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E. Hiyama

Publications and source records attributed to E. Hiyama.

At least 19 recordsLinked to original sources

Cluster phenomena using few-body and Lattice QCD theories

With the advancement of first-principles calculations for baryon-baryon interactions, it becomes possible to obtain reliable hyperon-nucleon potentials by lattice QCD simulations with the HAL QCD method. High-precision few-body methods, such as the Gaussian Expansion Method (GEM), are applicable to solve quantum few-body systems up to four- and five-body systems. By combining the HAL QCD potentials with the GEM, one can predict the level structure of novel hypernuclei prior to experimental observation. In this review, we utilize the lattice QCD $NΞ$ potential obtained by the HAL QCD method to investigate the few-body systems $NNΞ$ and $NNNΞ$. Our analysis indicates that the lightest bound $Ξ$ hypernucleus is the $NNNΞ$ system. To extract detailed information on the isospin and spin components of the $NΞ$ interaction, we perform a four-body calculation for the $ααNΞ$ system with the total isospin $T = 0$ and $T = 1$. We demonstrate that the level structure of this system is sensitive to the isospin and spin dependencies of the $NΞ$ interaction. Furthermore, we propose experimental investigations to produce the $NNNΞ$ and $ααNΞ$ systems via the $(K^-, K^+)$ and $(K^-, K^0)$ reactions on $^4$He and $^{10}$B targets, respectively.

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Mini-Proceedings of the "Fourth International Workshop on the Extension Project for the J-PARC Hadron Experimental Facility (HEF-ex 2024)"

The mini proceedings of the "Fourth International Workshop on the Extension Project for the J-PARC Hadron Experimental Facility (HEF-ex 2024) [https://kds.kek.jp/event/46965]" held at J-PARC, February 19-21, 2024, are presented. The workshop was devoted to discussing the physics case that connects both the present and the future Hadron Experimental Facility at J-PARC, covering a wide range of topics in flavor, hadron, and nuclear physics related to both experimental and theoretical activities being conducted at the facility.

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Probing $ΞN$ interaction through inversion of spin-doublets in $ΞN αα$ nuclei

A new way to study the spin-isospin dependence of the $ΞN$ interaction is explored through the energy levels of $ΞNα$ and $ΞNαα$ systems with $α$ being a spectator to attract the $ ΞN$ pair without changing its spin-isospin structure. By using the Gaussian expansion method (GEM) with the state-of-the-art $ΞN$ potential obtained from lattice QCD calculations, it is found that $ΞNαα$ has spin-doublet bound states with $J^π={1^-}$ and $2^-$ in both isospin triplet and singlet channels. The inversion of the $1^-$-$2^-$ spin-doublet between the iso-triplet and the iso-singlet is found to be strongly correlated with the relative strengths of the $ΞN$ interaction in the $^{11}{\rm S}_0, ^{13}{\rm S}_1,^{31}{\rm S}_0$ and $^{33}{\rm S}_1$ channels. The $(K^-, K^+)$ and $(K^-,K^0)$ reactions on the $^{10}$B target are proposed to produce those bound states.

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19B isotope as a 17B-n-n three-body cluster close to unitary limit

We describe 19B in terms of a 17B-n-n three-body system, where the two-body subsystems 17B-n and n-n are unbound (virtual) states close to the unitary limit. The energy of 19B ground state is well reproduced and two low-lying resonances are predicted. Their eventual link with the Efimov physics is discussed. This model can be extended to describe the recently discovered resonant states in 20,21B.

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Stable double-heavy tetraquarks: spectrum and structure

Bound states of double-heavy tetraquarks are studied in a constituent quark model. Two bound states are found for isospin and spin-parity I(J^P ) = 0(1^+) in the bb\bar{u}\bar{d} channel. One is deeply bound and compact made of colored diquarks, while the other is shallow and extended as a BB^* molecule. The former agrees well with lattice QCD results. A systematic decrease in the binding energy is seen by replacing one of the heavy quarks to a lighter one. Altogether we find ten bound states. It is shown for the first time that hadrons with totally different natures emerge from a single Hamiltonian.

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Possible lightest $Ξ$ Hypernucleus with Modern $ΞN$ Interactions

Experimental evidence exists that the $Ξ$-nucleus interaction is attractive. We search for $NNΞ$ and $NNNΞ$ bound systems on the basis of the AV8 $NN$ potential combined with either a phenomenological Nijmegen $ΞN$ potential or a first principles HAL QCD $ΞN$ potential. The binding energies of the three-body and four-body systems (below the $d+Ξ$ and $^3{\rm H}$/$^3{\rm He}+Ξ$ thresholds, respectively) are calculated by a high precision variational approach, the Gaussian Expansion Method. Although the two $ΞN$ potentials have significantly different isospin ($T$) and spin ($S$) dependence, the $NNNΞ$ system with quantum numbers $(T=0, J^π=1^+$) appears to be bound (one deep for Nijmegen and one shallow for HAL QCD) below the $^3{\rm H}$/$^3{\rm He}+Ξ$ threshold. Experimental implications for such a state are discussed.

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Efimov universality with Coulomb interaction

The universal properties of charged particles are modified by the presence of a long-range Coulomb interaction. We investigate the modification of Efimov universality as a function of the Coulomb strength using the Gaussian expansion method. The resonant short-range interaction is described by Gaussian potentials to which a Coulomb potential is added. We calculate binding energies and root mean square radii for the three- and four-body systems of charged particles and present our results in a generalised Efimov plot. We find that universal features can still be discerned for weak Coulomb interaction, but break down for strong Coulomb interaction. The root-mean-square radius plateaus at increasingly smaller values for strong Coulomb interaction and the probablity distributions of the states become more concentrated inside the Coulomb barrier. As an example, we apply our universal model to nuclei with an alpha-cluster substructure. Our results point to strong non-universal contributions in that sector.

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Ab initio calculations of 5H resonant states

By solving the 5-body Faddeev-Yakubovsky equations in configuration space with realistic nuclear Hamiltonians we have studied the resonant states of $^5$H isotope. Two different methods, allowing to bypass the exponentially diverging boundary conditions, have been employed providing consistent results. The existence of $^5$H broad J$^π$=1/2$^+$,3/2$^+$,5/2$^+$ states as S-matrix poles has been confirmed and compared with the, also calculated, resonant states in $^4$H isotope. We have established that the positions of these resonances only mildly depend on the nuclear interaction model.

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Multi-cluster dynamics in $^{13}_Λ{\rm C}$ and analogy to clustering in $^{12}{\rm C}$

We investigate structure of $^{13}_Λ{\rm C}$ and discuss the difference and similarity between the structures of $^{12}{\rm C}$ and $^{13}_Λ{\rm C}$ by answering the questions if the linear-chain and gaslike cluster states, which are proposed to appear in $^{12}{\rm C}$, survives, or new structure states appear or not. We introduce a microscopic cluster model called, Hyper-Tohsaki-Horiuchi-Schuck-Röpke (H-THSR) wave function, which is an extended version of the THSR wave function so as to describe $Λ$ hypernuclei. We obtained two bound states and two resonance (quasi-bound) states for $J^π=0^+$ in $^{13}_Λ{\rm C}$, corresponding to the four $0^+$ states in $^{12}{\rm C}$. However, the inversion of level ordering between the spectra of $^{12}{\rm C}$ and $^{13}_Λ{\rm C}$, i.e. that the $0_3^+$ and $0_4^+$ states in $^{13}_Λ{\rm C}$ correspond to the $0_4^+$ and $0_3^+$ states in $^{12}{\rm C}$, respectively, is shown to occur. The additional $Λ$ particle reduces sizes of the $0_2^+$ and $0_3^+$ states in $^{13}_Λ{\rm C}$ very much, but the shrinkage of the $0_4^+$ state is only a half of the other states. In conclusion, the Hoyle state becomes quite a compact object with ${^{9}_Λ{\rm Be}}+α$ configuration in $^{13}_Λ{\rm C}$ and is no more gaslike state composed of the $3α$ clusters. Instead, the $0_4^+$ state in $^{13}_Λ{\rm C}$, coming from the $^{12}{\rm C}(0_3^+)$ state, appears as a gaslike state composed of $α+α+^{5}_Λ{\rm He}$ configuration, i.e. the Hoyle analog state. A linear-chain state in a $Λ$ hypernucleus is for the first time predicted to exist as the $0_3^+$ state in $^{13}_Λ{\rm C}$ with more shrunk arrangement of the $3α$ clusters along $z$-axis than the $3α$ linear-chain configuration realized in the $^{12}{\rm C}(0_4^+)$ state.

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Tetramer Bound States in Heteronuclear Systems

We calculate the universal spectrum of trimer and tetramer states in heteronuclear mixtures of ultracold atoms with different masses in the vicinity of the heavy-light dimer threshold. To extract the energies, we solve the three- and four-body problem for simple two- and three-body potentials tuned to the universal region using the Gaussian expansion method. We focus on the case of one light particle of mass $m$ and two or three heavy bosons of mass $M$ with resonant heavy-light interactions. We find that trimer and tetramer cross into the heavy-light dimer threshold at almost the same point and that as the mass ratio $M/m$ decreases, the distance between the thresholds for trimer and tetramer states becomes smaller. We also comment on the possibility of observing exotic three-body states consisting of a dimer and two atoms in this region and compare with previous work.

cond-mat.quant-gas

Mean field approaches for $Ξ^-$ hypernuclei and current experimental data

Motivated by the recently observed hypernucleus (Kiso event) $^{15}_Ξ$C ($^{14}$N$+Ξ^-$), we identify the state of this system theoretically within the framework of the relativistic-mean-field and Skyrme-Hartree-Fock models. The $ΞN$ interactions are constructed to reproduce the two possibly observed $Ξ^-$ removal energies, $4.38\pm 0.25$ MeV or $1.11\pm 0.25$ MeV. The present result is preferable to be $^{14}{\rm N}({\rm g.s.})+Ξ^-(1p)$, corresponding to the latter value.

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Sensitivity of Λ single-particle energies to the ΛN spin-orbit coupling and to nuclear core structure in p-shell and sd-shell hypernuclei

We introduce a mean field model based on realistic 2-body baryon interactions and calculate spectra of a set of p-shell and sd-shell Λ hypernuclei - 13ΛC, 17ΛO, 21ΛNe, 29ΛSi and 41ΛCa. The hypernuclear spectra are compared with the results of a relativistic mean field (RMF) model and available experimental data. The sensitivity of Λ single-particle energies to the nuclear core structure is explored. Special attention is paid to the effect of spin-orbit ΛN interaction on the energy splitting of the Λ single particle levels 0p3/2 and 0p1/2. In particular, we analyze the contribution of the symmetric (SLS) and the anti-symmetric (ALS) spin-orbit terms to the energy splitting. We give qualitative predictions for the calculated hypernuclei.

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On the possibility of generating a 4-neutron resonance with a {\boldmath $T=3/2$} isospin 3-neutron force

We consider the theoretical possibility to generate a narrow resonance in the four neutron system as suggested by a recent experimental result. To that end, a phenomenological $T=3/2$ three neutron force is introduced, in addition to a realistic $NN$ interaction. We inquire what should be the strength of the $3n$ force in order to generate such a resonance. The reliability of the three-neutron force in the $T=3/2$ channel is exmined, by analyzing its consistency with the low-lying $T=1$ states of $^4$H, $^4$He and $^4$Li and the $^3{\rm H} + n$ scattering. The {\it ab initio} solution of the $4n$ Schrödinger equation is obtained using the complex scaling method with boundary conditions appropiate to the four-body resonances. We find that in order to generate narrow $4n$ resonant states a remarkably attractive $3N$ force in the $T=3/2$ channel is required.

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Equation of state for neutron stars with hyperons by the variational method

We investigate the effects of the odd-state part of bare $ΛΛ$ interactions on the structure of neutron stars (NSs) by constructing equations of state (EOSs) for uniform nuclear matter containing $Λ$ and $Σ^-$ hyperons with use of the cluster variational method. The isoscalar part of the Argonne v18 two-nucleon potential and the Urbana IX three-nucleon potential are employed as the interactions between nucleons, whereas, as the bare $ΛN$ and even-state $ΛΛ$ interactions, two-body central potentials that are determined so as to reproduce the experimental data on single- and double-$Λ$ hypernuclei are adopted. In addition, the $Σ^- N$ interaction is constructed so as to reproduce the empirical single-particle potential of $Σ^-$ in symmetric nuclear matter. Since the odd-state part of the $ΛΛ$ interaction is not known owing to lack of experimental data, we construct four EOSs of hyperonic nuclear matter, each with a different odd-state part of the $ΛΛ$ interaction. The EOS obtained for NS matter becomes stiffer as the odd-state $ΛΛ$ interaction becomes more repulsive, and correspondingly the maximum mass of NSs increases. It is interesting that the onset density of $Σ^-$ depends strongly on the repulsion of the odd-state $ΛΛ$ interaction. Furthermore, we take into account the three-baryon repulsive force to obtain results that are consistent with observational data on heavy NSs.

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The radiative capture reaction rate from $ΛΛ$ to H dibaryon in the imaginary time method

Radiative capture rates of thermal $ΛΛ+ Ξ$N states into H dibaryon are calculated in the novel imaginary time method. The H dibaryon is assumed to be a bound state of $Ξ$N with spin $J^π= 0^+$, isospin $I=0$ and strangeness $-2$. We consider $E1$ transition to H from $Ξ$N $(L=1)$ scattering states which mix with $ΛΛ(L=1)$. In order to calculate the transition rates, we formulate a coupled-channel imaginary time method by extending the one-channel formula originally proposed by Yabana and Funaki. The imaginary time method allows us to avoid the sum over all the excited thermal initial states, and thus to save computational time significantly. The transition rates are given as a function of temperature and the unknown binding energy of the H dibaryon, which we take as a parameter. It is found that the transition rate is not sensitive to the choices of the H binding energy or the strengths of the channel coupling for temperatures 3 MeV or higher.

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Resonant states of neutron-rich $Λ$ hypernucleus $^7_Λ$He

The structure of neutron-rich $Λ$ hypernucleus, $^7_Λ$He is studied within the framework of an $α+Λ+n+n$ four-body cluster model. We predict second $3/2^+$ and $5/2^+$ states, corresponding to a $0s$ $Λ$ coupled to the second $2^+$ state of $^6$He, as narrow resonant states with widths $Γ\sim 1$ MeV to be at 0.03 MeV and 0.07 MeV respect to the $α+Λ+n+n$ threshold. From an estimation of the differential cross section for the $^7{\rm Li} (γ,K^+) ^7_Λ$He reaction, there is a possibility to observe these state at JLab in the future. We also calculate the second $2^+$ state of $^6$He as resonant state within the framework of an $α+n+n$ three-body cluster model. Our result is $2.81$ MeV with $Γ=$4.63 MeV with respect to the $α+n+n$ threshold. This energy position is $\sim 1$ MeV higher, and with a much broader decay width, than the recent SPIRAL data. It is suggested that an experiment at JLab to search for the second $3/2^+$ and $5/2^+$ states of $^7_Λ$He would provide an opportunity to confirm the second $2^+$ state of the core nucleus $^6$He.

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Universality in Efimov associated tetramers in 4He

We calculated, using seven realistic 4He-4He potentials in the literature, the Efimov spectra of the 4He trimer and tetramer and analyzed the universality of the systems. The three-(four-)body Schroedinger equations were solved fully nonadiabatically with the high-precision calculation method employed in our previous work on the 4He trimer and tetramer [Phys. Rev. A 85, 022502 (2012); 85, 062505 (2012)]. We found the following universality in the four-boson system: i) The critical scattering lengths at which the tetramer ground and excited states couple to the four-body threshold are independent of the choice of the two-body realistic potentials in spite of the difference in the short-range details and do not contradict the corresponding values observed in the experiments in ultracold alkali atoms when scaled with the van der Waals length r_vdW, and ii) the four-body hyperradial potential has a repulsive barrier at the four-body hyperradius R_4 \approx 3 r_vdW, which prevents the four particles from getting close together to explore nonuniversal features of the interactions at short distances. This result is an extension of the universality in Efimov trimers that the appearance of the repulsive barrier at the three-body hyperradius R_3 \approx 2 r_vdW makes the critical scattering lengths independent of the short-range details of the interactions as reported in the literature and also in the present work for the 4He trimer with the realistic potentials.

cond-mat.quant-gas

Container structure of alpha alpha Lambda clusters in $_Λ^9$Be

New concept of clustering is discussed in $Λ$ hypernuclei using a new-type microscopic cluster model wave function, which has a structure that constituent clusters are confined in a container, whose size is a variational parameter and which we refer to as Hyper-Tohsaki-Horiuchi-Schuck-Röpke (Hyper-THSR) wave function. By using the Hyper-THSR wave function, $2α+ Λ$ cluster structure in ${^{9}_Λ{\rm Be}}$ is investigated. We show that full microscopic solutions in the $2α+ Λ$ cluster system, which are given as $2α+ Λ$ Brink-GCM wave functions, are almost perfectly reproduced by the single configurations of the Hyper-THSR wave function. The squared overlaps between the both wave functions are calculated to be $99.5$%, $99.4$%, and $97.7$% for $J^π=0^+$, $2^+$, and $4^+$ states, respectively. We also simulate the structural change by adding the $Λ$ particle, by varying the $ΛN$ interaction artificially. As the increase of the $ΛN$ interaction, the $Λ$ particle gets to move more deeply inside the core and invokes strongly the spatial core shrinkage, and accordingly distinct localized $2α$ clusters appear in the nucleonic intrinsic density, though in ${^{8}{\rm Be}}$ rather gaslike $2α$-cluster structure is shown. The origin of the localization is associated with the strong effect of Pauli principle. We conclude that the container picture of the $2α$ and $Λ$ clusters is essential in understanding the cluster structure in ${^{9}_Λ{\rm Be}}$, in which the very compact spatial localization of clusters is shown in the density distribution.

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