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Weak expansion properties and a large deviation principle for coarse expanding conformal systems 粗膨胀保形系统的弱膨胀特性和大偏差原理
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07305
Li, Zhiqiang, Zheng, Hanyun
In this paper, we prove that for a metric coarse expanding conformal system $f:(mathfrak{X}_1,X)rightarrow (mathfrak{X}_0,X)$ with repellor $X$, the map $f|_X:Xrightarrow X$ is asymptotically $h$-expansive. Moreover, we show that $f|_X$ is not $h$-expansive if there exists at least one branch point in the repellor. As a consequence of asymptotic $h$-expansiveness, for $f|_X$ and each real-valued continuous potential on $X$, there exists at least one equilibrium state. For such maps, if some additional assumptions are satisfied, we can furthermore establish a level-2 large deviation principle for iterated preimages, followed by an equidistribution result.
本文证明了对于一个度量粗展开共形系统$f:(mathfrak{X}_1,X)rightarrow (mathfrak{X}_0,X)$与邻域$X$,映射$f|_X:Xrightarrow X$是渐近$h$-可扩的。此外,我们证明了$f|_X$不是$h$-膨胀的,如果在驱避器中存在至少一个分支点。由于渐近的$h$-扩张性,对于$f|_X$和$X$上的每个实值连续势,存在至少一个平衡状态。对于这类映射,如果满足一些附加的假设,我们可以进一步建立迭代预像的二级大偏差原理,从而得到一个等分布结果。
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引用次数: 0
HESS J1809-193: Gamma-Ray Emission by Cosmic Rays from Past Explosion HESS J1809-193:由过去爆炸的宇宙射线发射的伽马射线
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07481
Boxi, Sovan, Gupta, Nayantara
The very high energy gamma-ray source HESS J1809-193 has been detected by the LHAASO and HAWC observatory beyond 100 TeV energy. It is an interesting candidate for exploring the underlying mechanisms of gamma-ray production due to the presence of supernova remnants, pulsar and molecular clouds close to it. We have considered the injection of the energetic cosmic rays from a past explosion, whose reminiscent may be SNR G011.0-00.0, which is located within the extended gamma-ray source HESS J1809-193. We explain the multi-wavelength data from the region of HESS J1809-193 with synchrotron, inverse Compton, bremsstrahlung emission of cosmic ray electrons and secondary gamma-ray production in interactions of cosmic ray protons with the cold protons in the local molecular clouds within a time-dependent framework including the diffusion loss of cosmic rays. The observational data has been modelled with the secondary photons produced by the time-evolved cosmic ray spectrum, assuming the age of the explosion is 4500 years.
高能伽玛射线源HESS J1809-193已经被LHAASO和HAWC天文台探测到,能量超过100 TeV。由于超新星残骸、脉冲星和分子云的存在,它是探索伽马射线产生的潜在机制的一个有趣的候选者。我们考虑了从过去的一次爆炸中注入的高能宇宙射线,它的信噪比可能是G011.0-00.0,它位于扩展的伽马射线源HESS J1809-193内。我们用同步加速器、逆康普顿、宇宙射线电子的轫致辐射和宇宙射线质子与局部分子云中的冷质子相互作用产生的二次伽马射线,在包括宇宙射线扩散损失在内的时间依赖框架内解释了来自HESS J1809-193区域的多波长数据。观测数据是用随时间演化的宇宙射线光谱产生的二次光子建模的,假设爆炸的年龄是4500年。
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引用次数: 0
Temporal Performance Prediction for Deep Convolutional Long Short-Term Memory Networks 深度卷积长短期记忆网络的时间性能预测
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07477
Fieback, Laura, Dash, Bidya, Spiegelberg, Jakob, Gottschalk, Hanno
Quantifying predictive uncertainty of deep semantic segmentation networks is essential in safety-critical tasks. In applications like autonomous driving, where video data is available, convolutional long short-term memory networks are capable of not only providing semantic segmentations but also predicting the segmentations of the next timesteps. These models use cell states to broadcast information from previous data by taking a time series of inputs to predict one or even further steps into the future. We present a temporal postprocessing method which estimates the prediction performance of convolutional long short-term memory networks by either predicting the intersection over union of predicted and ground truth segments or classifying between intersection over union being equal to zero or greater than zero. To this end, we create temporal cell state-based input metrics per segment and investigate different models for the estimation of the predictive quality based on these metrics. We further study the influence of the number of considered cell states for the proposed metrics.
量化深度语义分割网络的预测不确定性在安全关键任务中至关重要。在自动驾驶等视频数据可用的应用中,卷积长短期记忆网络不仅能够提供语义分割,还能够预测下一个时间步长的分割。这些模型使用单元状态,通过输入时间序列来预测未来的一步甚至一步,从而从以前的数据中传播信息。我们提出了一种时间后处理方法,通过预测预测段和真实段的交集并集或交集并集等于零或大于零之间的分类来估计卷积长短期记忆网络的预测性能。为此,我们为每个片段创建基于时间单元状态的输入指标,并研究基于这些指标的预测质量估计的不同模型。我们进一步研究了考虑的细胞状态的数量对所提出的度量的影响。
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引用次数: 0
Are We Falling in a Middle-Intelligence Trap? An Analysis and Mitigation of the Reversal Curse 我们是否陷入了中等智力的陷阱?逆转咒的分析与缓解
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07468
Lv, Ang, Zhang, Kaiyi, Xie, Shufang, Tu, Quan, Chen, Yuhan, Wen, Ji-Rong, Yan, Rui
Recent studies have highlighted a phenomenon in large language models (LLMs) known as "the reversal curse," in which the order of knowledge entities in the training data biases the models' comprehension. For example, if a model is trained on sentences where entity A consistently appears before entity B, it can respond to queries about A by providing B. However, it may encounter confusion when presented with questions concerning B. We contend that the reversal curse is partially a result of specific model training objectives, particularly evident in the prevalent use of the next-token prediction within most causal language models. For the next-token prediction, models solely focus on a token's preceding context, resulting in a restricted comprehension of the input. In contrast, we illustrate that the GLM, trained using the autoregressive blank infilling objective where tokens to be predicted have access to the entire context, exhibits better resilience against the reversal curse. We propose a novel training method, BIdirectional Casual language modeling Optimization (BICO), designed to mitigate the reversal curse when fine-tuning pretrained causal language models on new data. BICO modifies the causal attention mechanism to function bidirectionally and employs a mask denoising optimization. In the task designed to assess the reversal curse, our approach improves Llama's accuracy from the original 0% to around 70%. We hope that more attention can be focused on exploring and addressing these inherent weaknesses of the current LLMs, in order to achieve a higher level of intelligence.
最近的研究强调了大型语言模型(llm)中的一种被称为“逆转诅咒”的现象,即训练数据中知识实体的顺序会影响模型的理解。例如,如果一个模型在实体a始终出现在实体B之前的句子上进行训练,它可以通过提供B来响应关于a的查询。然而,当出现关于B的问题时,它可能会遇到困惑。我们认为,逆转诅咒部分是特定模型训练目标的结果,特别是在大多数因果语言模型中普遍使用下一个令牌预测。对于下一个令牌预测,模型只关注令牌的前一个上下文,导致对输入的理解受到限制。相比之下,我们说明了使用自回归空白填充目标训练的GLM,其中待预测的令牌可以访问整个上下文,对逆转诅咒表现出更好的弹性。我们提出了一种新的训练方法,双向因果语言建模优化(BICO),旨在减轻在新数据上微调预训练因果语言模型时的逆转诅咒。BICO将因果注意机制修改为双向作用,并采用掩模去噪优化。在评估逆转诅咒的任务中,我们的方法将羊驼的准确率从原来的0%提高到70%左右。我们希望更多的关注可以集中在探索和解决当前法学硕士的这些固有弱点上,以达到更高的智能水平。
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引用次数: 1
Finding and Editing Multi-Modal Neurons in Pre-Trained Transformer 在预训练变压器中寻找和编辑多模态神经元
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07470
Pan, Haowen, Cao, Yixin, Wang, Xiaozhi, Yang, Xun
Multi-modal large language models (LLM) have achieved powerful capabilities for visual semantic understanding in recent years. However, little is known about how LLMs comprehend visual information and interpret different modalities of features. In this paper, we propose a new method for identifying multi-modal neurons in transformer-based multi-modal LLMs. Through a series of experiments, We highlight three critical properties of multi-modal neurons by four well-designed quantitative evaluation metrics. Furthermore, we introduce a knowledge editing method based on the identified multi-modal neurons, for modifying a specific token to another designative token. We hope our findings can inspire further explanatory researches on understanding mechanisms of multi-modal LLMs.
近年来,多模态大语言模型(LLM)在视觉语义理解方面获得了强大的能力。然而,对于llm如何理解视觉信息和解释不同的特征模态,人们知之甚少。在本文中,我们提出了一种新的方法来识别基于变压器的多模态llm中的多模态神经元。通过一系列实验,我们通过四个精心设计的定量评价指标突出了多模态神经元的三个关键特性。此外,我们引入了一种基于已识别的多模态神经元的知识编辑方法,将一个特定的标记修改为另一个指示标记。我们希望我们的发现能够启发更多的解释性研究来理解多模态llm的机制。
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引用次数: 0
Goldberger-Treiman relation and Wu-type experiment in the decuplet sector 双扇区的Goldberger-Treiman关系和wu型实验
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07471
Bertilsson, Magnus, Leupold, Stefan
The leading-order chiral Lagrangian for the baryon octet and decuplet states coupled to Goldstone bosons and external sources contains six low-energy constants. Five of them are fairly well known from phenomenology, but the sixth one is practically unknown. This coupling constant provides the strength of the (p-wave) coupling of Goldstone bosons to decuplet states. Its size and even sign are under debate. Quark model and QCD for a large number of colors provide predictions, but some recent phenomenological analyses suggest even an opposite sign for the Delta-pion coupling. The Goldberger-Treiman relation connects this coupling constant to the axial charge of the Delta baryon. This suggests a Wu-type experiment to determine the unknown low-energy constant. While this is not feasible in the Delta sector because of the large hadronic width of the Delta, there is a flavor symmetry related process that is accessible: the weak semileptonic decay of the Omega baryon to a spin 3/2 cascade baryon. A broad research program is suggested that can pin down at least the rough size and the sign of the last unknown low-energy constant of the leading-order Lagrangian. It encompasses experimental measurements, in particular the forward-backward asymmetry of the semileptonic decay, together with a determination of the quark-mass dependences using lattice QCD for the narrow decuplet states and chiral perturbation theory to extrapolate to the Delta sector. Besides discussing the strategy of the research program, the present work provides a feasibility check based on a simple leading-order calculation.
与戈德斯通玻色子和外部源耦合的重子八重态和十重态的首阶手性拉格朗日量包含6个低能常数。其中的五个在现象学中是相当知名的,但第六个实际上是未知的。这个耦合常数提供了戈德斯通玻色子到十重态的(p波)耦合强度。它的大小和符号都在争论中。夸克模型和大量颜色的QCD提供了预测,但最近的一些现象学分析甚至对德尔塔-介子耦合提出了相反的迹象。Goldberger-Treiman关系将这个耦合常数与δ重子的轴向电荷联系起来。建议采用wu型实验来确定未知的低能常数。虽然这在三角洲扇区是不可行的,因为三角洲的强子宽度很大,但有一种与风味对称相关的过程是可行的:欧米伽重子的弱半光子衰变为自旋3/2级联重子。提出了一个广泛的研究计划,至少可以确定阶拉格朗日的最后一个未知低能常数的大致大小和符号。它包括实验测量,特别是半光子衰变的前后不对称性,以及使用窄十重态的晶格QCD和手性微扰理论外推到Delta扇区的夸克-质量依赖性的确定。本工作除了讨论研究方案的策略外,还提供了基于简单的超前计算的可行性检验。
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引用次数: 0
The apparent tidal decay of WASP-4 b can be explained by the R{o}mer effect wasp - 4b的明显潮汐衰减可以用R{o}mer效应来解释
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07098
Harre, Jan-Vincent, Smith, Alexis M. S.
Tidal orbital decay plays a vital role in the evolution of hot Jupiter systems. As of now, this was only observationally confirmed for the WASP-12 system. There are a few other candidates, including WASP-4 b, but no conclusive result could be obtained for these systems as of yet. In this study, we present an analysis of new TESS data of WASP-4 b together with archival data, taking the light-time effect (LTE), induced by the second planetary companion, into account as well. We make use of three different Markov-Chain-Monte-Carlo models; a circular orbit with a constant orbital period, a circular orbit with a decaying orbit, and an elliptical orbit with apsidal precession. This analysis is repeated for four cases. The first case features no LTE correction, with the remaining three cases featuring three different timing correction approaches. Comparison of these models yields no conclusive answer to the cause of WASP-4,b's apparent transit timing variations. A broad range of values of the orbital decay and apsidal precession parameters are possible, depending on the LTE correction. This work highlights the importance of continued photometric and spectroscopic monitoring of hot Jupiters.
潮汐轨道衰变在热木星系统的演化中起着至关重要的作用。到目前为止,这只在WASP-12系统中得到了观测证实。还有一些其他的候选者,包括wasp - 4b,但到目前为止还没有关于这些系统的结论性结果。在这项研究中,我们对WASP-4 b的新TESS数据和档案数据进行了分析,并考虑了第二颗行星伴星引起的光时效应(LTE)。我们使用了三种不同的马尔可夫链-蒙特卡罗模型;具有恒定轨道周期的圆形轨道,具有衰减轨道的圆形轨道,以及具有侧进动的椭圆轨道。对四个案例进行了重复分析。第一种情况没有LTE校正,其余三种情况采用三种不同的定时校正方法。这些模型的比较并没有得出WASP-4,b的明显凌日时间变化的决定性答案。轨道衰减和附加进动参数的取值范围很广,这取决于LTE的校正。这项工作强调了继续对热木星进行光度和光谱监测的重要性。
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引用次数: 0
Collaborative Goal Tracking of Multiple Mobile Robots Based on Geometric Graph Neural Network 基于几何图神经网络的多移动机器人协同目标跟踪
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07105
Lin, Qingquan, Lu, Weining
Multi-robot systems are widely used in spatially distributed tasks, and their collaborative path planning is of great significance for working efficiency. Currently, different multi-robot collaborative path planning methods have been proposed, but how to process the sensory information of neighboring robots at different locations from a local perception perspective in real environment to make better decisions is still a major difficulty. To address this problem, this paper proposes a multi-robot collaborative path planning method based on geometric graph neural network (GeoGNN). GeoGNN introduces the relative position information of neighboring robots into each interaction layer of the graph neural network to better integrate neighbor sensing information. An expert data generation method is designed for the robot to advance in a single step, by which expert data are generated in ROS to train the network. Experimental results show that the accuracy of the proposed method is improved by about 5% compared to the model based only on CNN on the expert data set. In ROS simulation environment path planning test, the success rate is improved by about 4% compared to CNN and flowtime increase is reduced about 8%, which outperforms other graph neural network models.
多机器人系统广泛应用于空间分布式任务,其协同路径规划对提高工作效率具有重要意义。目前,已经提出了不同的多机器人协同路径规划方法,但如何在真实环境中从局部感知的角度处理不同位置相邻机器人的感知信息以做出更好的决策仍然是一个主要难点。针对这一问题,提出了一种基于几何图神经网络(GeoGNN)的多机器人协同路径规划方法。GeoGNN将相邻机器人的相对位置信息引入到图神经网络的每个交互层中,以更好地整合相邻感知信息。设计了一种单步推进的专家数据生成方法,通过在ROS中生成专家数据对网络进行训练。实验结果表明,与专家数据集上仅基于CNN的模型相比,该方法的准确率提高了约5%。在ROS仿真环境下的路径规划测试中,与CNN相比,成功率提高了约4%,流时间增加减少了约8%,优于其他图神经网络模型。
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引用次数: 0
Secure Wireless Communication via Movable-Antenna Array 移动天线阵列的安全无线通信
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07104
Hu, Guojie, Wu, Qingqing, Xu, Kui, Si, Jiangbo, Al-Dhahir, Naofal
Movable antenna (MA) array is a novel technology recently developed where positions of transmit/receive antennas can be flexibly adjusted in the specified region to reconfigure the wireless channel and achieve a higher capacity. In this letter, we, for the first time, investigate the MA array-assisted physical-layer security where the confidential information is transmitted from a MA array-enabled Alice to a single-antenna Bob, in the presence of multiple single-antenna and colluding eavesdroppers. We aim to maximize the achievable secrecy rate by jointly designing the transmit beamforming and positions of all antennas at Alice subject to the transmit power budget and specified regions for positions of all transmit antennas. The resulting problem is highly non-convex, for which the projected gradient ascent (PGA) and the alternating optimization methods are utilized to obtain a high-quality suboptimal solution. Simulation results demonstrate that since the additional spatial degree of freedom (DoF) can be fully exploited, the MA array significantly enhances the secrecy rate compared to the conventional fixed-position antenna (FPA) array.
可移动天线阵列是近年来发展起来的一种新技术,它可以在指定区域内灵活地调整发射/接收天线的位置,从而重新配置无线信道,实现更高的容量。在这封信中,我们首次研究了MA阵列辅助的物理层安全,在多个单天线和串通窃听者存在的情况下,机密信息从启用MA阵列的Alice传输到单天线Bob。我们的目标是根据发射功率预算和所有发射天线位置的指定区域,共同设计发射波束形成和所有发射天线在Alice的位置,以最大限度地提高可实现的保密率。所得到的问题是高度非凸的,利用投影梯度上升(PGA)和交替优化方法来获得高质量的次优解。仿真结果表明,由于可以充分利用附加的空间自由度(DoF),与传统的固定位置天线(FPA)阵列相比,MA阵列显著提高了保密率。
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引用次数: 0
Robust Probabilistic Prediction for Stochastic Dynamical Systems 随机动力系统的鲁棒概率预测
Pub Date : 2023-11-13 DOI: 10.48550/arxiv.2311.07108
Xu, Tao, He, Jianping
It is critical and challenging to design robust predictors for stochastic dynamical systems (SDSs) with uncertainty quantification (UQ) in the prediction. Specifically, robustness guarantees the worst-case performance when the predictor's information set of the system is inadequate, and UQ characterizes how confident the predictor is about the predictions. However, it is difficult for traditional robust predictors to provide robust UQ because they were designed to robustify the performance of point predictions. In this paper, we investigate how to robustify the probabilistic prediction for SDS, which can inherently provide robust distributional UQ. To characterize the performance of probabilistic predictors, we generalize the concept of likelihood function to likelihood functional, and prove that this metric is a proper scoring rule. Based on this metric, we propose a framework to quantify when the predictor is robust and analyze how the information set affects the robustness. Our framework makes it possible to design robust probabilistic predictors by solving functional optimization problems concerning different information sets. In particular, we design a class of moment-based optimal robust probabilistic predictors and provide a practical Kalman-filter-based algorithm for implementation. Extensive numerical simulations are provided to elaborate on our results.
设计具有不确定性量化的随机动力系统的鲁棒预测器是一项重要而具有挑战性的工作。具体来说,当预测者的系统信息集不充分时,鲁棒性保证了最坏情况下的性能,而UQ表征了预测者对预测的自信程度。然而,传统的鲁棒预测器很难提供鲁棒的UQ,因为它们的设计是为了鲁棒点预测的性能。在本文中,我们研究了如何对SDS的概率预测进行鲁棒化,它可以提供固有的鲁棒性分布UQ。为了表征概率预测器的性能,我们将似然函数的概念推广到似然泛函,并证明了该度量是一个合适的评分规则。基于这个度量,我们提出了一个框架来量化预测器何时是鲁棒性的,并分析信息集如何影响鲁棒性。我们的框架使得通过解决涉及不同信息集的函数优化问题来设计稳健的概率预测器成为可能。特别地,我们设计了一类基于矩的最优鲁棒概率预测器,并提供了一个实用的基于卡尔曼滤波的算法来实现。提供了大量的数值模拟来详细说明我们的结果。
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引用次数: 0
期刊
arXiv (Cornell University)
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