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A. Gal

Publications and source records attributed to A. Gal.

At least 19 recordsLinked to original sources

Revisiting $\eta'(958)$ nuclear states

Observing $\eta'$-nuclear quasibound states requires that the $\eta'$-nuclear potential is both sufficiently attractive and weakly absorptive, as confirmed by the CBELSA/TAPS collaboration analysis of inclusive $\eta'$ production experiments on nuclear targets, including liquid hydrogen (LH$_2$). Here we present an alternative derivation of the $\eta'$-nuclear potential, constrained by near-threshold $pp\to pp\eta'$ and $\gamma p\to\eta' p$ production experiments on a free proton. The resulting $\eta'$-nuclear potential is weakly attractive and strongly absorptive, to the extent that observation of clear signals of $\eta'$-nuclear quasibound states is unlikely. Possible exceptions resulting from the dynamics of the nearby $I=\frac{1}{2}$ $J=({\frac{1}{2}})^-$ nucleon resonance $N^{\ast}$(1895) are briefly discussed.

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Compatibility of recent $\Xi$-nuclear bound state signals

J-PARC E05 reported recently a hint of a $\Xi^--{^{11}{\rm B}}$ nuclear state in the ${^{12}}{\rm C}(K^-,K^+){^{12}_{\Xi}}{\rm Be}$ spectrum, bound by $B_{\Xi^-}=8.9\pm 1.4 {^{+3.8}_{-3.1}}$ MeV. Using a density-dependent $\Xi$-nuclear optical potential $V_{\rm opt}^{\Xi}(\rho)$ we explore to what extent a $\Xi^-_{1s}$ assignment of this nuclear state is compatible with $\Xi^-_{1s}$ and $\Xi^-_{1p}$ nuclear-state interpretations of $\Xi^-$ capture events in light emulsion-nuclei experiments. We find that the only acceptable $\Xi^-_{1s}$ assignment at present, barring an abnormally strong repulsive $\rho^2$ component of $V_{\rm opt}^{\Xi}(\rho)$, is that for the $\Xi^--{^{11}{\rm B}}$ signal. This finding supports reassigning $\Xi^-$ capture events in $^{14}$N, originally assigned as $\Xi^-_{1s}-{^{14}{\rm N}}$ nuclear states, to $\Xi^0_{1p}-{^{14}{\rm C}}$ nuclear states. The depth of $V_{\rm opt}^{\Xi}(\rho)$ at nuclear-matter density $\rho_0=0.17$ fm$^{-3}$ is then $-V_{\rm opt}^{\Xi}(\rho_0)\sim 21$ MeV.

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Hypertriton lifetime

Over the last decade, conflicting values of the hypertriton ${}_{\Lambda}^3\mathrm{H}$ lifetime $\tau({}_{\Lambda}^3\mathrm{H})$ were extracted from relativistic heavy-ion (RHI) collision experiments, ranging from values compatible with the free-$\Lambda$ lifetime $\tau_\Lambda$-as expected naively for a very weakly bound $\Lambda$ in ${}_{\Lambda}^3\mathrm{H}$-to lifetimes as short as $\tau({}_{\Lambda}^3\mathrm{H}) \approx (0.4-0.7)\,\tau_\Lambda$. In a recent work [Phys. Lett. B 811, 135916 (2020)] we studied this ${}_{\Lambda}^3\mathrm{H}$ lifetime puzzle theoretically using realistic three-body ${}_{\Lambda}^3\mathrm{H}$ and ${}^3\mathrm{He}$ wave functions computed within the ab initio no-core shell model approach with interactions derived from chiral effective field theory. In particular, $\tau({}_{\Lambda}^3\mathrm{H})$ was found to be strongly correlated with the $\Lambda$ separation energy $B_\Lambda$ in ${}_{\Lambda}^3\mathrm{H}$, the value of which is rather poorly known experimentally and, in addition, is known to suffer from sizable theoretical uncertainties inherent in the employed nuclear and hypernuclear interaction models. In the present work we find that these uncertainties propagate into $\tau({}_{\Lambda}^3\mathrm{H})$, and thus limit considerably the theoretical precision of its computed value. Although none of the conflicting RHI measured $\tau({}_{\Lambda}^3\mathrm{H})$ values can be excluded, but rather can be attributed to a poor knowledge of $B_\Lambda$, we note the good agreement between the lifetime value $\tau({}_{\Lambda}^3\mathrm{H})=238(27)$ ps computed at the lowest value $B_\Lambda=66$ keV reached by us and the very recent ALICE measured lifetime value $\tau^{\mathrm{ALICE}}({}_{\Lambda}^3\mathrm{H})=253(11)(6)$ ps associated with the ALICE measured $B_\Lambda$ value $B^{\mathrm{ALICE}}_\Lambda=102(63)(67)$ keV [Phys. Rev. Lett. 131, 102302 (2023)].

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$\Lambda$ hypernuclear potentials beyond linear density dependence

In a recent paper [PLB 837 (2023) 137669] we showed that all measured ($1s_\Lambda$, $1p_\Lambda$) pairs of $\Lambda$ binding energies in $\Lambda$-hypernuclei across the periodic table, $12\leq A \leq 208$, can be obtained from a $\Lambda$-nucleus optical potential with only two adjustable $\Lambda N$ and $\Lambda NN$ parameters, associated with leading linear and quadratic terms in the nuclear density, derived by fitting $^{16}_{~\Lambda}$N binding energies. Here we extend the previous analysis by performing least-squares fits to the full set of data points. Consequences of suppressing $\Lambda NN$ interactions between `core' nucleons and `excess' neutrons are studied and related predictions are made for ($1s_\Lambda$, $1p_\Lambda$) binding energies in $^{40,48}_{~~~~\Lambda}$K, obtainable from upcoming $^{40,48}$Ca($e,e'K^+$) JLab experiments. We find $\Lambda$-nucleus partial potential depths of $D^{(2)}_\Lambda = -38.6\pm 0.8$~MeV ($\Lambda N$) and $D^{(3)}_\Lambda = 11.3\pm 1.4$~MeV ($\Lambda NN$), with a total depth $D_\Lambda = -27.3\pm 0.6$~MeV at nuclear-matter density $\rho_0$=0.17~fm$^{-3}$, consistently with our previous results. Extrapolation to higher nuclear densities and possible relevance to the `hyperon puzzle' in neutron-star matter are discussed.

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Lifetime of the hypertriton

Conflicting values of the hypertriton lifetime $\tau({}_\Lambda^3\mathrm{H})$ were derived in relativistic heavy ion (RHI) collision experiments over the last decade. A very recent ALICE Collaboration measurement is the only experiment where the reported $\tau({}_\Lambda^3\mathrm{H})$ comes sufficiently close to the free-$\Lambda$ lifetime $\tau_\Lambda$,as expected naively for a very weakly bound $\Lambda$ in ${}_\Lambda^3\mathrm{H}$. We revisited theoretically this ${}_\Lambda^3\mathrm{H}$ lifetime puzzle, using ${}_\Lambda^3\mathrm{H}$ and ${}^3\mathrm{He}$ wave functions computed within the abinitio no-core shell model employing interactions derived from chiral effective field theory to calculate the two-body decay rate $\Gamma({}_\Lambda^3\mathrm{H}\to{}^3\mathrm{He}+\pi^-)$. We found significant but opposing contributions arising from $\Sigma NN$ admixtures in ${}_\Lambda^3\mathrm{H}$ and from $\pi^- -{}^3\mathrm{He}$ final-state interaction. To derive $\tau({}_\Lambda^3\mathrm{H})$, we evaluated the inclusive $\pi^-$ decay rate $\Gamma_{\pi^-}({}_\Lambda^3\mathrm{H})$ by using the measured branching ratio $\Gamma({}_\Lambda^3\mathrm{H}\to{}^3\mathrm{He}+\pi^-)/\Gamma_{\pi^-}({}_\Lambda^3\mathrm{H})$ and added the $\pi^0$ contributions through the $\Delta I = \frac{1}{2}$ rule. The resulting $\tau({}_\Lambda^3\mathrm{H})$ varies strongly with the rather poorly known $\Lambda$ separation energy $E_{\mathrm{sep}}({}_\Lambda^3\mathrm{H})$ and it is thus possible to associate each one of the distinct RHI $\tau({}_\Lambda^3\mathrm{H})$ measurements with its own underlying value of $E_{\mathrm{sep}}({}_\Lambda^3\mathrm{H})$.

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Has J-PARC E07 observed a $\Xi^-_{1s}$ nuclear state?

The Strangeness ${\cal S}=-2$ J-PARC E07 emulsion experiment published recently two new $\Xi^-$--$^{14}$N capture events, IRRAWADDY and IBUKI, identified by observing weak-decay sequences of pairs of single-$\Lambda$ hypernuclei and interpreted as $\Xi^{-}_{1s}$ and $\Xi^{-}_{1p}$ nuclear bound states, respectively, with binding energies $B_{\Xi^-}^{1s}$=6.27$\pm$0.27 MeV and $B_{\Xi^-}^{1p}$=1.27$\pm$0.21 MeV. $\Xi^-$ capture events in emulsion play a major role in determining the $\Xi$-nuclear and the $\Lambda\Lambda$ potential strengths. Here we question the assignment of a $\Xi^{-}_{1s}$ nuclear bound state to IRRAWADDY and offer an alternative assignment as a near-threshold $\Xi^0_{1p}$--$^{14}$C nuclear bound state, slightly admixed with a $\Xi^{-}_{1p}$--$^{14}$N nuclear bound state component corresponding to IBUKI. We also question using IBUKI's $B_{\Xi^-}^{1p}$ value as is to determine the $\Xi$-nuclear potential depth. Altogether, $\Xi^-$ capture events in $^{12}$C and $^{16}$O should prove less ambiguous than in $^{14}$N.

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Constraints from $\Lambda$ hypernuclei on the $\Lambda NN$ content of the $\Lambda$-nucleus potential

A depth of $D_{\Lambda}\approx -28$ MeV for the $\Lambda$-nucleus potential was confirmed in 1988 by studying $\Lambda$ binding energies deduced from $(\pi^+,K^+)$ spectra measured across the periodic table. Modern two-body hyperon-nucleon interaction models require additional interaction terms, most likely $\Lambda NN$ three-body terms, to reproduce $D_{\Lambda}$. In this work we apply a suitably constructed $\Lambda$-nucleus density dependent optical potential to binding energy calculations of observed $1s_{\Lambda}$ and $1p_{\Lambda}$ states in the mass range $12\leq A\leq 208$. The resulting $\Lambda NN$ contribution to $D_{\Lambda}$, about 14 MeV repulsion at symmetric nuclear matter density $\rho_0=0.17$ fm$^{-3}$, makes $D_{\Lambda}$ increasingly repulsive at $\rho\gtrsim 3\rho_0$, leading possibly to little or no $\Lambda$ hyperon content of neutron-star matter. This suggests in some models a stiff equation of state that may support two solar-mass neutron stars.

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In-medium $\Lambda$ isospin impurity from charge symmetry breaking in the ${_{\Lambda}^4}{\rm H}-{_{\Lambda}^4}{\rm He}$ mirror hypernuclei

The $\Lambda$ separation energies in the mirror hypernuclei ${_{\Lambda}^4}{\rm H}-{_{\Lambda}^4}{\rm He}$ exhibit large charge symmetry breaking (CSB). Analyzing this CSB within pionless effective field theory while using partially conserved baryon-baryon SU(3) flavor symmetry, we deduce a $\Lambda -\Sigma^0$ induced in-medium admixture amplitude ${\cal A}_{I=1}\approx 1.5\%$ in the dominantly isospin $I=0$ $\Lambda$ hyperon. Our results confirm the free-space value ${\cal A}^{(0)}_{I=1}$ inferred directly within the SU(3) baryon octet by Dalitz and von-Hippel in 1964 and reaffirmed in a recent QCD+QED lattice calculation. Furthermore, exploring the consequences of SU(3) flavor symmetry on the $\Lambda$-nucleon interaction, we find that CSB is expected to impact the $S=1$ and $S=0$ spin channels in opposite directions, with the latter dominating by an order of magnitude. These observations explain a recent deduction of $\Lambda$-nucleon CSB strengths.

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Consequences of increased hypertriton binding for $s$-shell $Λ$-hypernuclear systems

Consequences of increasing the binding energy of the hypertriton ground state ${_Λ^3}{\rm H}(J^P={\frac{1}{2}}^+)$ from the emulsion value $B^{\rm EMUL}_Λ({_Λ^3}{\rm H}_{\rm g.s.})$=0.13$\pm$0.05 MeV to the STAR value $B^{\rm STAR}_Λ(^{3}_Λ{\rm H}) = (0.41\pm 0.12 \pm 0.11)$ MeV are studied for $s$-shell hypernuclei within a pionless EFT approach at leading order, constrained by the binding energies of the $0^+$ and $1^+$ ${_Λ^4} {\rm H}$ states. The stochastic variational method is used in bound-state calculations, whereas the inverse analytic continuation in the coupling constant method is used to locate $S$-matrix poles of continuum states. It is found that the $Λnn({\frac{1}{2}}^+)$ resonance becomes broader and less likely to be observed experimentally, whereas the ${_Λ^3}{\rm H}({\frac{3}{2}}^+)$ spin-flip virtual state moves closer to the $Λd$ threshold to become a shallow bound state for specific $ΛN$ interaction strengths. The effect of such a near-threshold ${_Λ^3}{\rm H}({\frac{3}{2}}^+)$ state on femtoscopic studies of $Λ$-deuteron correlations, and its lifetime if bound, are discussed. Increasing $B_Λ({_Λ^3} {\rm H}_{\rm g.s.})$ moderately, up to $\sim$0.5 MeV, hardly affects calculated values of $B_Λ({_Λ^5}{\rm He})$.

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First demonstration of in-beam performance of bent Monolithic Active Pixel Sensors

A novel approach for designing the next generation of vertex detectors foresees to employ wafer-scale sensors that can be bent to truly cylindrical geometries after thinning them to thicknesses of 20-40$μ$m. To solidify this concept, the feasibility of operating bent MAPS was demonstrated using 1.5$\times$3cm ALPIDE chips. Already with their thickness of 50$μ$m, they can be successfully bent to radii of about 2cm without any signs of mechanical or electrical damage. During a subsequent characterisation using a 5.4GeV electron beam, it was further confirmed that they preserve their full electrical functionality as well as particle detection performance. In this article, the bending procedure and the setup used for characterisation are detailed. Furthermore, the analysis of the beam test, including the measurement of the detection efficiency as a function of beam position and local inclination angle, is discussed. The results show that the sensors maintain their excellent performance after bending to radii of 2cm, with detection efficiencies above 99.9% at typical operating conditions, paving the way towards a new class of detectors with unprecedented low material budget and ideal geometrical properties.

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Constraints on $Ξ^-$ nuclear interactions from capture events in emulsion

Five $Ξ^- p\to ΛΛ$ two-body capture events in $^{12}$C and $^{14}$N emulsion nuclei, in which a pair of single-$Λ$ hypernuclei is formed and identified by their weak decay, have been observed in $(K^-,K^+)$ emulsion exposures at KEK and J-PARC. Applying a $Ξ^-$-nucleus optical potential methodology to study atomic and nuclear transitions, we confirm that these capture events occur from Coulomb assisted $1p_{Ξ^-}$ nuclear states. Long-range $ΞN$ shell-model correlations are found essential to achieve consistency between the $^{12}$C and $^{14}$N events. The resulting $Ξ$-nuclear interaction is strongly attractive, with $Ξ$ potential depth in nuclear matter $V_Ξ\gtrsim 20$ MeV. Implications to multi-strangeness features of dense matter are outlined.

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On the width of the $K^-$D atom ground state

Experiments at DA$Φ$NE-Frascati and at J-PARC are scheduled to produce $K^-$D atoms and observe their X-ray cascade down to the 1$S$ ground state (g.s.), thereby measuring its strong-interaction width and shift away from a purely Coulomb state. A width $Γ_{1S}\lesssim 1$ keV will ensure good resolution of the X-ray transitions feeding the 1$S$ g.s. Here we study the expected $K^-$D 1$S$ g.s. width from the perspective of global fits to level shifts and widths in heavier kaonic atoms across the periodic table, using $K^-$ nuclear optical potentials constructed from $\bar K N$ chiral interaction models. Special attention is paid to the subthreshold energy at which the $\bar K N$ subsystem interacts in the $K^-$D atomic g.s. Within this approach we predict strong-interaction upward level shift of close to 700 eV and width of about 1.2 to 1.3 keV for the $K^-$D atom 1$S$ g.s., in fair agreement with genuinely three-body $K^-$D atom calculations. Comparison is made with $π^-$D atom phenomenology.

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Revisiting the hypertriton lifetime puzzle

Conflicting values of the hypertriton ($_Λ^{3}$H) lifetime were extracted in recent relativistic heavy-ion collision experiments. The ALICE Collaboration's reported $_Λ^{3}$H lifetime $τ(_Λ^{3}$H) is compatible within measurement uncertainties with the free $Λ$ lifetime $τ_Λ$, as naively expected for a loosely bound $Λ$ hyperon in $_Λ^{3}$H, whereas STAR's reported range of $τ(_Λ^{3}$H) values is considerably shorter: $τ_{\rm STAR}(_Λ^{3}$H)$\sim$(0.4-0.7)$τ_Λ$. This $_Λ^{3}$H lifetime puzzle is revisited theoretically using $_Λ^{3}$H three-body wavefunctions generated in a chiral effective field theory approach to calculate the decay rate $Γ(_Λ^{3}$H$\,\to ^3$He$\,+π^-$). Significant but opposing contributions arise from $ΣNN$ admixtures in $_Λ^{3}$H and from $π^-$-$^3$He final-state interaction. Evaluating the inclusive $π^-$ decay rate $Γ_{π^-}(_Λ^{3}$H) via a branching ratio $Γ(_Λ^{3}$H$\,\to ^{3}$He+$π^-)/Γ_{π^-}(_Λ^{3}$H) determined in helium bubble-chamber experiments, and adding $Γ_{π^0}(_Λ^{3}$H) through the $ΔI=\frac{1}{2}$ rule, we derive $τ(_Λ^{3}$H) assuming several different values of the $Λ$ separation energy $B_Λ(_Λ^{3}$H). It is concluded that each of ALICE and STAR reported $τ(_Λ^{3}$H) intervals implies its own constraint on $B_Λ(_Λ^{3}$H): $B_Λ\lesssim 0.1$ MeV for ALICE, $B_Λ\gtrsim 0.2$ MeV for STAR.

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$Λ^*$ matter and its stability

We performed calculations of nuclear systems composed solely of $Λ^*$ hyperons, aiming at exploring the possibility of existence of absolutely stable $Λ^*$ matter. We considered $Λ^*$ interaction strengths compatible with the $Λ^*Λ^*$ binding energy $B_{Λ^*Λ^*}$ given by the $\bar{K}N$ interaction model by Yamazaki and Akaishi [1]. We found that the binding energy per $Λ^*$ saturates at values well below 100 MeV for mass number $A\geq120$. The $Λ^*$ matter is thus highly unstable against strong interaction decay.

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The onset of $ΛΛ$ hypernuclear binding

Binding energies of light, $A\leq 6$, $ΛΛ$ hypernuclei are calculated using the stochastic variational method in a pionless effective field theory (EFT) approach at leading order with the purpose of assessing critically the onset of binding in the strangeness S=-2 hadronic sector. The EFT input in this sector consists of (i) a $ΛΛ$ contact term constrained by the $ΛΛ$ scattering length $a_{ΛΛ}$, using a range of values compatible with $ΛΛ$ correlations observed in relativistic heavy ion collisions, and (ii) a $ΛΛN$ contact term constrained by the only available $A\leq 6$ $ΛΛ$ hypernucler binding energy datum of $^{6}_{ΛΛ}$He. The recently debated neutral three-body and four-body systems $^{3}_{ΛΛ}$n and $^{4}_{ΛΛ}$n are found unbound by a wide margin. A relatively large value of $|a_{ΛΛ}| \gtrsim 1.5$ fm is needed to bind $^{4}_{ΛΛ}$H, thereby questioning its particle stability. In contrast, the particle stability of the $A=5$ $ΛΛ$ hypernuclear isodoublet $^{5}_{ΛΛ} $H--$^{5}_{ΛΛ}$He is robust, with $Λ$ separation energy of order 1 MeV.

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The pion-nucleon $σ$ term from pionic atoms

Earlier work suggested that the in-medium $πN$ threshold isovector amplitude $b_1(ρ)$ gets renormalized in pionic atoms by about 30% away from its $ρ=0$ free-space value, relating such renormalization to the leading low-density decrease of the in-medium quark condensate $<\bar q q>$ and the pion decay constant $f_π$ in terms of the pion-nucleon $σ$ term $σ_{πN}$. Accepting the validity of this approach, we extracted $σ_{πN}$ from a large-scale fit of pionic-atom level shift and width data across the periodic table. Our fitted value $σ_{πN}=57\pm 7$ MeV is robust with respect to variation of $πN$ interaction terms other than the isovector $s$-wave term with which $σ_{πN}$ was associated. Higher order corrections to the leading order in density involve some cancellations, suggesting thereby only a few percent overall systematic uncertainty. The value of $σ_{πN}$ derived here agrees with values obtained in several recent studies based on near-threshold $πN$ phenomenology, but sharply disagrees with values obtained in recent direct lattice QCD calculations.

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On the Stability of $Λ(1405)$ Matter

A hypothesis of absolutely stable strange hadronic matter composed of $Λ(1405)$ baryons, here denoted $Λ^*$, is tested within many-body calculations performed using the Relativistic Mean-Field approach. In our calculations, we employed the $Λ^*Λ^*$ interaction compatible with the $Λ^*Λ^*$ binding energy $B_{Λ^*Λ^*}=40$~MeV given by the phenomenological energy-independent $\bar{K}N$ interaction model by Yamazaki and Akaishi (YA). We found that the binding energy per $Λ^*$, as well as the central density in $Λ^*$ many-body systems saturates for mass number $A\geq120$, leaving $Λ^*$ aggregates highly unstable against strong interaction decay. Moreover, we confronted the YA interaction model with kaonic atom data and found that it fails to reproduce the $K^-$ single-nucleon absorption fractions at rest from bubble chamber experiments.

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Eta-mesic nuclei

In this contribution we report on theoretical studies of $η$ nuclear quasi-bound states in few- and many-body systems performed recently by the Jerusalem-Prague Collaboration [1-5]. Underlying energy-dependent $ηN$ interactions are derived from coupled-channel models that incorporate the $N^*(1535)$ resonance. The role of self-consistent treatment of the strong energy dependence of subthreshold $ηN$ amplitudes is discussed. Quite large downward energy shift together with rapid decrease of the $ηN$ amplitudes below threshold result in relatively small binding energies and widths of the calculated $η$ nuclear bound states. We argue that the subthreshold behavior of $ηN$ scattering amplitudes is crucial to conclude whether $η$ nuclear states exist, in which nuclei the $η$ meson could be bound and if the corresponding widths are small enough to allow detection of these $η$ nuclear states in experiment.

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