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Ailin Zhang

Publications and source records attributed to Ailin Zhang.

At least 19 recordsLinked to original sources

Foreseeing the Invisible: Amodal Reconstruction of Leaf Fossil Images

Fossil leaves are rarely preserved whole -- sedimentary rock hides, breaks, and erodes the lamina, yet paleobotany depends on the complete shape and outline of the leaf. We cast the recovery of the missing tissue as amodal reconstruction and present AmodalDINO, a multi-head dense-prediction model that predicts four masks from a single RGB image: visible leaf, amodal complete leaf, amodal main vein, and fine veins. Unlike essentially all prior amodal work, AmodalDINO is given no visible mask. It predicts the visible and amodal regions jointly, so it needs no upstream instance segmenter at runtime. Two simple but effective changes adapt the model to the amodal segmentation task: fully fine-tune a DINOv3 ViT-L/16 at a small learning rate instead of freezing it, and attach auxiliary venation heads alongside the leaf heads. These two changes enable the model to learn the structural shape prior of leaves. Trained only on synthetic leaf fossil images, AmodalDINO reaches 95.0% Dice / 90.5% IoU on the validation set and transfers well to real fossil specimens. Stripped to two heads, the same recipe can run on two benchmark datasets, reaching 85.05 full mIoU / 66.65 occluded mIoU on KINS and 80.90 / 38.15 on COCOA-cls. The model is also practical: by quantizing to 4-bit weights, it runs entirely offline in a browser, matching the original model with an IoU of 0.910. We also add ruler-based calibration to estimate surface area, and a generative visualization of living leaves on local devices.

cs.CV

$P_{c\bar cs}(4459)^{0}$, $P_{c\bar c s}(4338)^0$ and mass spectrum of strange hidden-charm pentaquarks

Strange hidden-charm pentaquark states have been systematically investigated within a diquark-triquark model. Through a Gaussian expansion method, masses of some diquarks, triquarks and strange hidden-charmed pentaquark states from S-wave to P-wave excitations have been calculated with the non-relativistic Semay and Silvestre-Brac potentials in terms of the same parameters employed for tetraquark states. Masses of pentaquark states in S-wave excitations are found between $4200$ MeV and $4590$ MeV, while masses of all P-wave excitations are found above $4600$ MeV. Mass splittings between the S-wave and P-wave pentaquark states are about $350-570$ MeV. In comparison to the experimental data, $P_{c\bar cs}(4459)^{0}$ observed by LHCb in decay channel $Ξ_{b}^{-}\rightarrow J/ψΛK^-$ is assumed as the $|1; 0, 1/2; 3/2, 0\rangle_{3/2}$ $[sq][\bar{c}cq]$ pentaquark state with $J^P={3\over 2}^-$, while $P_{c\bar c s}(4338)^0$ observed in the decay channel $B^{-}\rightarrow J/ψΛ\bar{p}$ is very possibly the $|0; 1, 1/2; 1/2, 0\rangle_{1/2}$ $[cq][\bar{c}sq]$ pentaquark state with $J^P={1\over 2}^-$. We predict a lowest strange hidden-charm pentaquark state with $J^P={1\over 2}^-$ around $4200$ MeV.

hep-ph

Spectrum of $[cq][\bar{s}\bar{q}]$ tetraquarks: Nature of $D^*_{s0}(2317)$, $D_{s1}(2460)$ and $T^*_{c\bar s0}(2900)$

Motivated by the recent observations of exotic open-charm tetraquark candidates \(T^a_{c\bar{s}0}(2900)^{++}\) and \(T^a_{c\bar{s}0}(2900)^{0}\), we systematically calculate the mass spectra of \([cq][\bar{s}\bar{q}]\) tetraquarks within a nonrelativistic constituent quark potential model. In the model, the tetraquark states are treated as diquark-antidiquark bound systems with an interior interaction similar to the quark-antiquark interaction in conventional mesons. The well established states \(D_{s0}^*(2317)\) with \(J^P=0^+\) and \(D_{s1}(2460)\) with \(J^P=1^+\) could be identified as the two ground states of the \([cq][\bar{s}\bar{q}]\) system. \(T^a_{c\bar{s}0}(2900)^{0}\) and \(T^a_{c\bar{s}0}(2900)^{++}\) could be naturally interpreted as radially excited \(0^+\) tetraquark states with different interior components. Their large mass difference may result from their different interior structure instead of an isospin symmetry breaking. Whether \(T^a_{c\bar{s}0}(2900)^{0}\) and \(T^a_{c\bar{s}0}(2900)^{++}\) belong to an isospin triplet deserves further experimental investigation. In addition, there may be another \(0^+\) \([cq][\bar{s}\bar{q}]\) tetraquark state with mass around $2450$ MeV, which is composed of a $cq$ diquark and a $\bar s\bar q$ antidiquark both with spin-0. In the energy region $2640-2700$ MeV, there may be a $J^P=2^+$ \([cq][\bar{s}\bar{q}]\) tetraquark state composed of the $cq$ diquark and the $\bar s\bar q$ antidiquark both with spin-1.

hep-ph

Impact of Resistance Development Mechanisms on Antibiotic Treatment Outcomes

Bacteria develop resistance to antibiotics through various mechanisms, with the specific mechanism depending on the drug-bacteria pair. It remains unclear, however, which resistance mechanism best supports favorable treatment outcomes, specifically in clearing infections and inhibiting further resistance. In this study, we use periodic ordinary differential equation models to simulate different antibiotic treatment protocols for bacterial infections. Using stability analysis and numerical simulations, we investigate how different resistance mechanisms, including plasmid-induced and mutation-induced resistance, affect treatment outcomes. Our findings suggest that antibiotic treatments with fixed dosing schedules are more likely to be effective when resistance arises exclusively through plasmid-mediated transmission. Further, when treatment fails, mutation-driven mechanisms tend to favor the selection of fully resistant bacterial strains. We also investigated the efficacy of different treatment strategies based on these mechanisms, finding that a twice-daily regimen consistently outperforms a once-daily regimen in terms of infection clearance. Additionally, our simulations with short half-life antibiotics indicate that the "catch-up" strategy outperforms the "compensatory double-dose" approach after a missed dose, a finding that aligns with general pharmaceutical advice for short-half-life drugs.

q-bio.PE

Conceptual Design Report of Super Tau-Charm Facility: The Accelerator

Electron-positron colliders operating in the GeV region of center-of-mass energies or the Tau-Charm energy region, have been proven to enable competitive frontier research, due to its several unique features. With the progress of high energy physics in the last two decades, a new-generation Tau-Charm factory, Super Tau Charm Facility (STCF) has been actively promoting by the particle physics community in China. STCF holds great potential to address fundamental questions such as the essence of color confinement and the matter-antimatter asymmetry in the universe in the next decades. The main design goals of STCF are with a center-of-mass energy ranging from 2 to 7 GeV and a peak luminosity surpassing 5*10^34 cm^-2s^-1 that is optimized at a center-of-mass energy of 4 GeV, which is about 50 times that of the currently operating Tau-Charm factory - BEPCII. The STCF accelerator is composed of two main parts: a double-ring collider with the crab-waist collision scheme and an injector that provides top-up injections for both electron and positron beams. As a typical third-generation electron-positron circular collider, the STCF accelerator faces many challenges in both accelerator physics and technology. In this paper, the conceptual design of the STCF accelerator complex is presented, including the ongoing efforts and plans for technological R&D, as well as the required infrastructure. The STCF project aims to secure support from the Chinese central government for its construction during the 15th Five-Year Plan (2026-2030) in China.

physics.acc-ph

Mass spectra of doubly charmed tetraquarks $T_{cc}$

Motivated by the first observation of a doubly charmed tetraquark candidate $T_{cc}(3875)^+$, we perform a systematic calculation of the mass spectra of doubly charmed tetraquark states from $1S$ to $2P$ excitations in a nonrelativistic constituent quark potential model. In terms of the quark-quark potential, the mass of the charmed spin-$1$ diquark is predicted $\sim 3500$ MeV. The masses of the light ``good'' and ``bad'' antidiquark are calculated with $\sim 670$ MeV and $\sim 840$ MeV, respectively. The mass difference between light ``good'' and ``bad'' diquarks is $\sim 170$ MeV, which is consistent with previous phenomenological analyses. The interaction between the charmed diquark and the light antidiquark is then modulated by the quark-antiquark potential in the model, and the mass spectra of doubly charmed tetraquarks from $1S$ to $2P$ excitations are calculated with the calculated masses of diquarks/antidiquarks and refitted parameters from $T_{cc}(3875)^+$ and $X(3872)$. The $1S-1P$ and $1S-2S$ mass splittings of doubly charmed tetraquarks are about $410-430$ MeV and $610-650$ MeV, respectively, and this mass splittings pattern is similar to that for ordinary $D$ mesons. The mass splittings of doubly charmed tetraquarks with isospin-$0$ is about $10-25$ MeV higher than the corresponding mass splittings of doubly charmed tetraquarks with isospin-$1$ from $1S$ to $2P$ excitations. $T_{cc}(3875)^+$ is possible to be assumed as a $IJ^P=01^+$ ground doubly charmed tetraquark candidate with a light ``good'' antidiquark, and the next $P$-wave excited doubly charmed tetraquarks are predicted to have masses with an average $420-430$ MeV higher. A $J^P=0^+$ ground doubly charmed tetraquark $T_{cc}(3834)$ with isospin-$1$ located around $3834$ MeV is expected.

hep-ph

$X(3872)$ and hidden charmed tetraquarks

In a constituent quark model, a hidden charmed tetraquark is assumed consisting of a $cq$ diquark and an $\bar c\bar q$ antidiquark or vice versa. The Semay-Silvestre-Brac potentials are employed to calculate the masses of $cq$ (q=u, d) diquarks. The mass of the $cq$ diquark or $\bar c\bar q$ antidiquark with spin-$0$ is predicted with $\sim 2175$ MeV, and the spin-$1$ one is predicted with $\sim 2220$ MeV. The masses of hidden charmed tetraquarks from $1S$ to $2P$ excitations are systemically calculated in terms of the same potentials. It is found that the mass of hidden charmed tetraquark without radial excitation grows higher in $1^{+-},~1^{++},~1^{--},~0^{-+},~0^{--},~1^{-+},~\cdots$ sequence, and the tetraquarks with exotic $J^{PC}=0^{--},~1^{-+}$ have higher masses. The hidden charmed tetraquarks with radial excitations have masses larger than $4300$ MeV. The $1S-1P$ and $1S-2S$ mass splittings of the hidden charmed tetraquarks are about $390-400$ MeV and $550-570$ MeV, respectively, which are about $70$ MeV and $50$ MeV smaller than those of normal charmonium. The $1P-2P$ and $2S-2P$ mass splittings are similar to those for conventional $c\bar c$ charmonium mesons. Based on our predicted masses for hidden charmed tetraquarks, some XYZ exotics are analyzed and tentatively assigned. $X^*(3860)$ is possibly the $0^{++}$ tetraquark. $Z_c(3900)$ and $X(3940)$ are possibly the $1^{+-}$ tetraquarks, and $X(3872)$ is possibly a $1^{++}$ tetraquark. $X(4250)$ may be a $0^{-+}$, $0^{++}$ or $1^{-+}$ tetraquark, $X(4240)$ may be a $0^{--}$ tetraquark. With radial excitations, $X(4350)$ may be a $0^{++}$ tetraquark, $Z_c(4430)$ may be a $1^{+-}$ tetraquark, $X(4630)$ may be a $0^{-+}$ or $1^{-+}$ tetraquark, and $X(Y)(4660)$ may be the $1^{--}$ tetraquark. $Y(4008)$ or $Y(4390)$ seems impossibly the $1^{--}$ tetraquark.

hep-ph

Assignment of charmed-strange $D_{s0}(2590)^+$ and $D_{sJ}(3040)^+$

Based on analyses of the mass and the strong decay features, $D_{s0}(2590)^+$ observed by LHCb collaboration is identified as a radial excitation of the pseudoscalar $D_s$, and $D_{sJ}(3040)^+$ observed by BaBar collaboration is identified as a radial excitation of $D_{s1}(2536)^\pm$. $D_{s0}(2590)^+$ is possibly a pure $D_{s}(2~^1S_0)$ meson, both basic $D_{s1}(2536)^\pm$ and radially excited $D_{sJ}(3040)^+$ are possibly the mixtures $D_s(nP_1)$ between spin triplet $D_s(n~^3P_1)$ and spin singlet $D_s(n~^1P_1)$. In this arrangement, their masses meet the linear behavior of the radial Regge trajectory very well. In the $^3P_0$ strong decay model, the decay channels of $D_{s0}(2590)^+$ are $D^{*0}K^+$ and $D^{*+}K^0$, the total decay width is predicted with $Γ=76.12$ MeV. The main decay channels of $D_{sJ}(3040)^+$ are $D^{*0}K^+$/$D^{*+}K^0$ and $D^{*0}K^{*+}$/$D^{*+}K^{*0}$, the total decay width is predicted with $Γ=283.46$ MeV. These numerical strong decay results are consistent with the experiment data and support our arrangement. The dimensionless strength creation parameter $γ$ plays an important role in the calculation, and $γ=9.57$ is fixed through a comparison of the predicted strong decay widths of $D^*_{s2}(2573)$ and $D^*_{s3}(2860)^{\pm}$ with experimental data.

hep-ph

Mass spectrum of fully charmed $[cc][\bar c\bar c]$ tetraquarks

There are three $S$ and seven $P$ fully charmed $[cc][\bar c\bar c]$ tetraquarks, the mass spectrum from $1S$ to $2P$ excitations is calculated in a non-relativistic quark potential model. In the calculation, the interactions among four internal quarks/antiquark are approximated as a dominant color interaction between a diquark and an antidiquark, and a residual interaction responsible for the diquark/antidiquark cluster effect. The color interaction between the diquark and the antidiquark is characterized by the conventional Cornell potential, while the residual interaction is modeled as the Yukawa-type scalar $σ$ and vector $ω$ boson exchange potentials. In the numerical results, though the scalar $σ$ and vector $ω$ boson exchange interactions reduce the masses of $S-$wave $[cc][\bar c\bar c]$ tetraquarks $40-50$ MeV, they contribute to the masses of other $[cc][\bar c\bar c]$ tetraquarks small. The mass splittings of $[cc][\bar c\bar c]$ tetraquarks between different multiplets and within the same multiplet are smaller than those in charmonium, and the splittings are affected by the scalar $σ$ or vector $ω$ boson exchange interactions small. Our calculations suggest that the observed $X(6600)$, $X(6900)$ and $X(7300)$ should be different radial excitations of $[cc][\bar c\bar c]$. The measurements of the $J^{PC}$ quantum numbers and the mass splittings will be helpful to identify and understand of the $[cc][\bar c\bar c]$ candidates.

hep-ph

Dynamical mixing between $2^3S_1$ and $1^3D_1$ charmed mesons

In charmed $D$ and $D_s$ mesons sector, the matrix of a Hamiltonian in a quark potential model is computed in the $2^3S_1$ and $1^3D_1$ subspace. The masses of four mixed states of $2^3S_1$ and $1^3D_1$ denoted with $D^*_1(2635)$, $D^*_1(2739)$, $D^*_{s1}(2715)$ and $D^*_{s1}(2805)$ are obtained. It is an off-diagonal part of the spin-orbit tensor interaction that causes the mixing between the $2^3S_1$ and $1^3D_1$ states. The mixing angles between the $2^3S_1$ and $1^3D_1$ states are tiny. Under the mixing, a $^3P_0$ model is employed to compute the hadronic decay widths of all OZI-allowed decay channels of the four mixed states. The two light mixed states $D^*_1(2635)$ and $D^*_{s1}(2715)$ are close in mass to $D^*_J(2600)$ and $D^*_{s1}(2700)$, while the two heavy mixed states $D^*_1(2739)$ and $D^*_{s1}(2805)$ are lighter in mass than $D(2750)$ and $D^*_{s1}(2860)$. The mixing angles obtained from dynamical interaction are inconsistent with the mixing angles obtained from hadronic decay. Based on mass spectra and hadronic decay analyses, $D^*_J(2600)$, $D(2750)$, $D^*_{s1}(2700)$ and $D^*_{s1}(2860)$ are impossibly the mixed states of $2^3S_1$ and $1^3D_1$ at the small mixing angles. The inconsistence implies that $D^*_1(2760)$ and $D^*_{s1}(2860)$ have not been properly resolved from present experimental data, or there exist large unknown off-diagonal interactions that result in large mixing angles.

hep-ph

Jantzen coefficients and simplicity of generalized Verma modules

The main purpose of the paper is to establish new tools in the study of $\mathcal{O}^\mathfrak{p}$. We introduce the Jantzen coefficients of generalized Verma modules. It comes from the Jantzen's simplicity criteria for generalized Verma modules and has a deep relation with the structure of $\mathcal{O}^\mathfrak{p}$. We develop a reduction process to compute those coefficients. For which we need to consider generalized Verma modules induced from maximal parabolic subalgebras having maximal nontrivial singularity, so called basic generalized Verma modules. The classification of such modules is obtained in this paper. As the first application of our results, we give a refinement of Jantzen's simplicity criteria.

math.RT

Bottomonium spectrum in the relativistic flux tube model

The bottomonium spectrum is far from being established. The structures of higher vector states, including the $Υ(10580)$, $Υ(10860)$, and $Υ(11020)$ states, are still in dispute. In addition, whether the $Υ(10750)$ signal which was recently observed by the Belle Collaboration is a normal $b\bar{b}$ state or not should be examined. Faced with such a situation, we carried out a systematic investigation of the bottomonium spectrum in the scheme of the relativistic flux tube (RFT) model. A Chew-Frautschi like formula was derived analytically for the spin average mass of bottomonium states. We further incorporated the spin-dependent interactions and obtained a complete bottomonium spectrum. We found that the most established bottomonium states can be explained in the RFT scheme. The $Υ(10750)$, $Υ(10860)$, and $Υ(11020)$ could be predominantly the $3^3D_1$, $5^3S_1$, and $4^3D_1$ states, respectively. Our predicted masses of $1F$ and $1G$ $b\bar{b}$ states are in agreement with the results given by the method of lattice QCD, which can be tested by experiments in future. We also compared the RFT model with the quark potential model in detail. The differences of these two kinds of models were discussed.

hep-ph

Strong Decays of observed $Λ_c$ Baryons in the $^3P_0$ Model

The strong decay widths and some important branching ratios of possible Okubo-Zweig-Iizuka(OZI)-allowed strong decay channels of $Λ_c(2595)^+$, $Λ_c(2625)^+$, $Λ_c(2765)^+$ ($Σ_c(2765)^+$), $Λ_c(2860)^+$, $Λ_c(2880)^+$ and $Λ_c(2940)^+$ are computed in a $^{3}P_{0}$ model, and possible assignments of these $Λ_c$ are given. (1), $Λ_c(2595)^+$ and $Λ_c(2625)^+$ are possibly the $1P$-wave charmed baryons $Λ_{c1}(\frac{1}{2}^-)$ and $Λ_{c1}(\frac{3}{2}^-)$, respectively. (2), $Λ_c(2765)^+$ ($Σ_c(2765)^+$) seems impossibly the $1P$-wave $Λ_{c}$, it could be the $2S$-wave or $1D$-wave charmed baryon. So far, the experimental information has not been sufficient for its identification. (3), $Λ_c(2860)^+$ seems impossibly $2S$-wave charmed baryon, it may be the $P$-wave $\tildeΛ_{c2}^{ }(\frac{3}{2}^-)$ or $\tildeΛ_{c2}^{ }(\frac{5}{2}^-)$, it could also be the $D$-wave $\checkΛ_{c1}^{2}(\frac{1}{2}^+)$ or $\checkΛ_{c1}^{2}(\frac{3}{2}^+)$. If the hypothesis that $Λ_c(2860)^+$ has $J^P={3\over 2}^+$ is true, $Λ_c(2860)^+$ is possibly the $D$-wave $\checkΛ_{c1}^{2}(\frac{3}{2}^+)$ which has a predicted branching ratio $R=Γ(Σ_c(2520)π)/Γ(Σ_c(2455)π)=2.8$. (4), $Λ_c(2880)^+$ is impossibly a $1P$-wave or $2S$-wave charmed baryon, it may be a $D$-wave $\checkΛ_{c3}^{2}(\frac{5}{2}^+)$ with $Γ_{total}=1.3$ MeV. The predicted branching ratio $R=Γ(Σ_c(2520)π)/Γ(Σ_c(2455)π)=0.35$, which is consistent with experiment. (5), $Λ_c(2940)^+$ is the $P$-wave $\tildeΛ_{c2}^{ }(\frac{3}{2}^-)$ or $\tildeΛ_{c2}^{ }(\frac{5}{2}^-)$, it is also possibly the $D$-wave $\checkΛ_{c3}^{2}(\frac{5}{2}^+)$ or $\checkΛ_{c3}^{2}(\frac{7}{2}^+)$.

hep-ph

Identification of the newly observed $Σ_b(6097)^\pm$ baryons from their strong decays

Two bottom $Σ_b(6097)^\pm$ baryons were observed in the final states $Λ_b^0π^-$ and $Λ_b^0π^+$ in $pp$ collision by LHCb collaboration, whose masses and widths were measured. In a $^{3}P_{0}$ model, the strong decay widths of two ground $S$-wave and seven excited $P$-wave $Σ_b$ baryons have been systematically computed. Numerical results indicate that the newly observed $Σ_b(6097)^\pm$ are very possibly $Σ_{b2}^1({3\over 2}^-)$ with $J^P={3\over 2}^-$ or $Σ_{b2}^1({5\over 2}^-)$ with $J^P={5\over 2}^-$. The predicted decay widths of $Σ_b(6097)^\pm$ are consistent with experimental measurement from LHCb. In particular, it may be possible to distinguish these two assignments through ratios $Γ({Σ_b(6097)^\pm\to Σ_b^\pmπ^0})/Γ({Σ_b(6097)^\pm\to Σ_b^{*\pm}π^0})$, which can be measured by experiments in the future. In the meantime, our results support the assignments that $Σ_b^\pm$ and $Σ_b^{*\pm}$ are the ground $S$-wave $Σ_b$ baryons with $J^P={1\over 2}^+$ and $J^P={3\over 2}^+$, respectively.

hep-ph

Role of newly discovered $Ξ_b(6227)^-$ for constructing excited bottom baryon family

Selecting the newly observed $Ξ_b(6227)^-$ by LHCb as a study example, we decode its inner structure by giving the mass spectrum analysis and the investigation of its two-body strong decay behaviors. Our result indicates that the $Ξ_b(6227)^-$ is a good candidate of the $P$-wave $Ξ_b^{\prime}$ state with $J^P=3/2^-$ or $5/2^-$. In addition, we further provide the information of the properties of the partners of the $Ξ_b(6227)^-$. These predicted states include three $2S$ states and the remaining $1P$ states in the bottom-strange baryon family. The calculated sizable Okubo-Zweig-Iizuka$-$allowed decay widths of these partners show that the experimental search for them becomes possible via LHCb. We have a reason to believe that the present study can be treated as a start point for constructing the highly excited bottom baryon spectroscopy.

hep-ph

Study of $P$-wave excitations of observed charmed strange baryons

Many excited charmed strange baryons such as $Ξ_c(2790)$, $Ξ_c(2815)$, $Ξ_c(2930)$, $Ξ_c(2980)$, $Ξ_c(3055)$, $Ξ_c(3080)$ and $Ξ_c(3123)$ have been observed. In order to understand their internal structure and to determine their spin-parities, the strong decay properties of these baryons as possible $P$-wave excited $Ξ_c$ candidates have been systematically studied in a $^3P_0$ model. The configurations and $J^P$ assignments of $Ξ_c(2790)$, $Ξ_c(2815)$, $Ξ_c(2930)$, $Ξ_c(2980)$, $Ξ_c(3055)$, $Ξ_c(3080)$ and $Ξ_c(3123)$ have been explored based on recent experimental data. In our analyses, $Ξ_c(3055)$, $Ξ_c(3080)$ and $Ξ_c(3123)$ seem impossible to be the $P$-wave excited $Ξ_c$. $Ξ_c(2790)$, $Ξ_c(2815)$, $Ξ_c(2930)$ and $Ξ_c(2980)$ may be the $P$-wave excited $Ξ_c$. In particular, $Ξ_c(2790)$ and $Ξ_c(2815)$ are very possibly the $P$-wave excited $Ξ_{c1}(1/2^-)$ and $Ξ_{c1}(3/2^-)$, respectively. $Ξ_c(2980)$ may be the $P$-wave excited $Ξ_{c1}^{'}(\frac{1}{2}^-)$. $Ξ_c(2930)$ may be the $P$-wave $Ξ_{c0}^{'}(\frac{1}{2}^-)$, $\tildeΞ_{c0}(\frac{1}{2}^-)$, $Ξ_{c2}^{'}(\frac{3}{2}^-)$, $Ξ_{c2}^{'}(\frac{5}{2}^-)$, $\tildeΞ_{c2}(\frac{3}{2}^-)$ or $\tildeΞ_{c2}(\frac{5}{2}^-)$. Furthermore, some branching fraction ratios related to the internal structure and quark configuration of $P$-wave $Ξ_c$ have also been computed. Measurements of these ratios in the future will be helpful to understand these excited $Ξ_c$.

hep-ph

Study of $2S$- and $1D$- excitations of observed charmed strange baryons

Strong decays of $Ξ_c$ baryons with radial or orbital excitations with positive parity have been studied in a $^3P_0$ model. As candidates of these $Xi_c$, possible configurations and $J^P$ of $Ξ_c(2930)$, $Ξ_c(2980)$, $Ξ_c(3055)$, $Ξ_c(3080)$ and $Ξ_c(3123)$ have been assigned. There are $40$ kinds of configurations to describe these excited $Ξ_c$. In these assignments, $Ξ_c(2930)$ may be a $2S$-wave excited $\tildeΞ_{c1}(\frac{1}{2}^+)$ or $\tildeΞ_{c1}(\frac{3}{2}^+)$, or a $D$-wave excited $\hatΞ_{c1}^{' }(\frac{1}{2}^+)$, $\checkΞ_{c1}^{\ 0}(\frac{1}{2}^+)$, $\checkΞ_{c1}^{\ 2}(\frac{1}{2}^+)$, $\hatΞ_{c1}^{' }(\frac{3}{2}^+)$, $\checkΞ_{c1}^{\ 0}(\frac{3}{2}^+)$ or $\checkΞ_{c1}^{\ 2}(\frac{3}{2}^+)$. $Ξ_c(2980)^+$ may be a $2S$-wave excited $\tildeΞ_{c1}(\frac{1}{2}^+)$ or $\tildeΞ_{c0}^{'}(\frac{1}{2}^+)$ with $J^P={1\over 2}^+$, or a $D$-wave excited $\checkΞ_{c0}^{'0}(\frac{1}{2}^+)$ or $\checkΞ_{c1}^{\ 0}(\frac{1}{2}^+)$ with $J^P={1\over 2}^+$. $Ξ_c(3055)^+$ may be a $2S$-wave excited $\acuteΞ_{c1}^{'}(\frac{3}{2}^+)$ or $\acuteΞ_{c0}(\frac{1}{2}^+)$. It may be a $D$-wave excited $Ξ_{c1}^{' }(\frac{3}{2}^+)$, $Ξ_{c2}^{' }(\frac{5}{2}^+)$, $Ξ_{c2}^{ }(\frac{3}{2}^+)$ or $Ξ_{c2}^{ }(\frac{5}{2}^+)$. $Ξ_c(3080)^+$ is very possibly a $2S$-wave excited $\acuteΞ_{c0}(\frac{1}{2}^+)$, and seems not a $D$-wave excitation of $Ξ_c$. For the poor experimental information of $Ξ_c(3123)$, it is impossible to identify this state at present. It is found that the channel $ΛD$ vanishes in the strong decay of $P$-wave, $D$-wave and $2S$-wave excited $Ξ_c$ without $ρ$- mode excitation between the two light quarks ($n_ρ=L_ρ=0$). Some branching fraction ratios have been computed and can be employed to distinguish different configurations in forthcoming experiments.

hep-ph