Search arXivSearch

arXiv · 1911.06089

$Ξ_c$ and $Ξ_b$ excited states within a ${\rm SU(6)}_{\rm lsf}\times$HQSS model

Abstract

We study odd parity $J=1/2$ and $J=3/2$ $Ξ_c$ resonances using a unitarized coupled-channel framework based on a ${\rm SU(6)}_{\rm lsf}\times$HQSS-extended Weinberg-Tomozawa baryon-meson interaction, while paying a special attention to the renormalization procedure. We predict a large molecular $Λ_c \bar K$ component for the $Ξ_c(2790)$ with a dominant $0^-$ light-degree-of-freedom spin configuration. We discuss the differences between the $3/2^-$ $Λ_c(2625)$ and $Ξ_c(2815)$ states, and conclude that they cannot be SU(3) siblings, whereas we predict the existence of other $Ξ_c-$states, two of them related to the two-pole structure of the $Λ_c(2595)$. It is of particular interest a pair of $J=1/2$ and $J=3/2$ poles, which form a HQSS doublet and that we tentatively assign to the $Ξ_c(2930)$ and $Ξ_c(2970)$, respectively. Within this picture, the $Ξ_c(2930)$ would be part of a SU(3) sextet, containing either the $Ω_c(3090)$ or the $Ω_c(3119)$, and that would be completed by the $Σ_c(2800)$. Moreover, we identify a $J=1/2$ sextet with the $Ξ_b(6227)$ state and the recently discovered $Σ_b(6097)$. Assuming the equal spacing rule and to complete this multiplet, we predict the existence of a $J=1/2$ $Ω_b$ odd parity state, with a mass of 6360 MeV and that should be seen in the $Ξ_b \bar K$ channel.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

J. Nieves, R. Pavao, L. Tolos. 2019-11-14. $Ξ_c$ and $Ξ_b$ excited states within a ${\rm SU(6)}_{\rm lsf}\times$HQSS model. https://doi.org/10.1140/epjc%2Fs10052-019-7568-8

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Exploring the Singlino-dominated Thermal Neutralino Dark Matter in the $Z_3$ invariant NMSSM

We examine the parameter space of the Next to Minimal Supersymmetric Standard Model (NMSSM) with Singlino-dominated neutralino $\widetildeχ_1^0$ as the lightest supersymmetric particle (LSP). Our study focuses on identifying the regions within this parameter space that produce a thermal relic abundance of $\widetildeχ_1^0$ smaller than the observed cold dark matter relic density while remaining consistent with constraints from LEP measurements, low-energy experiments, Higgs measurements, LHC data, and dark matter direct detection experiments. We identify the dominant annihilation modes of the LSP neutralino across varying LSP mass ranges $\sim \mathcal{O}(1)-\mathcal{O}(10^{3})~$GeV. Furthermore, we conduct a benchmark study to assess the production rates of triple-boson final states emerging from direct electroweakino pair production at the LHC. Drawing insights from these findings, we perform a detailed collider analysis to explore the future potential of probing the triple-boson final states involving a light Higgs boson at the high-luminosity LHC (HL-LHC).

hep-ph

Unveiling the Collins-Soper kernel in inclusive DIS at threshold

We revisit the factorization of inclusive deep inelastic scattering (DIS) near the kinematic threshold in terms of collinear, off-light-cone operators. At threshold, particle production develops around two opposite near-light-cone directions in close analogy with transverse-momentum-dependent semi-inclusive DIS. The Collins-Soper kernel then emerges as the universal function governing the rapidity evolution of the relevant parton correlators in both cases. Our new framework also clarifies outstanding issues related to soft radiation and rapidity divergences at threshold.

hep-ph

Novel Light Dark Matter Detection with Quantum Parity Detector Using Qubit Arrays

We present the design and the sensitivity reach of the Qubit-based Light Dark Matter detection experiment. We propose the novel two-chip design to reduce signal dissipation, with quantum parity measurement to enhance single-phonon detection sensitivity. We demonstrate the performance of the detector with full phonon and quasiparticle simulations. The experiment is projected to detect $\gtrsim 30$ meV energy deposition with nearly $100\%$ efficiency and high energy resolution. The sensitivity to $m_χ\gtrsim 0.01$ MeV dark matter scattering cross section is expected to be advanced by orders of magnitude for both light and heavy mediators, and similar improvements will be achieved for axion and dark photon absorption in the $0.04$-$0.2$ eV mass range.

hep-ph