56(10) MeV, and together they allow for assignment of the new Ar state with the 2p-decay energy of 3.56(15) MeV, see Fig. 11. Interpretation of the projections in Fig. 10 (iv) is more complicated, because it has the additional components, and one of them matches the peak (2) at 37 mrad due to a suspected state in Cl.
The contribution of such a state can be spotted also in the projection (vi) in Fig. 10 as well as in the “inclusive” distribution labelled as (2). The corresponding fits provide the 1p-decay energy of 0.97(3) MeV assigned to the Cl state. Then the whole structure of the distribution (iv) in Fig. 10 may be explained by a sequential 2p-decay of one state in Ar by two branches via the intermediate 0.97 and 2.00 states in Cl. The respective fits provide two independent evaluations of the 2p-decay energy of the Ar state of 0.97(3)+1.65(10)=2.62(13) and 2.00(5)+0.45(3)=2.45(8) MeV, respectively. They agree within the statistical uncertainties. One may note that the assigned 2p-decay branch via the 2.00 MeV state in Cl has the first-emitted proton energy of 0.45(3) MeV, which coincides with the 1p-decay energy of the g.s. of Cl. Therefore the sequential 2p decay may proceed also via the g.s. of Cl. These two assignments undistinguishable in our experiment are shown in Fig. 11 by the dotted arrows. Due to this uncertainty, we accept the Ar state to be at 2.62(13) MeV.
Finally, the gated projection in Fig. 10 (vi) with the assumed peak (2) due to the 0.97 MeV state in Cl allows for identification of the highest state observed in Ar with the 2p-decay energy of 0.97(3)+3.2(2)=4.2(2) MeV.
The only un-discussed peak (5) at about 65 mrad in the “inclusive” distribution in the lowest panel of Fig. 10 is also detected in the observed S-- correlations, see Fig. 9(b). However, energy of another emitted proton is distributed in a broad range of energy, which points to a continuum region of Ar excitations above 5 MeV. Therefore the peak (5) can not be assigned to an individual Ar state. We may speculate that it probably belongs to the 3.0(2) MeV state in Cl which is strongly populated by de-excitation of high-energy continuum in Ar.
Summarizing the above considerations, we have assigned the Cl states with the decay energies of 0.48(2), 0.97(3), 1.35(5), 2.00(5) and 3.0(2) MeV. There is also some indication that the structure around mrad may consist of two sub-structures at about 24 and 28 mrad (corresponding to the values of 0.48 and 0.55 MeV, respectively), which we will discuss below. The newly prescribed states in Ar have the 2p-decay energies MeV. All derived levels in Ar and Cl and their decay transitions are shown in Fig. 11.
Iii Systematics for chlorine isotopes
As a first step in the interpretation of the data, we would like to evaluate the energies of the states in proton-rich chlorine isotopes systematically by using the known information about their isobaric mirror partners. The obstacle here is the Thomas-Ehrman shift (TES) effect Ehrman (1951); Thomas (1952), especially pronounced in the - shell nuclei. The systematics of orbital size variations for - and -wave configurations are different when approaching the proton dripline and beyond it. This leads to a significant relative shift of the -wave and -wave dominated states distorting the expected (due to isobaric symmetry) nuclear level ordering in isotopes near the proton dripline. The core+ cluster model is a reasonable tool for consideration of this effect.
The Coulomb displacement energies in the core+ cluster model depend on two parameters: the orbital radius, which is mainly controlled by the potential radius, and the charge radius of the core. We use the potential with a Woods-Saxon formfactor and with a conventional diffuseness parameter fm. The radius value is provided by the standard parameterizations
The charge radii of sulphur isotopes are poorly studied Angeli and Marinova (2013), so we use the extrapolation shown in Fig. 12. Here we use two limits, corresponding to either ascending or descending trend near the dripline (both trends are not excluded by the available systematics of the charge radii). One should note that the S case is already uncertain. This particle-unstable nuclide (expected to be a -precursor Fomichev et al. (2011)) has the valence-proton wave function expected to well penetrate into the sub-barrier region.
Then the Coulomb potential of the charged sphere is used with the radius parameter ,
iii.1 Cl and Cl cases
One can see in Fig. 13 (a,b), that for known isotopes Cl and Cl the used systematics of potential parameters given by Eqs. (1) and (2) provides level energies which are overbound a bit (by keV) in comparison with the data. However, the general trend is well reproduced, thus the standard set of the parameters could be the good starting point for the systematic evaluation of the whole isotope chain.
iii.2 Cl and Cl cases
Spectrum of Cl was discussed in details in Mukha et al. (2015); Xu et al. (2018), see Fig. 13 (d). The data on Cl spectrum is reported in this work for the first time. The spectra of these isotopes can be reasonably interpreted only on the bases of the strong TES effect for some states. The calculated levels shown in Fig. 13 (c) present evidence that two low-lying structures in the spectrum of Cl (at 0.48(2) and 0.97(3) MeV) can be associated with nearly-overlapping doublets – and –. We assume that the g.s. in Al has a -wave structure. Then its doublet partner, the state is expected to be strongly shifted down by TES, and therefore to become the Cl g.s. There is a hint in the data shown in Figs. 9 and 10, that the “ground state peak” in Cl at mrad actually consists of two substructures, differently populated in the decays of several Ar states. In this work, the Cl g.s. prescription is based on the lower substructure with the corresponding proton emission energy MeV.
Why the above-mentioned prescription is reliable? The Thomas-Ehrman shift for the Al-Cl g.s. pair is about 330 keV. If we assume that the g.s. in Al has an -wave structure, then the Thomas-Ehrman shift leads to the evaluated energies keV of the g.s. in Cl. For such low decay energies, the Cl g.s. should live sufficiently long time in order to “survive” the flight through the second achromatic stage of the FRS fragment separator (of ns). We don’t report such an experimental observation. We may also assume a -wave structure of the and second states. However such an assumption practically does not change the predicted energy of Cl, but it requires the existence of peaks which are not seen in our data.
iii.3 Cl case
A doublet of low-lying states can be found in the bottom of Na spectrum, see Fig. 13 (e). Presumably, the and states are separated by just of keV. The state can be only -wave dominated, while can be either -wave or -wave dominated. If both states have a -wave structure, then the Cl g.s. should be found at about 2.4 MeV. In contrast, the observation of decay events corresponding to MeV can be easily interpreted as the -wave g.s. of Cl with the predicted energy of MeV.
Iv Systematics look on argon isotopes
After we have systematically investigated the behavior of 1p separation energies for the chlorine isotopic chain, we can turn to the systematic studies of the corresponding argon isotopic chain, which is based on the obtained information. Namely, we apply the systematics of odd-even staggering (OES) energies which were shown to be a very helpful indicator concerning the dripline systems in our previous works Fomichev et al. (2011); Mukha et al. (2015); Grigorenko et al. (2017). The OES energy is defined as
The systematics of is presented in Fig. 14. One can see that the systematic trends are very stable for the all considered isotopic chains. The is always smaller for the proton-rich systematics compared to the neutron-rich one. The difference of 0.5 MeV is practically the same value for all three cases, see the gray line in Fig. 14. also systematically decreases with an increase of mass number, which indicates a borderline of nuclear stability. The for Ar was found to be smaller than the corresponding systematic expectation Mukha et al. (2015). It was argued in this work that such a deviation is typical for systems beyond the dripline, which is confirmed by the examples of well studied 2p emitters O, Ne and Mg. Theoretical basis for such an effect is provided by the three-body mechanism of TES Grigorenko et al. (2002), which was recently validated by the high-precision data and theoretical calculations in Ref. Grigorenko et al. (2015). When extrapolating this trend to the nearby isotopes, one may expect that Ar should reside on the systematics curve or slightly below, while the Ar could be considerably below.
The excitation spectrum of Ar obtained in this work demonstrates a very high level of isobaric symmetry in respect to its mirror Al, see Fig. 11. Based on the isobaric symmetry assumption, we can infer very small value of the 2p threshold keV for the g.s. of Ar. This value is obtained by a comparison of the 2p-decay energy of 950(50) keV and the literature value of 946.7(3) keV of the excitation energy of the first excited state in Ar and its mirror Al Ouellet and Singh (2013), respectively. The value of Ar g.s. may be also obtained by a comparison of the aligned low-energy exited states in Ar and Al. Namely, the states in Ar with 2p-decay energy of 1.580(60), 2.120(70) and 2.620(130) MeV match the known excited states in Al Ouellet and Singh (2013) at excitation energy of 1.613(0.24), 2.090(11) and 2.676(28) MeV, respectively. By assuming the same energy between the g.s. and the respective excited state both in Ar and Al, we obtain more estimations of the g.s. of Ar: at keV, respectively.
The weighted mean of all four pairs provides the averaged value of +6(34) keV which we finally accept for the g.s. of Ar. Our evaluation agrees within the experimental uncertainties with the previously-estimated value of -3(110) keV obtained in beta-decay studies of Ar Axelsson et al. (1998), and precision of the present result is improved by the factor of 3. Our conclusion is that the Ar g.s. is rather bound than not. With the known value MeV, we can estimate the value MeV for Ar, which is in a good agreement with the extrapolated OES energy trend in Fig. 14 (a), which gives MeV. This is an additional argument in favour of the isobaric symmetry (or very close to that) of the Ar and Al ground states.
So, the Ar g.s. is evaluated to be likely bound with the separation energy of less than 40 keV. Even if it is -unbound (which can not be excluded by our results), its decay status is not affected: for such a small decay energy the partial-lifetime of Ar is incomparably longer than its -decay lifetime. Then the g.s. of Ar can still be considered as a quasi-stable state in many theoretical applications. An interesting issue here could be the possible existence of the -halo in such an extremely lousy-bound proton-rich nuclide.
Now let us turn to the Ar system. As discussed above, we expect the chlorine isotopes to be overbound in comparison with their mirror isobars (relative to the isobaric symmetry expectations) in a region beyond the dripline because of the TES. For the argon isobars far beyond the dripline, there should be a competition of two trends. One is the overbinding because of TES (the Coulomb displacement energy decreases because of the increase of the valence orbital size). An opposite trend is underbinding due to reductions (the p-p pairing energy decreases because of the increase of the valence-proton orbital size). One must note that the absolute value of extrapolated OES energy is quite low, MeV [see Fig. 14 (c)]. As the negative or extremely small value of paring energy seems to be unrealistic assumptions, we accept the following values MeV as the limits of an OES energy variation. Then we obtain the value MeV for the g.s. of Ar by accepting . According to this estimate, the state observed in Ar at MeV can not be assigned as its ground state, and therefore it should be one of the excited states in Ar. However, one should note that this prediction based on the OES systematics is not in accord with the other systematics and the results of theoretical calculations available in the literature, see Table 2 reviewing the published results on Ar. So, further studies of the Ar system are required in order to clarify the issue.
The new isotopes Cl and Ar were recently discovered Mukha et al. (2015) and the spectroscopy of these two nuclei was performed Xu et al. (2018) with the reactions of Ar exotic beam at 620 AMeV energy on light target. In this work, we investigated the additional inelastic excitation and particle knockout channels of those reactions. The main results of this work are:
(i) Two previously-unknown isotopes, Cl and Cl, which are unbound respective to the emission have been observed. The ground state energies of Cl and Cl have been derived by using angular S+ correlations. In addition, four excited states of Cl have been identified as the sub-systems of the previously-unknown excited states of Ar. These states were populated by inelastic excitation of secondary Ar beam and identified by registering S++ correlations.
(ii) The first-time observed excitation spectrum of Ar matches very well the excitation spectrum of its isobaric partner Al. The registered isobaric symmetry is used in order to infer the position of the Ar ground state at the 2p separation energy MeV. The high level of isobaric symmetry of these mirror nuclei is confirmed by the systematics of OES energies. The near-zero value of of Ar suggests speculations about the possibility of halo in this nuclide.
(iii) First evidence on a state in a previously-unobserved isotope Ar has been obtained by detecting S++ correlations. The state was found to be -unbound with MeV. The results of the different energy systematics do not allow to clarify the status of the observed state. It may be either an excited at MeV above the ground state (as estimated in this work) or it may be a ground state of Ar according to Refs. Cole (1998); Tian et al. (2013); Simonis et al. (2016). This situation calls for further measurements.
Acknowledgements.This work was supported in part by the Helmholtz International Center for FAIR (HIC for FAIR), the Helmholtz Association (grant IK-RU-002), the Russian Science Foundation (grant No. 17-12-01367), the Polish National Science Center (Contract No. UMO-2015/17/B/ST2/00581), the Polish Ministry of Science and Higher Education (Grant No. 0079/DIA/2014/43, Grant Diamentowy), the Helmholtz- CAS Joint Research Group (grant HCJRG-108), the FPA2016-77689-C2-1-R contract (MEC, Spain), the MEYS Projects LTT17003 and LM2015049 (Czech Republic), the Justus-Liebig-Universität Giessen (JLU) and GSI under the JLU-GSI strategic Helmholtz partnership agreement.
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