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Faisal Etminan

Publications and source records attributed to Faisal Etminan.

At least 19 recordsLinked to original sources

Symmetry-Reduced Variational Quantum Simulation of the $U(5)\rightarrow SU(3)$ Quantum Phase Transition in the Interacting Boson Model

The spherical-to-deformed quantum phase transition of the Interacting Boson Model (IBM) is investigated using the variational quantum eigensolver (VQE). The $U(5)$--$SU(3)$ transitional Hamiltonian is studied with $χ=-\sqrt{7}/2$. We develop a symmetry-preserving, minimum-qubit VQE framework for collective nuclear models, achieving a substantial reduction in qubit requirements without compromising the finite-size quantum-phase-transition physics. The transition is characterized through the normalized $d$-boson occupation and ground-state energy derivatives. Finite-size results are found to approach the analytic critical point $ξ_c=8/17\simeq0.470588$, with an independent order-parameter extrapolation yielding $ξ_\infty=0.46986(61)$. The VQE reproduces ground-state energies and structural observables to numerical precision. These results demonstrate the potential of symmetry-reduced VQE for efficient quantum simulations of collective nuclear dynamics and quantum phase transitions.

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Examination of the $c\bar{c}+n+^{10}$Be bound-state problem within three cluster models based on QCD charmonium-nucleon interactions

The possible bound state of the $c\bar{c}+n+^{10}$Be system, representing a hypothetical charmonium-nucleus configuration, is investigated. The analysis is conducted within a three-cluster framework, in which the binary subsystems are treated as $n+^{10}\textrm{Be}$, $^{10}\textrm{Be}+c\bar{c}$, and $c\bar{c}+n$. The hyperspherical harmonics method is employed to provide a convenient description of this three-cluster configuration. The calculations are performed using effective $^{10}\textrm{Be}\textrm{-}c\bar{c}$ potentials constructed via the single-folding procedure. These potentials have been derived recently on the basis of state-of-the-art lattice QCD results from the HAL QCD Collaboration, which provided interactions for the spin-$3/2$ $J/ψN$, spin-$1/2$ $J/ψN$, spin-$1/2$ $η_{c}N$, and spin-averaged $J/ψN$ channels, all obtained at nearly physical pion masses. The numerical results indicate that the central binding energies of the spin-$3/2$ $J/ψ+n+^{10}$Be, spin-$1/2$ $J/ψ+n+^{10}$Be, and spin-$1/2$ $η_{c}+n+^{10}$Be systems are 3.47, 3.55, and 1.91 MeV, respectively. The corresponding root-mean-square nuclear matter radii are predicted to be approximately 2.49, 2.48, and 2.60 fm.

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Probing $NNΩ_{ccc}$ three-body systems with the modern QCD $NΩ_{ccc}$ interaction

Newly, first-principles lattice QCD results at the physical pion mass, $ m_π\backsimeq 137.1 $ MeV, have been reported by the HAL QCD Collaboration for the S-wave interaction between the nucleon ($N$) and the triply charmed Omega baryon ($Ω_{ccc}$). The $NΩ_{ccc}$ potentials in the spin-1 $ \left(^{3}S_{1}\right) $ and spin-2 $ \left(^{5}S_{2}\right) $ channels were derived and found to be attractive, though no two-body bound state was supported in these channels. The present work investigates the $NNΩ_{ccc}$ three-body system using the Malfliet-Tjon $NN$ potential. Analyses of spin-1, spin-averaged, and spin-2 $NΩ_{ccc}$ channels (at Euclidean times 16, 17, 18) reveal a three-body bound state only for the d-$Ω_{ccc}$ configuration with spin $(0)1/2^{+}$ and $t/a=16$. Its binding energy ($B_3 = -2.255$ MeV) lies slightly below the deuteron's ($B_d = -2.23$ MeV). Other parameter sets do not yield a bound state, and complex scaling analysis indicates these configurations correspond to virtual states rather than resonances. The Coulomb potential's role was also examined to differentiate charged states.

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Quantitative predictions of alpha-charmonium correlation functions in high-energy collisions

Two-body $ ^{4}\textrm{He}\left(α\right)$-charmonium $ \left(c\bar{c}\right) $ potentials in the single-folding potential (SFP) approach are built by using a first principles HAL QCD low-energy $ NJ/ψ$ and $ Nη_{c} $ interactions. The $N\textrm{-}c\bar{c}$ potentials are observed to exhibit an attractive nature across all distances, accompanied by a characteristic long-range tail. It is found that the $ α\textrm{-}J/ψ$ system appears to be loosely bound with the central binding energy in the range of 0.1-0.6 MeV, while for spin-$ 1/2 $ $α\textrm{-}η_{c}$, no bound or resonance state (with respect to the $ α\textrm{-} c\bar{c} $ threshold) was found. The $ α\textrm{-}c\bar{c} $ correlation function in high-energy collisions is examined to explore the $ N\textrm{-}c\bar{c} $ interaction. The analysis revealed that variations in spin-dependent $α\textrm{-}c\bar{c}$ interactions-spin-$3/2$ $α\textrm{-}J/ψ$, spin-$1/2$ $α\textrm{-}J/ψ$, spin-$1/2$ $α\textrm{-}η_c$, and the spin-averaged $α\textrm{-}J/ψ$-produce noticeable differences in the $α\textrm{-}c\bar{c}$ correlation function, especially when the source size is around $ 3 $ fm. It is found that different results are produced by the Lednicky-Lyuboshits formula at small source sizes. This indicates that a relatively long-range interaction exists for the $ α\textrm{-}c\bar{c} $ system. Furthermore, a comparison has been conducted between two density functions of $ ^{4}\textrm{He}$ the central depression (CD) and the simple single Gaussian (SG) density-both of which share an identical rms radius of 1.56 fm. Although the $α\textrm{-}J/ψ$ binding energies for the two models are nearly indistinguishable, their corresponding correlation functions demonstrate markedly different behaviors.

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Probing $ ϕ$N interaction through bound states of $ ϕ\textrm{N-}α$ system

The possible bound state of the $ ϕN α$ system is explored within the framework of the three-body cluster model. The calculations are done by employing the state-of-the-art $ ϕ$N interactions obtained from the analysis of the pure elastic scattering and the coupled-channel in the $ϕp$ correlation functions. The $ ϕα$ potentials are constructed by two methods: the single-folding potential (SFP) method for the given spin-averaged $ ϕ$N potentials in coordinate space, and the optical model potential (OMP) approximation within the multiple-scattering framework for the given scattering length of the $ ϕ$N interaction. It is found that, when only the single-channel $ ϕN$ interactions are employed, the $ ϕN α$ system could be bound with a binding energy in the interval [3-26] MeV. However, the coupled-channel $ϕp$ interaction, which is most consistent with experimental measurements, does not yield any bound state, even when the spin-averaged $ϕN$ potential is employed, and this potential is found to be more attractive than the corresponding coupled-channel counterpart. It is essential to consider the contributions from the dynamics of the vector-baryon coupled channels $ϕp$ interaction. This effect is capable of playing a decisive role in the existence of mesic nuclei.

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Bound states of $_{c\bar{c}}^{9}$Be within $c\bar{c}+α+α$ cluster models based on state-of-the-art HAL QCD charmonium-nucleon interactions

The possible bound state of the $ _{c\bar{c}}^{9}$Be, a charmonium-nucleus system, is investigated. The analysis is carried out within a three-cluster model, where its binary subsystems are represented as $ c\bar{c}\textrm{+}α$ and $α+α$. The hyperspherical harmonics method is employed to facilitate a convenient description of this three-cluster configuration. The calculations are done by employing the effective $ c\bar{c}\textrm{-}α$ potentials. These potentials were derived recently based on state-of-the-art lattice QCD calculations, which provided interactions for the spin 3/2 $J/ψN $, spin 1/2 $J/ψN $, spin 1/2 $η_{c}N$ and spin-averaged $J/ψN$ interactions, all obtained with nearly physical pion masses. The Coulomb interaction was also incorporated into the current calculations. It is determined that, despite neither the $ _{c\bar{c}}^{5}$He nor the $^{8}$Be binary subsystems being bound, a bound state of the $ c\bar{c}\textrm{-} αα$ nuclear system could potentially exist. The maximum central binding energy is found to be approximately 1.71 MeV, based on the spin 1/2 $J/ψN $ interaction, while a minimum value of about 0.56 MeV is obtained from calculations involving the spin 1/2 $η_{c}N$ interaction.

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The role of the screening potential in the deuteron-deuteron thermonuclear reaction rates

The deuteron-deuteron (D-D) thermonuclear reaction rates in metallic environments (considering the electron screening effects) is calculated using the S-factor functions which were obtained by fitting to low-energy data on D-D reactions. For this purpose, a fitted S-factor model based on the NACRE compilation is employed. This limited the energy range of Big Bang nucleosynthesis (BBN) for the $ ^{2}\textrm{H}\left(d,p\right) ^{3}\textrm{H}$ and $^{2} \textrm{H} \left(d,n\right) ^{3}\textrm{He}$ reactions. The corresponding Maxwellian-averaged thermonuclear reaction rates of relevance in astrophysical plasmas at temperatures in the range from $10^{6}$ K to $10^{10}\left(\textrm{or }1.3\times10^{8}\right)$ K are provided in tabular formats. In these evaluations, the screening energy ($ U_{e} $) is assumed to be $100, 400, 750, 1000$ eV and $1250$ eV. This series of values has been selected based on theoretical and experimental studies conducted so far. % Eventually, our numerical analysis suggests that the ratio of the reaction rate with the screening potential to the reaction rate without the screening potential, can be described by the term $ \exp\left(4.70 +6.50\:{U_{e}}/{T_{9}}\right) $ for both $ ^{2}\textrm{H}\left(d,p\right) ^{3}\textrm{H}$ and $^{2} \textrm{H} \left(d,n\right) ^{3}\textrm{He}$ reactions. This series of values has been selected based on theoretical and experimental studies conducted so far.

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Exploring $ Λ{\text-} $ and $ Ξ{\text -}$triton correlation functions in heavy-ion collisions

The $ Λ{\text -} $ and $ Ξ{\text -}$triton(t) momentum correlation functions, to be measured in high-energy heavy-ion collisions, are explored. Mainly, STAR detector acquired data provides an opportunity to explore the $ Λt $ correlation function. The $ Λt $ correlation functions are calculated using an isle-type and spin-averaged $ Λt $ potential, also, its sensitivity to changes in potential strength has also been investigated. % Besides, even though there is no experimental data on the $ Ξ{\text -} $triton interaction yet, I constructed $Ξt$ potentials based on the first principles HAL QCD and Nijmegen extended soft-core (ESC08c) model of spin- and isospin averaged $ΞN$ interactions in single-folding potentials (SFP) approach. Then, the $Ξt$ correlation functions are calculated for these two modern potentials as well as for Nijmegen hard-core model D (NHC-D) $ΞN$ potential. The numerical results predict that, with good measurement resolution, it might be possible to recognize different potentials with a correlation function at relatively small source sizes, i.e., $ R = 1-3 $ fm.

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Femtoscopic study of the $ Ωα$ interaction in heavy-ion collisions

The two-particle momentum correlation between the Omega-baryon ($Ω$) and the $^{4}He (α) $ in high-energy heavy ion collisions is explored. Such correlations as an alternative source of information can help us further understand the interaction between $ Ω$ and nucleons (N). $ Ωα$ potentials in the single-folding potential approach are constructed by employing two different available $ΩN $ interactions in $^{5}S_{2}$ channel, i.e, one is based on the (2 + 1)-flavor lattice QCD simulations near the physical point by the HAL QCD collaboration, and another is based on the meson exchanges with effective Lagrangian, where in the latter case coupled channels effect is considered. It is found that the correlation functions at small size source depends on the used potential model. This implicitly means that at high density nuclear medium, $ Ωα$ momentum correlation could drive the feature of $ ΩN $ interactions. Moreover, by extracting the scattering length and the effective range from obtained $ Ωα$ potentials, the correlation functions are calculated within the Lednicky-Lyuboshits (LL) formalism. It is shown that since the $Ωα$ has large interaction range, the LL formula leads to different results at small source size.

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Exploring the $ ϕ{\text -}α$ interaction via femtoscopic study

Very recently the Wood-Saxon (WS) type interaction in the single-folding potential approach are constructed to simulate the $ ϕ{\text -}α$ potentials. One set of the $ ϕ{\text -}α$ potentials are based on the first principle HAL QCD $ϕ{\text -}N $ interactions in $^{4}S_{3/2}$ channel, and in another set, the $ϕ$-meson-nucleus potentials were calculated by employing the quark-meson coupling (QMC) model. By utilizing these two set of $ ϕ{\text -}α$ potentials, the two-particle momentum correlation of $ ϕ{\text -}α$ in high-energy heavy ion collisions is explored. The numerical results show that the correlation functions at small source size (high density nuclear medium) depends on the employed potential model. Also, the correlation functions are obtained within the Lednicky-Lyuboshits (LL) formalism. For small source size, it is found that, the LL formula returns significantly different values due to the large interaction range of the $ϕ{\text -}α$ potential.

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$_Ξ^{5}H $ hypernuclei by folding the state-of-the-art $ ΞN $ interactions

I examined a phenomenological Nijmegen and a first principles HAL QCD $ΞN$ potentials to study $αΞ$ ineractions. A Woods-Saxon type form for $αΞ$ potential in the single-folding potential approach is derived by using the spin- and isospin averaged $ΞN$ interactions. The possibility of resonance or bound state is searched and accordingly, the low energy scattering phase shift parameters of $αΞ$ are calculated. The numerical results show that even though two $ ΞN $ potentials have significantly dissimilar isospin (I) and spin (S) components, $_Ξ^{5}H $ could be only a Coulomb-assisted resonance state that appears about $ 0.5 $ MeV below the threshold of $α+Ξ^{-} $ for both model of potentials.

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Examination of the $ ϕ-NN $ bound-state problem with lattice QCD $ N-ϕ$ potentials

The developed Faddeev three-body equations are solved to search for bound-state solutions of a phi-meson $ \left(ϕ\right) $ and two nucleons $ \left( \textrm{NN} \right) $ system. The newly published spin $ 3/2 $ $ \textrm{N-\ensuremathϕ} $ potential based on the $ \left(\textrm{2+1}\right) $-flavor lattice QCD simulations near physical point, and realistic $ \textrm{NN} $ Malfliet-Tjon (MT) potential, are employed. Our numerical calculations for $ (I)J^π=(0)2^{-}$ $ ϕ\textrm{-d} $ system in maximum spin leads to ground state binding energy of about $ 7 $ MeV and a matter radius of about $ 8 $ fm. Our results indicates the possibility of the formation of new nuclear clusters.

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Coupled-channel $Λ_{c}K^{+}-pD_{s}$ Interaction in Flavor $ \textrm{SU}\left(3\right) $ Limit of Lattice QCD

We study $S$-wave interactions in the $I\left(J^{p}\right)=1/2\left(1/2^{-}\right)$ $Λ_{c}K^{+}-pD_{s}$ system on the basis of the coupled-channel HAL QCD method. The potentials which are faithful to QCD S-matrix below the $ pD^{*} $ threshold are extracted from Nambu-Bethe-Salpeter wave functions on the lattice in Flavor $ \textrm{SU}\left(3\right) $ Limit. For the simulation, we employ $ 3 $-flavor full QCD gauge configurations on a $\left(1.93 \:\textrm{fm} \right)^{3}$ volume at $m_π\simeq 872$ MeV. %\textcolor{red}{For the charm quark, the relativistic heavy quark action is employed to treat its dynamics on the lattice}. We present our results of the S-wave coupled-channel potentials for the $Λ_{c}K^{+}-pD_{s}$ system in the $1/2\left(1/2^{-}\right)$ state as well as scattering observables obtained from the extracted potential matrix. We observe that the coupling between $Λ_{c}K^{+}$ and $pD_{s}$ channels is weak. The phase shifts and scattering length obtained from the extracted potential matrix show that the $Λ_{c}K^{+}$ interaction is attractive at low energy and stronger than the $pD_{s}$ interaction though no bound state at $m_π\geq872$ MeV.

hep-lat

$Ω$-deuteron Interaction in Folding Model

A simple single folding model for $Ω$-deuteron with maximal spin $\left(I\right)J^{P}=\left(0\right)5/2^{+}$ is investigated. $Ω$ is assumed to orbit an unperturbed deuteron in a $Ω$-deuteron potential based on a separable $Ω$-nucleon potential from lattice QCD. We show that the effective central folding potential of $Ωd$ in the $^{5}S_{2}$ channel has a simple Wood-Saxon form, and approximate the upper bound for the binding energy of $Ω$ particle on a deuteron. In order to investigate how changes in the wave functions affect the results, we consider four analytical forms for $S$-state deuteron wave functions, i.e., two widely used Hulthén forms, as well as the modified Reid93 and Argonne v18 forms. Our calculations of binding energy from simple two-body approximation are compared with the results reported for the three-body problem; it is confirmed that the $Ωd$ system is deeply bound. Although the single folding model reduces the three-body problem to a two-body problem, this simplification is inadequate.

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A simple model of the charmed hypertriton

We investigate the three-baryon system with charm +1 in a simple model. Charmed lambda $Λ_{c}$ is assumed to orbit an unperturbed deuteron in a charmed lambda-deuteron potential based on a separable charmed lambda-nucleon potential from chiral effective field theory techniques extrapolations of lattice QCD data for the $Λ_{c}N$ $^{1}S_{0}$ and $^{3}S_{1}$ partial waves. We have estimated the strength and the range of the $Λ_{c}$d potential. Also, the $Λ_{c}$ particle momentum distribution in $_{Λ_{c}}^{3}H$ is presented and compared by $Λ$ particle in $_Λ^{3}H$. It is found that there is no bound $_{Λ_{c}}^{3}H$ state by solving eigenvalue condition equation.

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Simple Woods-Saxon type form for $Ωα$ and $Ξα$ interactions using Folding Model

We derive a simple Woods-Saxon type form for the potentials between $Y=Ξ, Ω$ and $α$ by using a single-folding potential method, based on a separable $Y$-nucleon potential. Accordingly, the potentials $Ξ+α$ and $Ω+α$ are obtained using the ESC08c Nijmegens $ΞN$ potential (in $^{3}S_{1}$ channel) and HAL QCD Collaboration $ΩN$ interactions (in lattice QCD), respectively. In deriving the potential between $Y$ and $α$, the same potential between $Y$ and $N$ is used. Binding energy, scattering length and effective range of $Y$ particle on the alpha particle are approximated by the resultant potentials. The depths of the potentials in $Ωα$ and $Ξα$ systems are obtained $-61$ and $-24.4$ MeV, respectively. In the case of $Ξα$ potential, a fairly good agreement is observed between the single-folding potential method and the phenomenological potential of Dover-Gal model. These potentials can be used in 3-,4- and 5-body cluster structures of $ Ω$ and $Ξ$ hypernuclei.

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$NΩ$ dibaryon from lattice QCD near the physical point

The nucleon($N$)-Omega($Ω$) system in the S-wave and spin-2 channel ($^5$S$_2$) is studied from the (2+1)-flavor lattice QCD with nearly physical quark masses ($m_π\simeq 146$~MeV and $m_K \simeq 525$~MeV). The time-dependent HAL QCD method is employed to convert the lattice QCD data of the two-baryon correlation function to the baryon-baryon potential and eventually to the scattering observables. The $NΩ$($^5$S$_2$) potential, obtained under the assumption that its couplings to the D-wave octet-baryon pairs are small, is found to be attractive in all distances and to produce a quasi-bound state near unitarity: In this channel, the scattering length, the effective range and the binding energy from QCD alone read $a_0= 5.30(0.44)(^{+0.16}_{-0.01})$~fm, $r_{\rm eff} = 1.26(0.01)(^{+0.02}_{-0.01})$~fm, $B = 1.54(0.30)(^{+0.04}_{-0.10})$~MeV, respectively. Including the extra Coulomb attraction, the binding energy of $pΩ^-$($^5$S$_2$) becomes $B_{pΩ^-} = 2.46(0.34)(^{+0.04}_{-0.11})$~MeV. Such a spin-2 $pΩ^-$ state could be searched through two-particle correlations in $p$-$p$, $p$-nucleus and nucleus-nucleus collisions.

hep-lat

Constrained Path Monte Carlo method for spin $ 1/2 $ fermions at unitarity limit

We present calculations for spin $ 1/2 $ fermions at unitarity limit, where the effective range of the interaction is zero and the scattering length is infinite. We compute the ground-state energy for a system of 6, 10,14,18 and 20 particles, with equal numbers of up and down spins in a periodic cube in the full ground-state constrained-path Monte Carlo (CPMC) method using the extended, attractive Hubbard model. Our results in a careful extrapolation to the thermodynamic limit may suggest that the ratio of the ground-state energy to that of a free Fermi gas is $ ξ= 0.43(4) $, which can compare with recent experimental results and consistent with the fixed node Green's function Monte Carlo and novel lattice approaches results. We also obtain results for interactions with different effective ranges and find that the energy is consistent with a universal linear dependence on the product of the Fermi momentum and the effective range.

cond-mat.str-el