DUKE

Mohd Hezri Amir, Albert Quek, Nur Rasyid Bin Sulaiman, John See
{"title":"DUKE","authors":"Mohd Hezri Amir, Albert Quek, Nur Rasyid Bin Sulaiman, John See","doi":"10.1145/3001773.3001804","DOIUrl":null,"url":null,"abstract":"We calculated the thresholds for charged–current electron neutrino and antineutrino interactions for most of the stable isotopes. Looking at the isotopes with the lowest thresholds, we found that 181 Ta and 160 Gd are reasonable candidates for low–threshold neutrino detectors, with thresholds at 0 . 188 MeV and 0 . 105 MeV respectively. These materials are both metals, have relatively high natural abundance, and are not frequently found in conjunction with radioactive substances, making them potentially viable for this task. Using the SNOwGLoBES software library, we computed estimated cross sections and event rates for supernova fluxes in these two materials. When neutron stars in a low mass x-ray binary system collect matter from their H or He rich companion star, nuclear burning can occur on the high temperature and pressure surface. If a critical accretion rate is reached, it can cause the nuclear reactions to run away, resulting in an X-Ray Burst (XRB). By studying the sensitivity of XRB models to different nuclear reactions, we can help identify which are most important in the burst process. The stellar model used for this study was of an XRB in Modules for Experiments with Stellar Astrophysics (MESA) with a co-processed nuclear network. A single stellar model was rerun once for each nuclear reaction and its inverse in the network, varying its reaction rate by 100. The models with the greatest change indicate reactions that are key to XRB nucleosynthesis. Preliminary results identified 5 significant nuclear reactions. While the study is in its preliminary stage, it has proved capable of highlighting reactions that significantly affect XRB properties. Λ 0 hyperons can be produced from hadronization of a struck quark in Semi-Inclusive Deep In- elastic Scattering (SIDIS). This process is of interest because the Λ 0 hyperon polarization may be inferred from its self-analyzing weak decay. Such probes allow one to extract information about the polarization of the constituent quarks within the proton and provide a test of fundamental aspects of Quantum Chromodynamics (QCD). In this study, we generated SIDIS events using a Lund Monte Carlo and simulated the response of the CLAS12 detector at Jefferson Lab’s Continuous Electron Beam Accelerator Facility (CEBAF)using GEANT4 with different toroidal magnet field strengths and configurations (either inbending or outbending). We then processed events using the CLAS12 reconstruction framework to find the optimal configuration and maximize our reconstruction efficiency from the Λ 0 → π − + p + decay channel. For Λ 0 hyperons coming from a struck quark ( x F > 0 ), we obtained our best reconstruction efficiency in the low field outbending toroidal configuration. Nuclear data for photo-nuclear reactions is scarce. By using the activation technique, ( γ,n ) cross sections can be measured to a high precision. 169 Tm( n, 2 n ) is a common neutron monitor reaction, but there is no available data on its photo-nuclear counterpart, the 169 Tm( γ,n ) reaction. Measurement of this reaction would allow use of thulium as a standard γ -ray monitor. Thulium, tin, and gold samples were irradiated by monoenergetic γ rays provided by the High Intensity γ -ray Source (HI γ S), located at Duke University. The resulting activity was quantified using γ -ray spectroscopy with high purity germanium (HPGe) detectors. The data confirmed the literature half-lives of 196 Au, 123 m Sn, and 168 Tm as 6.16 d, 40.1 m, and 93.1 d, respectively. Cross sections were extracted for the 124 Sn( γ,n ) 123 m Sn and 169 Tm( γ,n ) 168 Tm reactions, representing the first measurements of these reactions. Tritium, a radioactive isotope of hydrogen, will be the basis of experiment P-02-13 at HI γ S. This study will utilize a tritium gas target to obtain cross-section measurements of two-and three-body photodisintegration of the triton in order to further understand nuclear structure and reactions, specifically three-nucleon interactions. In order to reduce loss of the radioactive gas, safety systems will be implemented including a tritium scrubber system. This system will work in conjunction with a copper-zinc catalyst in order to utilize the reduction of copper to continuously transform elemental tritium into T 2 O or HTO, allowing the tritiated water to be collected within a molecular sieve and safely disposed of. Reactions catalyzed by the CuZn bed were examined using a Residual Gas Analyzer at temperatures of 23 ◦ C to 200 ◦ C to measure isotope concentrations and compositions of the various gas streams that will flow through the scrubbing system during normal operation. Low-mass nuclear Compton scattering projects at HI γ S are focused on determining experimentally the static electric ( α E ) and magnetic ( β M ) dipole polarizabilities of neutrons. Building on past experiments, the next iteration will use a liquid 3 He target volume to offer a new nuclear structure for analysis. This project is centered around preparing for the upcoming experiments. A new epoxy-lined gas storage tank was commissioned and sealed for the 3 He gas containment system. Leakage rates were measured, and a residual gas analysis was performed. The sealed tank was shown to have a leak rate of < 2 . 0 × 10 7 mbar*L/sec and main contamination from water, nitrogen, and oxygen at levels that can be removed by internal systems. A computational model was constructed based on particle beam flux attenuation in scattering processes. Values of the contaminate 4 He level C 4 (along with the percentage uncertainty in this value p ( C 4 ) ), the percentage uncertainty in the cross section of the experimental scattering with 4 He p ( σ 4 ) , and the experimental runtime T were varied to determine impact on the percentage uncertainty in the scattering cross section with 3 He. Optimal values (against cost) of T and p ( σ 4 ) were found to be 200h and 10% respectively for C 4 less than 10% and p ( C 4 ) less than 25%. When a proton is placed into an external magnetic field, it will attempt to align its magnetic moment to that field. Then if that external magnetic field is suddenly turned off, the proton will start to precess around the only other magnetic field available, the Earth’s. The goal of this project was to get an instrument operational that would take advantage of this concept. It would be used to find the spin relaxation time ( T 2 ), a measure of the magnetic field gradients, of the sample. This would then be used to test the magnetization of other materials for a larger project. An Earth’s field nuclear magnetic resonance control box and sample coil were used along with a sample of water (our proton source) to produce a waveform from the precession of the water molecules. From that waveform we were able to calculate our T 2 value. After many setbacks and multiple trials, we were successful in operating the instrument to produce waveforms in the correct shape and scale, thus getting a T 2 value that was close to the established value. While more testing and calibration is still needed, the instrument is now working and can be used in future testing of the magnetization of materials. We are developing a pulsed and tunable Pelletron accelerator to provide measurements of bremsstrahlung energy loss for next generation neutron beta decay experiments. The development of our Pelletron system is the first step before any measurements are made. The goals of our project are to improve the performance of an N 2 purge and implement a suppressor electrode to reduce arcing, understand possible sources of coronal discharge loss, make a first detection of the electron beam, and develop a test beam line. These first steps were successful, greatly reducing charge loss and arcing, and confirming the production of over 250 keV electron beams. If the Higgs Boson is made of new constituent particles, it is likely that the top quark is also made of similar particles based on how strongly they couple. In this case, events with four top quarks would be produced in excess of predictions from current theories. The purpose of this project is to study top quark kinematics to determine how to distinguish between background and signal top decays based on top quark transverse momentum. We used MADGRAPH to generate Monte Carlo events where t and ¯ t decay to a bottom quark and a W boson, and the W bosons decay to q ¯ q . Our analysis shows that as the top quark’s transverse momentum increases, the distance between the top quark and its decays in the η − φ space decreases, where η is the pseudo-rapidity and φ is the azimuthal angle. This decrease in distance in the η − φ space as top transverse momentum increases demonstrates that the two high momentum tops in a four top process can be tagged primarily by using position. Searches for c ¯ c from Higgs/ Z decays have been done exclusively for the ground J/ψ state using leptonic decay modes. This project aims to tag excited c ¯ c states via hadronic decay modes. The study of c ¯ c is relevant to Higgs coupling with the charm quark. Excited energy states such as ψ (2 S ) and χ c 0 ,c 1 ,c 2 are of interest as we can follow their decays into J/ψ γ . Excited states of c ¯ c are produced via the standard Higgs/ Z production chain gg → H which creates c ¯ c by H → c ¯ cγ . The purpose of creating this tagging algorithm is to apply it to ATLAS data. The tagging is done using machine learning. Training data for the machine learning algorithm comes from Monte Carlo simulations of particle decays and simulations of interactions in ATLAS. Other Monte Carlo simulations are being tested to verify the stability of the algorithm. The accuracy for the fully-connected neural network trained on J/ψ , ψ (2 S ) , and quark/gluon background is 93%. This novel approach to c ¯ c tagging resulted in a production-ready tagger. Further study is being done using a convolution neural network for c ¯ c tagging. This project explored the possibility of using pileup events, the proton-proto","PeriodicalId":127730,"journal":{"name":"Proceedings of the 13th International Conference on Advances in Computer Entertainment Technology","volume":"30 8","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2016-11-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of the 13th International Conference on Advances in Computer Entertainment Technology","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1145/3001773.3001804","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3

Abstract

We calculated the thresholds for charged–current electron neutrino and antineutrino interactions for most of the stable isotopes. Looking at the isotopes with the lowest thresholds, we found that 181 Ta and 160 Gd are reasonable candidates for low–threshold neutrino detectors, with thresholds at 0 . 188 MeV and 0 . 105 MeV respectively. These materials are both metals, have relatively high natural abundance, and are not frequently found in conjunction with radioactive substances, making them potentially viable for this task. Using the SNOwGLoBES software library, we computed estimated cross sections and event rates for supernova fluxes in these two materials. When neutron stars in a low mass x-ray binary system collect matter from their H or He rich companion star, nuclear burning can occur on the high temperature and pressure surface. If a critical accretion rate is reached, it can cause the nuclear reactions to run away, resulting in an X-Ray Burst (XRB). By studying the sensitivity of XRB models to different nuclear reactions, we can help identify which are most important in the burst process. The stellar model used for this study was of an XRB in Modules for Experiments with Stellar Astrophysics (MESA) with a co-processed nuclear network. A single stellar model was rerun once for each nuclear reaction and its inverse in the network, varying its reaction rate by 100. The models with the greatest change indicate reactions that are key to XRB nucleosynthesis. Preliminary results identified 5 significant nuclear reactions. While the study is in its preliminary stage, it has proved capable of highlighting reactions that significantly affect XRB properties. Λ 0 hyperons can be produced from hadronization of a struck quark in Semi-Inclusive Deep In- elastic Scattering (SIDIS). This process is of interest because the Λ 0 hyperon polarization may be inferred from its self-analyzing weak decay. Such probes allow one to extract information about the polarization of the constituent quarks within the proton and provide a test of fundamental aspects of Quantum Chromodynamics (QCD). In this study, we generated SIDIS events using a Lund Monte Carlo and simulated the response of the CLAS12 detector at Jefferson Lab’s Continuous Electron Beam Accelerator Facility (CEBAF)using GEANT4 with different toroidal magnet field strengths and configurations (either inbending or outbending). We then processed events using the CLAS12 reconstruction framework to find the optimal configuration and maximize our reconstruction efficiency from the Λ 0 → π − + p + decay channel. For Λ 0 hyperons coming from a struck quark ( x F > 0 ), we obtained our best reconstruction efficiency in the low field outbending toroidal configuration. Nuclear data for photo-nuclear reactions is scarce. By using the activation technique, ( γ,n ) cross sections can be measured to a high precision. 169 Tm( n, 2 n ) is a common neutron monitor reaction, but there is no available data on its photo-nuclear counterpart, the 169 Tm( γ,n ) reaction. Measurement of this reaction would allow use of thulium as a standard γ -ray monitor. Thulium, tin, and gold samples were irradiated by monoenergetic γ rays provided by the High Intensity γ -ray Source (HI γ S), located at Duke University. The resulting activity was quantified using γ -ray spectroscopy with high purity germanium (HPGe) detectors. The data confirmed the literature half-lives of 196 Au, 123 m Sn, and 168 Tm as 6.16 d, 40.1 m, and 93.1 d, respectively. Cross sections were extracted for the 124 Sn( γ,n ) 123 m Sn and 169 Tm( γ,n ) 168 Tm reactions, representing the first measurements of these reactions. Tritium, a radioactive isotope of hydrogen, will be the basis of experiment P-02-13 at HI γ S. This study will utilize a tritium gas target to obtain cross-section measurements of two-and three-body photodisintegration of the triton in order to further understand nuclear structure and reactions, specifically three-nucleon interactions. In order to reduce loss of the radioactive gas, safety systems will be implemented including a tritium scrubber system. This system will work in conjunction with a copper-zinc catalyst in order to utilize the reduction of copper to continuously transform elemental tritium into T 2 O or HTO, allowing the tritiated water to be collected within a molecular sieve and safely disposed of. Reactions catalyzed by the CuZn bed were examined using a Residual Gas Analyzer at temperatures of 23 ◦ C to 200 ◦ C to measure isotope concentrations and compositions of the various gas streams that will flow through the scrubbing system during normal operation. Low-mass nuclear Compton scattering projects at HI γ S are focused on determining experimentally the static electric ( α E ) and magnetic ( β M ) dipole polarizabilities of neutrons. Building on past experiments, the next iteration will use a liquid 3 He target volume to offer a new nuclear structure for analysis. This project is centered around preparing for the upcoming experiments. A new epoxy-lined gas storage tank was commissioned and sealed for the 3 He gas containment system. Leakage rates were measured, and a residual gas analysis was performed. The sealed tank was shown to have a leak rate of < 2 . 0 × 10 7 mbar*L/sec and main contamination from water, nitrogen, and oxygen at levels that can be removed by internal systems. A computational model was constructed based on particle beam flux attenuation in scattering processes. Values of the contaminate 4 He level C 4 (along with the percentage uncertainty in this value p ( C 4 ) ), the percentage uncertainty in the cross section of the experimental scattering with 4 He p ( σ 4 ) , and the experimental runtime T were varied to determine impact on the percentage uncertainty in the scattering cross section with 3 He. Optimal values (against cost) of T and p ( σ 4 ) were found to be 200h and 10% respectively for C 4 less than 10% and p ( C 4 ) less than 25%. When a proton is placed into an external magnetic field, it will attempt to align its magnetic moment to that field. Then if that external magnetic field is suddenly turned off, the proton will start to precess around the only other magnetic field available, the Earth’s. The goal of this project was to get an instrument operational that would take advantage of this concept. It would be used to find the spin relaxation time ( T 2 ), a measure of the magnetic field gradients, of the sample. This would then be used to test the magnetization of other materials for a larger project. An Earth’s field nuclear magnetic resonance control box and sample coil were used along with a sample of water (our proton source) to produce a waveform from the precession of the water molecules. From that waveform we were able to calculate our T 2 value. After many setbacks and multiple trials, we were successful in operating the instrument to produce waveforms in the correct shape and scale, thus getting a T 2 value that was close to the established value. While more testing and calibration is still needed, the instrument is now working and can be used in future testing of the magnetization of materials. We are developing a pulsed and tunable Pelletron accelerator to provide measurements of bremsstrahlung energy loss for next generation neutron beta decay experiments. The development of our Pelletron system is the first step before any measurements are made. The goals of our project are to improve the performance of an N 2 purge and implement a suppressor electrode to reduce arcing, understand possible sources of coronal discharge loss, make a first detection of the electron beam, and develop a test beam line. These first steps were successful, greatly reducing charge loss and arcing, and confirming the production of over 250 keV electron beams. If the Higgs Boson is made of new constituent particles, it is likely that the top quark is also made of similar particles based on how strongly they couple. In this case, events with four top quarks would be produced in excess of predictions from current theories. The purpose of this project is to study top quark kinematics to determine how to distinguish between background and signal top decays based on top quark transverse momentum. We used MADGRAPH to generate Monte Carlo events where t and ¯ t decay to a bottom quark and a W boson, and the W bosons decay to q ¯ q . Our analysis shows that as the top quark’s transverse momentum increases, the distance between the top quark and its decays in the η − φ space decreases, where η is the pseudo-rapidity and φ is the azimuthal angle. This decrease in distance in the η − φ space as top transverse momentum increases demonstrates that the two high momentum tops in a four top process can be tagged primarily by using position. Searches for c ¯ c from Higgs/ Z decays have been done exclusively for the ground J/ψ state using leptonic decay modes. This project aims to tag excited c ¯ c states via hadronic decay modes. The study of c ¯ c is relevant to Higgs coupling with the charm quark. Excited energy states such as ψ (2 S ) and χ c 0 ,c 1 ,c 2 are of interest as we can follow their decays into J/ψ γ . Excited states of c ¯ c are produced via the standard Higgs/ Z production chain gg → H which creates c ¯ c by H → c ¯ cγ . The purpose of creating this tagging algorithm is to apply it to ATLAS data. The tagging is done using machine learning. Training data for the machine learning algorithm comes from Monte Carlo simulations of particle decays and simulations of interactions in ATLAS. Other Monte Carlo simulations are being tested to verify the stability of the algorithm. The accuracy for the fully-connected neural network trained on J/ψ , ψ (2 S ) , and quark/gluon background is 93%. This novel approach to c ¯ c tagging resulted in a production-ready tagger. Further study is being done using a convolution neural network for c ¯ c tagging. This project explored the possibility of using pileup events, the proton-proto
我们计算了大多数稳定同位素的带电电流电子中微子和反中微子相互作用的阈值。观察最低阈值的同位素,我们发现181 Ta和160 Gd是低阈值中微子探测器的合理候选者,阈值为0。188mev和0。分别为105mev。这两种材料都是金属,具有相对较高的天然丰度,并且不经常与放射性物质一起发现,因此它们可能适用于这项任务。利用SNOwGLoBES软件库,我们计算了这两种物质中超新星通量的估计截面和事件率。当低质量x射线双星系统中的中子星从富含氢或氦的伴星那里收集物质时,在高温高压表面会发生核燃烧。如果达到临界吸积速率,就会导致核反应失控,从而产生x射线暴(XRB)。通过研究XRB模型对不同核反应的敏感性,我们可以帮助确定在爆炸过程中哪些是最重要的。本研究使用的恒星模型是恒星天体物理实验模块(MESA)中的XRB,具有协同处理的核网络。对于每个核反应及其在网络中的逆反应,一个单一的恒星模型重新运行一次,将其反应速率改变100。变化最大的模型表明了XRB核合成的关键反应。初步结果确定了5个重要的核反应。虽然这项研究还处于初步阶段,但它已经证明能够突出影响XRB性质的反应。Λ在半包容深弹性散射(SIDIS)中,撞击夸克的强子化可以产生0超子。这个过程是有趣的,因为Λ 0超子极化可以从它的自分析弱衰变中推断出来。这种探针允许人们提取质子内组成夸克的极化信息,并提供量子色动力学(QCD)基本方面的测试。在这项研究中,我们使用隆德蒙特卡罗生成了SIDIS事件,并使用GEANT4模拟了杰斐逊实验室连续电子束加速器设施(CEBAF)中具有不同环形磁场强度和配置(内弯曲或外弯曲)的CLAS12探测器的响应。然后,我们使用CLAS12重构框架处理事件,从Λ 0→π−+ p +衰变通道找到最佳配置并最大化我们的重构效率。对于来自撞击夸克(x F > 0)的Λ 0超子,我们在低场外弯环面构型下获得了最好的重构效率。光核反应的核数据很少。利用活化技术,可以高精度地测量(γ,n)截面。169 Tm(n, 2 n)是一种常见的中子监测反应,但没有关于其光核对应的169 Tm(γ,n)反应的可用数据。测量这种反应将允许使用铥作为标准的γ射线监测器。铥、锡和金样品由位于杜克大学的高强度γ射线源(HI γ S)提供的单能γ射线照射。用高纯锗(HPGe)探测器的γ射线能谱法对所得活性进行了定量分析。资料证实196 Au、123 m Sn和168 Tm的文献半衰期分别为6.16 d、40.1 m和93.1 d。提取了124 Sn(γ,n) 123 m Sn和169 Tm(γ,n) 168 Tm反应的截面,代表了这些反应的首次测量。氚,氢的一种放射性同位素,将是HI γ s实验P-02-13的基础。这项研究将利用氚气体靶来获得两体和三体光分解的截面测量,以进一步了解核结构和反应,特别是三核子相互作用。为了减少放射性气体的损失,将实施包括氚洗涤器系统在内的安全系统。该系统将与铜锌催化剂一起工作,以利用铜的还原,不断地将元素氚转化为t2o或HTO,使氚化水可以在分子筛内收集并安全处理。使用残余气体分析仪在23°C至200°C的温度下检测由CuZn床催化的反应,以测量在正常操作期间流经洗涤系统的各种气流的同位素浓度和组成。低质量核康普顿散射项目的重点是实验测定中子的静电(α E)和磁(β M)偶极极化率。在过去实验的基础上,下一次迭代将使用液体3氦靶体积来提供新的核结构进行分析。 这个项目的中心是为即将到来的实验做准备。一个新的环氧内衬储气罐被投入使用并密封用于3 He气体密封系统。测量了泄漏率,并进行了残余气体分析。密封罐的泄漏率显示为< 2。0 × 10 7毫巴*升/秒和主要污染的水,氮,氧的水平,可以通过内部系统去除。建立了基于粒子束在散射过程中通量衰减的计算模型。通过改变污染4氦水平的c4值(以及该值的百分比不确定度p (c4))、实验4氦散射截面的百分比不确定度p (σ 4)和实验运行时间T来确定对3氦散射截面百分比不确定度的影响。当c4小于10%,p (c4)小于25%时,T和p (σ 4)的最优值分别为200h和10%。当质子被置于外部磁场中时,它会试图使其磁矩与该磁场对齐。然后,如果外部磁场突然关闭,质子就会开始绕着唯一可用的磁场——地球磁场前进。这个项目的目标是让一个仪器运作,将利用这一概念。它将用于计算样品的自旋弛豫时间(t2),这是测量磁场梯度的一种方法。这将被用来测试其他材料的磁化强度,用于更大的项目。地球磁场核磁共振控制箱和样品线圈与水样品(我们的质子源)一起使用,从水分子的进动产生波形。从这个波形中我们可以计算出t2的值。经过多次挫折和多次试验,我们成功地使仪器产生了正确形状和比例的波形,从而获得了接近既定值的t2值。虽然还需要更多的测试和校准,但该仪器现在正在工作,可以用于未来材料磁化的测试。我们正在开发一种脉冲和可调谐的Pelletron加速器,为下一代中子衰变实验提供轫致辐射能量损失的测量。我们的Pelletron系统的开发是任何测量之前的第一步。我们项目的目标是提高n2吹扫的性能,实现抑制电极以减少电弧,了解冠状放电损耗的可能来源,首次检测电子束,并开发测试束流线。这些第一步是成功的,大大减少了电荷损失和电弧,并确认了超过250千伏特电子束的产生。如果希格斯玻色子是由新的组成粒子组成的,那么根据它们的耦合强度,顶夸克很可能也是由类似的粒子组成的。在这种情况下,具有四个顶夸克的事件将产生超出当前理论预测的结果。本课题的目的是研究顶夸克运动学,以确定如何根据顶夸克横向动量区分背景顶衰减和信号顶衰减。我们使用MADGRAPH生成蒙特卡罗事件,其中t和¯t衰变成一个底夸克和一个W玻色子,W玻色子衰变成q¯q。我们的分析表明,随着顶夸克横动量的增大,顶夸克与它在η - φ空间中的衰变之间的距离减小,其中η为伪速度,φ为方位角。随着顶部横向动量的增加,η−φ空间中距离的减小表明,在四顶过程中,两个高动量的顶部可以主要用位置来标记。从希格斯/ Z衰变中寻找c¯c是专门针对使用轻子衰变模式的基态J/ψ态进行的。该项目旨在通过强子衰变模式标记激发态c¯c。c¯c的研究与希格斯与粲夸克的耦合有关。激发态如ψ (2s)和χ c0, c1, c2是我们感兴趣的,因为我们可以跟随它们的衰变到J/ψ γ。c¯c的激发态是通过标准的希格斯/ Z生产链gg→H产生的,该链条由H→c¯cγ产生c¯c。创建这个标记算法的目的是将其应用于ATLAS数据。标记是用机器学习完成的。机器学习算法的训练数据来自粒子衰变的蒙特卡罗模拟和ATLAS中相互作用的模拟。其他的蒙特卡罗模拟也在测试中,以验证算法的稳定性。在J/ψ, ψ (2s)和夸克/胶子背景下训练的全连接神经网络的精度为93%。这种新颖的c¯c标记方法产生了可用于生产的标记器。进一步的研究正在使用卷积神经网络进行c¯c标记。 这个项目探索了利用堆积事件,质子-原型的可能性 这个项目探索了利用堆积事件,质子-原型的可能性
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