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Measurements of $$ {K}_S^0 $$ - $$ {K}_L^0 $$ asymmetries in the decays $$ {Lambda}_c^{+}to p{K}_{L,S}^0 $$ , $$ p{K}_{L,S}^0{pi}^{+}{pi}^{-} $$ and $$ p{K}_{L,S}^0{pi}^0 $$ 在衰变 $$ {Lambda}_c^{+}to p{K}_{L,S}^0 $$ , $$ p{K}_{L,S}^0{pi}^{+}{pi}^{-} 中测量 $$ {K}_S^0 $$ - $$ {K}_L^0 $$ 的不对称性。$$ 和 $$ p{K}_{L,S}^0{pi}^0 $$
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-09-03 DOI: 10.1007/jhep09(2024)007
M. Ablikim, M. N. Achasov, P. Adlarson, O. Afedulidis, X. C. Ai, R. Aliberti, A. Amoroso, Q. An, Y. Bai, O. Bakina, I. Balossino, Y. Ban, H.-R. Bao, V. Batozskaya, K. Begzsuren, N. Berger, M. Berlowski, M. Bertani, D. Bettoni, F. Bianchi, E. Bianco, A. Bortone, I. Boyko, R. A. Briere, A. Brueggemann, H. Cai, X. Cai, A. Calcaterra, G. F. Cao, N. Cao, S. A. Cetin, J. F. Chang, G. R. Che, G. Chelkov, C. Chen, C. H. Chen, Chao Chen, G. Chen, H. S. Chen, H. Y. Chen, M. L. Chen, S. J. Chen, S. L. Chen, S. M. Chen, T. Chen, X. R. Chen, X. T. Chen, Y. B. Chen, Y. Q. Chen, Z. J. Chen, Z. Y. Chen, S. K. Choi, G. Cibinetto, F. Cossio, J. J. Cui, H. L. Dai, J. P. Dai, A. Dbeyssi, R. E. de Boer, D. Dedovich, C. Q. Deng, Z. Y. Deng, A. Denig, I. Denysenko, M. Destefanis, F. De Mori, B. Ding, X. X. Ding, Y. Ding, Y. Ding, J. Dong, L. Y. Dong, M. Y. Dong, X. Dong, M. C. Du, S. X. Du, Y. Y. Duan, Z. H. Duan, P. Egorov, Y. H. Fan, J. Fang, J. Fang, S. S. Fang, W. X. Fang, Y. Fang, Y. Q. Fang, ..

Using e+e annihilation data sets corresponding to an integrated luminosity of 4.5 fb1, collected with the BESIII detector at center-of-mass energies between 4.600 and 4.699 GeV, we report the first measurements of the absolute branching fractions ( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0right) ) = (1.67 ± 0.06 ± 0.04)%, ( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0{pi}^{+}{pi}^{-}right) ) = (1.69 ± 0.10 ± 0.05)%, and ( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0{pi}^0right) ) = (2.02 ± 0.13 ± 0.05)%, where the first uncertainties are statistical and the second systematic. Combining with the known branching fractions of ( {Lambda}_c^{+}to p{K}_S^0 ), ( {Lambda}_c^{+}to p{K}_S^0{pi}^{+}{pi}^{-} ), and ( {Lambda}_c^{+}to p{K}_S^0{pi}^0 ), we present the first measurements of the ( {K}_S^0 )-( {K}_L^0 ) asymmetries ( Rleft({Lambda}_c^{+},{K}_{S,L}^0Xright)=frac{mathcal{B}left({Lambda}_c^{+}to {K}_S^0Xright)-mathcal{B}left({Lambda}_c^{+}to {K}_L^0Xright)}{mathcal{B}left({Lambda}_c^{+}to {K}_S^0Xright)+mathcal{B}left({Lambda}_c^{+}to {K}_L^0Xright)} ) in charmed baryon decays: ( Rleft({Lambda}_c^{+},p{K}_{S,L}^0right)=-0.025pm 0.031 ), ( Rleft({Lambda}_c^{+},p{K}_{S,L}^0{pi}^{+}{pi}^{-}right)=-0.027pm 0.048 ) and ( Rleft({Lambda}_c^{+},p{K}_{S,L}^0{pi}^0right)=-0.015pm 0.046 ). No significant asymmetries with statistical significance are observed.

利用BESIII探测器在4.600和4.699 GeV之间的质心能量上收集到的对应于4.5 fb-1综合光度的e+e-湮灭数据集,我们报告了对绝对分支分数( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0right) ) = (1.67 ± 0.06 ± 0.04)%,( ( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0{pi}^{+}{pi}^{-}right) = (1.69 ± 0.10 ± 0.05)%,而 ( mathcal{B}left({Lambda}_c^{+}to p{K}_L^0{pi}^0right) ) = (2.02 ± 0.13 ± 0.05)%,其中第一个不确定性是统计不确定性,第二个是系统不确定性。结合已知的 ( {Lambda}_c^{+}to p{K}_S^0 ), ( {Lambda}_c^{+}to p{K}_S^0{pi}^{+}{pi}^{-} )、和( {Lambda}_c^{+}to p{K}_S^0{pi}^0 ),我们首次测量了( {K}_S^0 )-( {K}_L^0 )不对称的( ( Rleft({Lambda}_c^{+}、{K}_{S、L}^0Xright)=frac{mathcal{B}left({Lambda}_c^{+}to {K}_S^0Xright)-}{mathcal{B}left({Lambda}_c^{+}to {K}_L^0Xright)} {mathcal{B}left({Lambda}_c^{+}to {K}_S^0Xright)+mathcal{B}left({Lambda}_c^{+}to {K}_L^0Xright)}) in charmed baryon decays:( Rleft({Lambda}_c^{+},p{K}_{S,L}^0right)=-0.025pm 0.031 ), ( Rleft({Lambda}_c^{+},p{K}_{S,L}^0pi}^{+}{pi}^{-}right)=-0.027pm 0.048) and( Rleft({Lambda}_c^{+},p{K}_{S,L}^0{pi}^0right)=-0.015pm 0.046).没有观察到具有统计学意义的明显不对称性。
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引用次数: 0
Missing energy plus jet in the SMEFT SMEFT 中的失踪能量加射流
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-09-03 DOI: 10.1007/jhep09(2024)009
Gudrun Hiller, Daniel Wendler

We study the production of dineutrinos in proton-proton collisions, with large missing transverse energy and an energetic jet as the experimental signature. Recasting a search from the ATLAS collaboration we work out constraints on semileptonic four-fermion operators, gluon and electroweak dipole operators and Z-penguins in the SMEFT. All but the Z-penguin operators experience energy-enhancement. Constraints on gluon dipole operators are the strongest, probing new physics up to 14 TeV, and improve over existing ones from collider studies. Limits on FCNC four-fermion operators are competitive with Drell-Yan production of dileptons, and improve on those for tau final states. For left-handed |∆s| = |∆d| = 1 and right-handed |∆c| = |∆u| = 1 transitions these are the best available limits, also considering rare kaon and charm decays. We estimate improvements for the 3000 fb−1 High Luminosity Large Hadron Collider.

我们研究了质子-质子对撞中产生的正中微子,其实验特征是巨大的缺失横向能量和高能喷流。我们重塑了 ATLAS 合作研究的搜索结果,研究了 SMEFT 中对半轻子四费米子算子、胶子和电弱偶极子算子以及 Z 企鹅的约束。除了 Z 企鹅算子之外,所有算子都经历了能量增强。对胶子偶极子算子的约束是最强的,探测了高达 14 TeV 的新物理,并改进了对撞机研究的现有约束。对FCNC四费米子算子的限制与二重子的德雷尔-扬产生具有竞争性,并改进了对tau终态的限制。对于左手|Δs| = |Δd|=1和右手|Δc| = |Δu|=1转换,这些是现有的最佳极限,同时也考虑了罕见的κ子和粲子衰变。我们估计了 3000 fb-1 高亮度大型强子对撞机的改进情况。
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引用次数: 0
Tree-level superstring amplitudes: the Neveu-Schwarz sector 树级超弦振幅:奈沃-施瓦兹扇面
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-09-03 DOI: 10.1007/jhep09(2024)008
Sergio L. Cacciatori, Samuel Grushevsky, Alexander A. Voronov

We present a complete computation of superstring scattering amplitudes at tree level, for the case of Neveu-Schwarz insertions. Mathematically, this is to say that we determine explicitly the superstring measure on the moduli space ( {mathcal{M}}_{0,n,0} ) of super Riemann surfaces of genus zero with n ≥ 3 Neveu-Schwarz punctures. While, of course, an expression for the measure was previously known, we do this from first principles, using the canonically defined super Mumford isomorphism [1]. We thus determine the scattering amplitudes, explicitly in the global coordinates on ( {mathcal{M}}_{0,n,0} ), without the need for picture changing operators or ghosts, and are also able to determine canonically the value of the coupling constant. Our computation should be viewed as a step towards performing similar analysis on ( {mathcal{M}}_{0,0,n} ), to derive explicit tree-level scattering amplitudes with Ramond insertions.

我们提出了一种在树级上完整计算超弦散射振幅的方法,适用于内韦乌-施瓦茨(Neveu-Schwarz)插入的情况。从数学上讲,这意味着我们明确地确定了零属超黎曼曲面的模空间({mathcal{M}}_{0,n,0} )上的超弦度量,这些曲面具有 n ≥ 3 个内韦乌-施瓦茨穿刺。当然,我们以前就知道量纲的表达式,但这次我们利用经典定义的超芒福德同构[1],从第一性原理出发。因此,我们在全局坐标上明确地确定了散射振幅({mathcal{M}}_{0,n,0} ),而不需要改变图象的算子或重影,并且还能够规范地确定耦合常数的值。我们的计算应该被视为在 ( {mathcal{M}}_{0,0,n} ) 上进行类似分析的一个步骤,从而推导出带有拉蒙插入的明确的树级散射振幅。
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引用次数: 0
Defect fusion and Casimir energy in higher dimensions 高维度的缺陷聚变和卡西米尔能
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-09-02 DOI: 10.1007/jhep09(2024)006
Oleksandr Diatlyk, Himanshu Khanchandani, Fedor K. Popov, Yifan Wang

We study the operator algebra of extended conformal defects in more than two spacetime dimensions. Such algebra structure encodes the combined effect of multiple impurities on physical observables at long distances as well as the interactions among the impurities. These features are formalized by a fusion product which we define for a pair of defects, after isolating divergences that capture the effective potential between the defects, which generalizes the usual Casimir energy. We discuss general properties of the corresponding fusion algebra and contrast with the more familiar cases that involve topological defects. We also describe the relation to a different defect setup in the shape of a wedge. We provide explicit examples to illustrate these properties using line defects and interfaces in the Wilson-Fisher CFT and the Gross-Neveu(-Yukawa) CFT and determine the defect fusion data thereof.

我们研究了超过两个时空维度的扩展共形缺陷的算子代数。这种代数结构编码了多个杂质对远距离物理观测值的综合影响以及杂质之间的相互作用。在分离出捕捉缺陷间有效势能的发散之后,我们为一对缺陷定义了融合积,从而将这些特征形式化,而这一融合积概括了通常的卡西米尔能。我们讨论了相应融合代数的一般性质,并与我们更熟悉的涉及拓扑缺陷的情况进行了对比。我们还描述了与不同的楔形缺陷设置的关系。我们提供了明确的例子,用威尔逊-费舍 CFT 和格罗斯-涅维乌(-汤川)CFT 中的线缺陷和界面来说明这些性质,并确定了其中的缺陷融合数据。
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引用次数: 0
Massive twistor worldline in electromagnetic fields 电磁场中的大规模扭曲世界线
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-09 DOI: 10.1007/jhep08(2024)080
Joon-Hwi Kim, Jung-Wook Kim, Sangmin Lee

We study the (ambi-)twistor model for spinning particles interacting via electromagnetic field, as a toy model for studying classical dynamics of gravitating bodies including effects of both spins to all orders. We compute the momentum kick and spin kick up to one-loop order and show precisely how they are encoded in the classical eikonal. The all-orders-in-spin effects are encoded as a dynamical implementation of the Newman-Janis shift, and we find that the expansion in both spins can be resummed to simple expressions in special kinematic configurations, at least up to one-loop order. We confirm that the classical eikonal can be understood as the generator of canonical transformations that map the in-states of a scattering process to the out-states. We also remark that cut contributions for converting worldline propagators from time-symmetric to retarded amount to the iterated action of the leading eikonal at one-loop order.

我们研究了通过电磁场相互作用的自旋粒子的(ambi-)扭转模型,将其作为研究引力体经典动力学的玩具模型,包括所有阶次的自旋效应。我们计算了高达一环阶的动量踢和自旋踢,并精确地展示了它们是如何在经典电子函件中编码的。全阶自旋效应被编码为纽曼-詹尼斯位移的动力学实现,我们发现在特殊的运动构型中,两种自旋的扩展都可以重和为简单的表达式,至少可以达到一环阶。我们证实,经典电子函纳可以理解为将散射过程的入态映射到出态的典型变换的发生器。我们还注意到,将世界线传播者从时间对称转换为迟滞传播者的切贡献相当于一回路阶的前导 Eikonal 的迭代作用。
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引用次数: 0
Consistent actions for massive particles interacting with electromagnetism and gravity 与电磁力和引力相互作用的大质量粒子的一致行动
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-09 DOI: 10.1007/jhep08(2024)081
Lukas W. Lindwasser

Consistent interactions with electromagnetism and gravity for mass m particles of any spin are obtained. This is done by finding interactions which preserve the covariantized massive gauge symmetry present in recently constructed massive particle actions. This gauge principle is sufficient for finding consistent completions of minimal as well as non-minimal couplings of any type. For spins s ≥ 3/2, consistency requires infinitely many interaction terms in the action, including arbitrarily high order derivatives of electromagnetic and gravitational curvatures, with correspondingly high powers of 1/m. These interactions may be formally resummed and expressed in terms of non-local operators. Finally, although the interactions appear non-local, evidence is presented for the existence of a field redefinition which makes the interacting action local. This work provides the first explicit realization of an exactly gauge invariant formulation of massive particles interacting with electromagnetism and gravity.

对于任意自旋的质量为 m 的粒子,我们获得了与电磁力和引力一致的相互作用。这是通过寻找相互作用来实现的,这种相互作用保留了最近构建的大质量粒子作用中存在的共变大质量规对称性。这个量规原理足以找到任何类型的最小和非最小耦合的一致补全。对于自旋 s ≥ 3/2,一致性要求在作用中包含无限多的相互作用项,包括电磁和引力曲率的任意高阶导数,以及相应的 1/m 的高次幂。这些相互作用可以用非局部算子形式重和和表达。最后,尽管这些相互作用看起来是非局部的,但有证据表明存在着一种场的重新定义,这种场的重新定义使相互作用成为局部的。这项研究首次明确实现了大质量粒子与电磁和引力相互作用的精确规不变表述。
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引用次数: 0
Spectral representation in Klein space: simplifying celestial leaf amplitudes 克莱因空间的光谱表示:简化天体叶振幅
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-09 DOI: 10.1007/jhep08(2024)079
Sarthak Duary, Sourav Maji

In this paper, we explore the spectral representation in Klein space, which is the split (2, 2) signature flat spacetime. The Klein space can be foliated into Lorentzian AdS3/ slices, and its identity resolution has continuous and discrete parts. We calculate the identity resolution and the Plancherel measure in these slices. Using the foliation of Klein space into the slices, the identity resolution, and the Plancherel measure in each slice, we compute the spectral representation of the massive bulk-to-bulk propagator in Klein space. It can be expressed as the sum of the product of two massive (or tachyonic) conformal primary wavefunctions, with both continuous and discrete parts, and sharing a common boundary coordinate. An interesting point in Klein space is that, since the identity resolution has discrete and continuous parts, a new type of conformal primary wavefunction naturally arises for the massive (or tachyonic) case. For the conformal primary wavefunctions, both the discrete and continuous parts involve integrating over the common boundary coordinate and the real (or imaginary) mass. The conformal dimension is summed in the discrete part, whereas it is integrated in the continuous part. The spectral representation in Klein space is a computational tool to derive conformal block expansions for celestial amplitudes in Klein space and its building blocks, called celestial leaf amplitudes, by integrating the particle interaction vertex over a single slice of foliation.

本文探讨了克莱因空间的谱表示,即分裂(2,2)签名平坦时空。克莱因空间可以对折成洛伦兹AdS3/ℤ切片,其特征解析有连续和离散两部分。我们计算这些切片中的同一解析度和 Plancherel 度量。利用克莱因空间对切片的对折、同一性解析和每个切片中的 Plancherel 度量,我们计算了克莱因空间中大质量体对大质量体传播者的谱表示。它可以表示为两个大质量(或超音速)共形主波函数的乘积之和,其中既有连续部分,也有离散部分,并共享一个共同的边界坐标。克莱因空间的一个有趣之处在于,由于同一解析具有离散和连续部分,在大质量(或超音速)情况下自然会产生一种新型的共形主波函数。对于保角主波函数,离散和连续部分都涉及对共同边界坐标和实(或虚)质量的积分。共形维度在离散部分求和,而在连续部分积分。克莱因空间的谱表示是一种计算工具,通过对粒子相互作用顶点在单片折线上的积分,推导出克莱因空间天体振幅的共形块展开及其构件(称为天体叶振幅)。
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引用次数: 0
Pileup density estimate independent on jet multiplicity 堆积密度估算与喷流倍率无关
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-09 DOI: 10.1007/jhep08(2024)078
P. Berta, J. Smieško, M. Spousta

The hard-scatter processes in hadronic collisions are often largely contaminated with soft background coming from pileup in proton-proton collisions, or underlying event in heavy-ion collisions. There are multiple methods to remove the effect of pileup for jets. Two such methods, Area Subtraction and Constituent Subtraction, use the pileup density as the main ingredient to estimate the magnitude of pileup contribution on an event-by-event basis. The state-of-the-art approaches to estimating pileup density are sensitive to the number of hard-scatter jets in the event. This paper presents a new pileup-density estimation method that minimizes the sensitivity on the presence of hard-scatter jets in the event. Using a detector-level simulation, we provide a comparison of the new method with the state-of-the-art estimation methods. We observe a significantly lower bias for the estimated pileup density when using the new method. We conclude that the new method has the potential to significantly improve pileup mitigation in proton-proton collisions or the underlying event subtraction in heavy-ion collisions.

强子对撞中的硬散射过程往往在很大程度上被质子-质子对撞中的堆积或重离子对撞中的潜在事件产生的软背景所污染。有多种方法可以消除射流的堆积效应。其中两种方法,即面积减法和成分减法,使用堆积密度作为主要成分,逐个事件估计堆积的贡献大小。最先进的堆积密度估算方法对事件中硬散射射流的数量很敏感。本文提出了一种新的堆积密度估算方法,它能最大限度地降低对事件中是否存在硬散射射流的敏感性。通过探测器级模拟,我们将新方法与最先进的估计方法进行了比较。我们发现,在使用新方法时,估计堆积密度的偏差明显降低。我们的结论是,新方法有可能显著改善质子-质子碰撞中的堆积减缓或重离子碰撞中的基本事件减除。
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引用次数: 0
Holographic fluids from 5D dilaton gravity 来自 5D 稀释引力的全息流体
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-09 DOI: 10.1007/jhep08(2024)077
Sylvain Fichet, Eugenio Megías, Mariano Quirós

We study a solvable class of five-dimensional dilaton gravity models that continuously interpolate between anti-de Sitter (AdS5), linear dilaton (LD5) and positively curved spacetimes as a function of a continuous parameter ν. The dilaton vacuum expectation value is set by a potential localized on a flat brane. We chart the elementary properties of these backgrounds for any admissible ν, and determine stability conditions of the brane-dilaton system. We find that the spectrum of metric fluctuations can be either continuous or discrete. It features a massless graviton mode confined between the brane and the curvature singularity, and a massive radion mode tied to brane-dilaton stability. We show that, in the presence of a bulk black hole, the holographic theory living on the brane features a perfect fluid. The equation of state of the holographic fluid interpolates between radiation, pressureless matter and vacuum energy as a function of ν. This extends earlier findings on holographic fluids. Our results suggest that the thermodynamics of the fluid mirrors precisely the thermodynamics of the bulk black hole.

我们研究了一类可解的五维稀拉顿引力模型,该模型在反德西特(AdS5)、线性稀拉顿(LD5)和正曲时空之间连续插值,是连续参数ν的函数。稀拉顿的真空期望值是由一个定位在平坦 "rane "上的势设定的。我们绘制了这些背景的基本特性图,适用于任何可容许的 ν,并确定了布线-稀拉顿系统的稳定条件。我们发现度量波动谱可以是连续的,也可以是离散的。它的特点是无质量引力子模式被限制在栅线和曲率奇点之间,而大质量辐射子模式则与栅线-迪拉顿稳定性相关。我们的研究表明,在存在大块黑洞的情况下,生活在鹤膜上的全息理论具有完美流体的特征。全息流体的状态方程是辐射、无压物质和真空能量之间的插值,是ν的函数。这扩展了早先关于全息流体的发现。我们的结果表明,流体的热力学恰好反映了体黑洞的热力学。
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引用次数: 0
Teleparallel Geroch geometry Teleparallel Geroch 几何图形
IF 5.4 1区 物理与天体物理 Q1 Physics and Astronomy Pub Date : 2024-08-08 DOI: 10.1007/jhep08(2024)076
Guillaume Bossard, Martin Cederwall, Jakob Palmkvist

We construct the teleparallel dynamics for extended geometry where the structure algebra is (an extension of) an untwisted affine Kac-Moody algebra. This provides a geometrisation of the Geroch symmetry appearing on dimensional reduction of a gravitational theory to two dimensions. The formalism is adapted to the underlying tensor hierarchy algebra, and will serve as a stepping stone towards the geometrisation of other infinite-dimensional, e.g. hyperbolic, symmetries.

我们构建了扩展几何的远距平行动力学,其中结构代数是非扭曲仿射 Kac-Moody 代数(的扩展)。这为引力理论降维到二维时出现的格罗赫对称性提供了几何解析。该形式主义适用于底层张量层次代数,并将作为其他无限维对称性(如双曲对称性)几何化的垫脚石。
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引用次数: 0
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Journal of High Energy Physics
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