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Towards NNLO QCD corrections to Higgs boson pair production 走向 NNLO QCD 对希格斯玻色子成对产生的修正
Pub Date : 2024-09-11 DOI: arxiv-2409.07573
Matthias Steinhauser
Higgs boson pair production plays an important role in the determination ofthe Higgs boson self coupling. The predictions based on next-to-leading ordercorrections show a large dependence on the renormalization scheme of the topquark mass, which requires a next-to-next-to-leading order calculation. Wediscuss the current status and show first results of the three-loop virtualcorrections.
希格斯玻色子对的产生在确定希格斯玻色子自耦合方面起着重要作用。基于次领先阶校正的预测显示出对顶夸克质量重正化方案的巨大依赖性,这需要次领先阶计算。我们讨论了三环虚拟校正的现状,并展示了三环虚拟校正的初步结果。
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引用次数: 0
Anomalous Ionization in the Central Molecular Zone by sub-GeV Dark Matter 亚GeV暗物质在中央分子区的反常电离作用
Pub Date : 2024-09-11 DOI: arxiv-2409.07515
Pedro De la Torre Luque, Shyam Balaji, Joseph Silk
We demonstrate that the anomalous ionization rate observed in the CentralMolecular Zone can be attributed to MeV dark matter annihilations into $e^+e^-$pairs for galactic dark matter profiles with slopes $gamma>1$. The lowannihilation cross-sections required avoid cosmological constraints and implyno detectable inverse Compton, bremsstrahlung or synchrotron emissions inradio, X and gamma rays. The possible connection to the source of theunexplained 511 keV line emission in the Galactic Center suggests that bothobservations could be correlated and have a common origin.
我们证明,在中央分子区观测到的异常电离率可归因于MeV暗物质湮灭成$e^+e^-$对,银河系暗物质剖面的斜率为$gamma>1$。所需的低湮灭截面避免了宇宙学约束,并意味着在无线电、X 射线和伽马射线中没有可探测到的反康普顿、轫致辐射或同步辐射。与银河中心的 511 keV 线发射源的可能联系表明,这两个观测结果可能是相关的,并且有一个共同的起源。
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引用次数: 0
Finite Energy Resolution, Correlations Between Bins and Non-Nested Hypotheses 有限能量分辨率、箱间相关性和非嵌套假设
Pub Date : 2024-09-11 DOI: arxiv-2409.07157
Emilio Ciuffoli, Jarah Evslin
We show that whenever independent events are binned, there is no correlationbetween bins. In particular, neither the uncertainty in the energy resolutionnor a systematic error in the energy response of a detector will lead to acorrelation between bins. This is in contrast with a result that recentlyappeared in the literature, where it was claimed that the finite energyresolution could induce correlation between bins, changing the distribution of$Deltachi^2$ when attempting to determine the neutrino mass ordering usingreactor neutrinos. We will compute the expression for the variance of$Deltachi^2$ in the case of non-nested hypotheses if correlations betweenbins are present, showing that they could indeed affect the distribution. Wewill also show, however, that the detector response cannot introducestatistical correlations between bins unless these are already present in theoriginal spectrum. Both of these results are valid in general: the absence ofcorrelation is true for any detector response and the distribution of$Deltachi^2$ in the presence of (intrinsic) correlations, while obtainedhaving the mass ordering in mind, it is true for any non-nested hypotheses.
我们的研究表明,只要对独立事件进行分选,分选之间就不存在相关性。特别是,无论是能量分辨率的不确定性,还是探测器能量响应的系统误差,都不会导致分箱之间的相关性。这与最近在文献中出现的一个结果形成了鲜明的对比,在文献中,有人声称有限的能量分辨率可能会引起分级之间的相关性,从而在试图使用反应堆中微子确定中微子质量排序时改变$Deltachi^2$的分布。我们将计算在非嵌套假设的情况下,如果bins之间存在相关性,$Deltachi^2$的方差表达式,表明它们确实会影响分布。然而,我们还将证明,探测器的响应不能引入频带间的统计相关性,除非这些相关性已经存在于原始频谱中。这两个结果在一般情况下都是有效的:不存在相关性对于任何探测器响应和存在(内在)相关性的$Deltachi^2$的分布都是真实的,而在考虑到质量排序的情况下得到的,它对于任何非嵌套假说都是真实的。
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引用次数: 0
Possibility of the experimental study on semi-leptonic and non-leptonic $D^*_{(s)}$ weak decays 对半轻子和非轻子 $D^*_{(s)}$ 弱衰变进行实验研究的可能性
Pub Date : 2024-09-11 DOI: arxiv-2409.07302
Hao Yang, Zhi-Qing Zhang, Peng Li, You-Ya Yang
Just like other heavy flavor mesons, the weak decays of $D^*_{(s)}$ mesonscan also provide a platform to check the Standard Model (SM), explore newphysics (NP) and understand the mechanisms of weak interactions. At present,the theoretical and experimental researches on $D^*_{(s)}$ mesons arerelatively limited. In addition to the dominant electromagnetic decays, the$D^*_{(s)}$ weak decays should also be feasible to explore the $D^*_{(s)}$mesons. In this paper, we use the covariant light-front quark model (CLFQM) tostudy the branching ratios of the semi-leptonic decays $D^*_{(s)}toPell^{+}nu_{ell}$ and the non-leptonic decays $D^*_{(s)}to PP, PV$ with$P=pi, K, eta^{(prime)}, V=rho, K^*, phi$ and $ell=e, mu$, which arewithin the range $10^{-13}sim 10^{-6}$. Among these decays, the channels$D_{s}^{*+}toeta ell^{+}nu_{ell}$ and $D^{*+}_{s}to etarho^{+}$ possessthe largest branching ratios, which can reach up to $10^{-6}$ order. Thesedecays are most likely to be accessible at the future high-luminosityexperiments. One can find that the branching ratios$mathcal{B}r(D_{s}^{*+}toeta ell^{+}nu_{ell})=1.46times10^{-6}$ and$mathcal{B}r(D_{s}^{*+}toeta rho^{+})=1.04times10^{-6}$ correspond to tensof thousands of events in the $e^+e^-$ collider experiments, such as the STCF,CEPC and FCC-ee, and tens of millions of events at the HL-LHC. In a word, it isfeasible to study the $D^*_{(s)}$ meson weak decays in the future experiments.Furthermore, we also predict and discuss another two physical observations,that is, the longitudinal polarization fraction $f_{L}$ and theforward-backward asymmetry $A_{FB}$, for our considered decays.
与其他重味介子一样,$D^*_{(s)}$介子的弱衰变也可以为检验标准模型(SM)、探索新物理(NP)和理解弱相互作用机制提供一个平台。目前,关于 $D^*_{(s)}$ 介子的理论和实验研究相对有限。除了主要的电磁衰变之外,$D^*_{(s)}$弱衰变也应该是探索$D^*_{(s)}$介子的可行方法。在本文中,我们使用协变光前夸克模型(CLFQM)来研究半轻子衰变 $D^*_{(s)}toPell^{+}nu_{ell}$ 和非轻子衰变 $D^*_{(s)}to PP、PV$,其中$P=pi, K, eta^{(prime)}, V=rho,K^*,phi$和$ell=e,mu$,它们的范围都在$10^{-13}/sim 10^{-6}$之内。在这些衰变中,$D_{s}^{*+}toeta ell^{+}nu_{ell}$ 和$D^{*+}_{s}to etarho^{+}$ 信道的分支比最大,可达 10^{-6}$ 级。这些衰变最有可能在未来的高亮度实验中出现。我们可以发现,分支比$mathcal{B}r(D_{s}^{*+}toeta ell^{+}nu_{ell})=1.46 (times10^{-6}$)和$mathcal{B}r(D_{s}^{*+}toeta rho^{+})=1.04(times10^{-6}$对应于在STCF、CEPC和FCC-ee等$e^+e^-$对撞机实验中的数万个事件,以及在HL-LHC中的数千万个事件。总之,在未来的实验中研究$D^*_{(s)}$介子弱衰变是可行的。此外,我们还预测并讨论了另外两个物理观测值,即我们所考虑的衰变的纵向极化分数$f_{L}$和正向-反向不对称度$A_{FB}$。
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引用次数: 0
CP violation at finite temperature 有限温度下的 CP 违约
Pub Date : 2024-09-11 DOI: arxiv-2409.07180
Károly Seller, Zsolt Szép, Zoltán Trócsányi
We present a comprehensive study of the finite temperature CP-asymmetryfactor needed in the semi-classical treatment of leptogenesis originating fromMajorana fermion decays into a lepton and a scalar particle. The imaginary partof the relevant one-loop integrals are evaluated using both the real time andthe imaginary time formalisms of thermal quantum field theory. In the former weconsider the retarded-advanced approach as well as the original thermal cuttingmethod developed by Kobes and Semenoff. Specific care is directed towardsshowing the consistency between the various approaches. We show that the finalphysical result of the calculation is linear in the statistical factors and isconsistent with what is obtained in the Kadanoff-Baym approach. We also presentanalytic expressions for the full CP-asymmetry factor in the form ofwell-behaved triple-integrals, and provide numerical benchmark predictions in aspecific particle physics model.
我们介绍了对源自马约拉纳费米子衰变成轻子和标量粒子的轻子发生的半经典处理中所需的有限温度CP不对称因子的全面研究。我们使用热量子场论的实时间和虚时间形式来评估相关一环积分的虚部。在前者中,我们考虑了延迟-高级方法以及由 Kobes 和 Semenoff 发展的原始热切割方法。我们特别注意显示各种方法之间的一致性。我们证明,计算的最终物理结果与统计因子呈线性关系,并且与卡达诺夫-贝姆方法的结果一致。我们还提出了完整 CP 不对称因子的解析表达式,其形式为完备的三重积分,并提供了特定粒子物理模型中的数值基准预测。
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引用次数: 0
Detect anomalous quartic gauge couplings at muon colliders with quantum kernel k-means 在μ介子对撞机上利用量子核K均值检测反常四元规耦合
Pub Date : 2024-09-11 DOI: arxiv-2409.07010
Shuai Zhang, Ke-Xin Chen, Ji-Chong Yang
In recent years, with the increasing luminosities of colliders, handling thegrowing amount of data has become a major challenge for future New Physics~(NP)phenomenological research. To improve efficiency, machine learning algorithmshave been introduced into the field of high-energy physics. As a machinelearning algorithm, kernel k-means has been demonstrated to be useful forsearching NP signals. It is well known that the kernel k-means algorithm can becarried out with the help of quantum computing, which suggests that quantumkernel k-means~(QKKM) is also a potential tool for NP phenomenological studiesin the future. This paper investigates how to search for NP signals using thek-means anomaly detection event selection strategy with quantum kernels. Takingthe $mu^+mu^-to vbar{v}gammagamma$ process at a muon collider as anexample, the dimension-8 operators contributing to anomalous quartic gaugecouplings~(aQGCs) are studied. The expected coefficient constraints obtainedusing the QKKM of three different forms of quantum kernels and k-meansalgorithm are presented, it can be shown that QKKM can help to find the signalof aQGCs.
近年来,随着对撞机光度的不断提高,处理日益增长的数据量已成为未来新物理现象研究的一大挑战。为了提高效率,机器学习算法被引入高能物理领域。作为一种机器学习算法,核 k-means 已被证明可用于搜索 NP 信号。众所周知,核仁 k-means 算法可以在量子计算的帮助下实现,这表明量子核仁 k-means~ (QKKM)也是未来 NP 现象学研究的潜在工具。本文研究了如何利用量子核的k均值异常检测事件选择策略来搜索NP信号。以μ介子对撞机上的$mu^+mu^-to vbar{v}gammagamma$ 过程为例,研究了贡献于反常四元规耦合~(aQGCs)的8维算子。研究给出了利用三种不同形式量子核的QKKM和k-means算法得到的预期系数约束,表明QKKM有助于发现aQGCs的信号。
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引用次数: 0
Wigner rotations for cascade reactions 级联反应的维格纳旋转
Pub Date : 2024-09-10 DOI: arxiv-2409.06913
Kai Habermann, Mikhail Mikhasenko
Cascade parameterization of hadronic reactions is a central tool in hadronspectroscopy for modeling matrix elements and extracting parameters of hadronicstates. Implementing the helicity formalism consistently presents challenges,particularly for particles with spin, due to the need for matching spin statesof final-state particles, known as the Wigner rotations. This paper discussesthese challenges in detail and offers solutions, including a practical methodfor implementation. Equipped with a general algorithm for computing Wignerrotations, we extend the studies to alternative amplitude formulations, theminus-phi and canonical conventions.
强子反应的级联参数化是强子谱学的核心工具,用于建立矩阵元素模型和提取强子态参数。由于需要匹配终态粒子的自旋态(即维格纳旋转),因此螺旋形式主义的实施始终面临挑战,特别是对于具有自旋的粒子。本文详细讨论了这些挑战并提供了解决方案,包括一种实用的实现方法。借助计算维格纳旋转的通用算法,我们将研究扩展到其他振幅公式、inus-phi 和卡农惯例。
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引用次数: 0
Dual Gravitational Wave Signatures of Instant Preheating 瞬间预热的双重引力波信号
Pub Date : 2024-09-10 DOI: arxiv-2409.06483
Wei-Yu Hu, Kazunori Nakayama, Volodymyr Takhistov, Yong Tang
In the instant preheating scenario efficient particle production occursimmediately following the period of inflationary expansion in the earlyUniverse. We demonstrate that instant preheating predicts unique gravitationalwave (GW) signals arising from two distinct origins. One source is thebremsstrahlung GWs produced through the decay of superheavy particles, aninevitable consequence of instant preheating. The other is GWs generated fromthe nonlinear dynamics of the inflaton and coupled scalar fields. Usingnumerical simulations, we show that the peak of the GW spectrum shiftsdepending on the coupling constants of the theory. The detection of these dualGW signatures, characteristic of instant preheating, provides novelopportunities for probing the dynamics of the early Universe.
在瞬时预热假设中,高效粒子的产生紧随早期宇宙的膨胀扩张期之后。我们证明,瞬时预热预言了来自两个不同来源的独特引力波(GW)信号。一个来源是超重粒子衰变产生的轫致辐射引力波,这是瞬时预热的必然结果。另一种是由流入子和耦合标量场的非线性动力学产生的巨波。通过数值模拟,我们发现 GW 谱的峰值会随着理论耦合常数的变化而变化。探测这些具有瞬时预热特征的双GW信号,为探测早期宇宙的动力学提供了新的机会。
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引用次数: 0
Malaphoric $Z'$ models for $b rightarrow s ell^+ ell^-$ anomalies 用于 $b rightarrow s ell^+ ell^-$ 异常现象的拟合 $Z'$ 模型
Pub Date : 2024-09-10 DOI: arxiv-2409.06804
Ben Allanach, Nico Gubernari
We study some phenomenological effects of kinetic mixing between thehypercharge field and a new $U(1)$ gauge field in specific $Z^prime$ modelsthat ameliorate the tensions between measurements and Standard Modelpredictions in $b rightarrow sell^+ ell^-$ decays. To this end, we rederivethe dimension-6 SMEFT coefficients resulting from integrating out thekinetically-mixed (`malaphoric') $Z^prime$ field. The kinetic mixing providesa family-universal component to the couplings of the $Z^prime$ field, whichcan improve fits to lepton flavour universality observables. We show howkinetic mixing improves the best fit of the $B_3-L_2$ model to $brightarrow s$data by 7.3 units of $chi^2$ while remaining compatible with other relevantdata sets such as electroweak precision observables and measurements of $e^+e^- rightarrow ell^+ ell^-$ at LEP2.
我们研究了在特定的$Z^prime$模型中超电荷场和新的$U(1)$规量场之间的动力学混合的一些现象学效应,这些效应改善了在$b rightarrow sell^+ ell^-$ 衰变中测量和标准模型预测之间的紧张关系。为此,我们重新解读了对动力学混合("隐喻")$Z^prime$场进行积分后得到的六维度SMEFT系数。动力学混合为$Z^prime$场的耦合提供了一个族普遍性成分,它可以改善对轻子味道普遍性观测值的拟合。我们展示了动力学混合如何将$B_3-L_2$模型与$brightarrow s$数据的最佳拟合提高了7.3个单位的$chi^2$,同时与其他相关数据集保持兼容,如电弱精密观测数据和在LEP2测量的$e^+e^- rightarrow ell^+ ell^-$ 。
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引用次数: 0
Exploring the nature of $Y(4230)$ and $Y(4360)$ in B decays 探索B衰变中$Y(4230)$和$Y(4360)$的性质
Pub Date : 2024-09-10 DOI: arxiv-2409.06539
Ming-Zhu Liu, Qi Wu
The vector charmonium states can be directly produced at the $e^+e^{-}$annihilation process. Among them, $Y(4230)$ and $Y(4360)$ splitting from thepreviously discovered $Y(4260)$ are not easily arranged into the conventionalcharmonium spectrum, while the recent studies indicated that they have strongcouplings to $Dbar{D}_1$ and $D^*bar{D}_1$. In this work, we investigate theproductions of $Y(4230)$ and $Y(4360)$ as the heavy quark spin symmetry doublethadronic molecules of $Dbar{D}_1$ and $D^*bar{D}_1$ in $B$ decays via thetriangle diagram mechanism. In particular, we propose that the decay constantsof $Y(4230)$ and $Y(4360)$ extracted in $B$ decays are helpful to clarify theirnature.
矢量粲态可以在$e^+e^{-}$反湮灭过程中直接产生。其中,从以前发现的$Y(4260)$分裂出来的$Y(4230)$和$Y(4360)$不容易排列到常规的粲谱中,而最近的研究表明它们与$D^*bar{D}_1$和$D^*bar{D}_1$有强耦合。在这项工作中,我们研究了$Y(4230)$和$Y(4360)$作为$Dbar{D}_1$和$D^*bar{D}_1$的重夸克自旋对称双重子分子在$B$衰变中通过三角图机制产生的情况。我们特别提出,在$B$衰变中提取的$Y(4230)$和$Y(4360)$的衰变常数有助于澄清它们的性质。
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引用次数: 0
期刊
arXiv - PHYS - High Energy Physics - Phenomenology
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