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A. Pérez-Obiol

Publications and source records attributed to A. Pérez-Obiol.

7 recordsLinked to original sources

Hypertriton lifetime

Over the last decade, conflicting values of the hypertriton ${}_Λ^3\mathrm{H}$ lifetime $τ({}_Λ^3\mathrm{H})$ were extracted from relativistic heavy-ion (RHI) collision experiments, ranging from values compatible with the free-$Λ$ lifetime $τ_Λ$-as expected naively for a very weakly bound $Λ$ in ${}_Λ^3\mathrm{H}$-to lifetimes as short as $τ({}_Λ^3\mathrm{H}) \approx (0.4-0.7)\,τ_Λ$. In a recent work [Phys. Lett. B 811, 135916 (2020)] we studied this ${}_Λ^3\mathrm{H}$ lifetime puzzle theoretically using realistic three-body ${}_Λ^3\mathrm{H}$ 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, $τ({}_Λ^3\mathrm{H})$ was found to be strongly correlated with the $Λ$ separation energy $B_Λ$ in ${}_Λ^3\mathrm{H}$, 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 $τ({}_Λ^3\mathrm{H})$, and thus limit considerably the theoretical precision of its computed value. Although none of the conflicting RHI measured $τ({}_Λ^3\mathrm{H})$ values can be excluded, but rather can be attributed to a poor knowledge of $B_Λ$, we note the good agreement between the lifetime value $τ({}_Λ^3\mathrm{H})=238(27)$ ps computed at the lowest value $B_Λ=66$ keV reached by us and the very recent ALICE measured lifetime value $τ^{\mathrm{ALICE}}({}_Λ^3\mathrm{H})=253(11)(6)$ ps associated with the ALICE measured $B_Λ$ value $B^{\mathrm{ALICE}}_Λ=102(63)(67)$ keV [Phys. Rev. Lett. 131, 102302 (2023)].

nucl-th↗

Quantum entanglement patterns in the structure of atomic nuclei within the nuclear shell model

Quantum entanglement offers a unique perspective into the underlying structure of strongly-correlated systems such as atomic nuclei. In this paper, we use quantum information tools to analyze the structure of light and medium-mass berillyum, oxygen, neon and calcium isotopes within the nuclear shell model. We use different entanglement metrics, including single-orbital entanglement, mutual information, and von Neumann entropies for different equipartitions of the shell-model valence space and identify mode-entanglement patterns related to the energy, angular momentum and isospin of the nuclear single-particle orbitals. We observe that the single-orbital entanglement is directly related to the number of valence nucleons and the energy structure of the shell, while the mutual information highlights signatures of proton-proton and neutron-neutron pairing, as well as nuclear deformation. Proton and neutron orbitals are weakly entangled by all measures, and in fact have the lowest von Neumann entropies among all possible equipartitions of the valence space. In contrast, orbitals with opposite angular momentum projection have relatively large entropies, especially in spherical nuclei. This analysis provides a guide for designing more efficient quantum algorithms for the noisy intermediate-scale quantum era.

nucl-th↗

Nuclear shell-model simulation in digital quantum computers

The nuclear shell model is one of the prime many-body methods to study the structure of atomic nuclei, but it is hampered by an exponential scaling on the basis size as the number of particles increases. We present a shell-model quantum circuit design strategy to find nuclear ground states by exploiting an adaptive variational quantum eigensolver algorithm. Our circuit implementation is in excellent agreement with classical shell-model simulations for a dozen of light and medium-mass nuclei, including neon and calcium isotopes. We quantify the circuit depth, width and number of gates to encode realistic shell-model wavefunctions. Our strategy also addresses explicitly energy measurements and the required number of circuits to perform them. Our simulated circuits approach the benchmark results exponentially with a polynomial scaling in quantum resources for each nucleus. This work paves the way for quantum computing shell-model studies across the nuclear chart and our quantum resource quantification may be used in configuration-interaction calculations of other fermionic systems.

quant-ph↗

Lifetime of the hypertriton

Conflicting values of the hypertriton lifetime $τ({}_Λ^3\mathrm{H})$ 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 $τ({}_Λ^3\mathrm{H})$ comes sufficiently close to the free-$Λ$ lifetime $τ_Λ$,as expected naively for a very weakly bound $Λ$ in ${}_Λ^3\mathrm{H}$. We revisited theoretically this ${}_Λ^3\mathrm{H}$ lifetime puzzle, using ${}_Λ^3\mathrm{H}$ 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 $Γ({}_Λ^3\mathrm{H}\to{}^3\mathrm{He}+π^-)$. We found significant but opposing contributions arising from $ΣNN$ admixtures in ${}_Λ^3\mathrm{H}$ and from $π^- -{}^3\mathrm{He}$ final-state interaction. To derive $τ({}_Λ^3\mathrm{H})$, we evaluated the inclusive $π^-$ decay rate $Γ_{π^-}({}_Λ^3\mathrm{H})$ by using the measured branching ratio $Γ({}_Λ^3\mathrm{H}\to{}^3\mathrm{He}+π^-)/Γ_{π^-}({}_Λ^3\mathrm{H})$ and added the $π^0$ contributions through the $ΔI = \frac{1}{2}$ rule. The resulting $τ({}_Λ^3\mathrm{H})$ varies strongly with the rather poorly known $Λ$ separation energy $E_{\mathrm{sep}}({}_Λ^3\mathrm{H})$ and it is thus possible to associate each one of the distinct RHI $τ({}_Λ^3\mathrm{H})$ measurements with its own underlying value of $E_{\mathrm{sep}}({}_Λ^3\mathrm{H})$.

nucl-th↗

Roadmap on Atomtronics: State of the art and perspective

Atomtronics deals with matter-wave circuits of ultra-cold atoms manipulated through magnetic or laser-generated guides with different shapes and intensities. In this way, new types of quantum networks can be constructed, in which coherent fluids are controlled with the know-how developed in the atomic and molecular physics community. In particular, quantum devices with enhanced precision, control and flexibility of their operating conditions can be accessed. Concomitantly, new quantum simulators and emulators harnessing on the coherent current flows can also be developed. Here, we survey the landscape of atomtronics-enabled quantum technology and draw a roadmap for the field in the near future. We review some of the latest progresses achieved in matter-wave circuits design and atom-chips. Atomtronic networks are deployed as promising platforms for probing many-body physics with a new angle and a new twist. The latter can be done both at the level of equilibrium and non-equilibrium situations. Numerous relevant problems in mesoscopic physics, like persistent currents and quantum transport in circuits of fermionic or bosonic atoms, are studied through a new lens. We summarize some of the atomtronics quantum devices and sensors. Finally, we discuss alkali-earth and Rydberg atoms as potential platforms for the realization of atomtronic circuits with special features.

cond-mat.quant-gas↗

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.

nucl-th↗

On the bound states of magnetic Laplacians on wedges

This paper is mainly inspired by the conjecture about the existence of bound states for magnetic Neumann Laplacians on planar wedges of any aperture $ϕ\in (0,π)$. So far, a proof was only obtained for apertures $ϕ\lesssim 0.511π$. The conviction in the validity of this conjecture for apertures $ϕ\gtrsim 0.511π$ mainly relied on numerical computations. In this paper we succeed to prove the existence of bound states for any aperture $ϕ\lesssim 0.583π$ using a variational argument with suitably chosen test functions. Employing some more involved test functions and combining a variational argument with computer-assistance, we extend this interval up to any aperture $ϕ\lesssim 0.595π$. Moreover, we analyse the same question for closely related problems concerning magnetic Robin Laplacians on wedges and for magnetic Schrödinger operators in the plane with $δ$-interactions supported on broken lines.

math-ph↗