第五届粒子物理前沿研讨会 - The Fifth Workshop on Frontiers of Particle Physics

Name: 第五届粒子物理前沿研讨会 - The Fifth Workshop on Frontiers of Particle Physics
Start: 2024-04-12T09:00:00+08:00
End: 2024-04-16T11:00:00+08:00
Location: No location set

12 Apr 2024, 09:00 → 16 Apr 2024, 11:00 Asia/Shanghai

深圳市光明区天安云谷

Wei Su (SYSU)

Description

第五届粒子物理前沿研讨会将于2024年4月12日至16日（4月12日周五报道注册）在广东省深圳市光明区天安云谷国际会议酒店召开。会议由中山大学主办，中国科学院理论物理研究所、高能物理研究所、中国高等科学技术中心、郑州大学、济南大学、河南师范大学、华南师范大学合办。

会议主题主要围绕粒子物理相关最新进展展开，包括但不限于超越标准模型的新物理、Higgs物理、暗物质物理、中微子物理、粒子天体物理和宇宙学等方面的理论和实验的最新进展，诚挚邀请国内外专家学者参加此次会议。

注册费用：学者及博士后2000元/人，学生1700元/人。会场将主要在酒店学术报告厅。

会务组：杨金民，李田军，刘纯，廖益，岩斌，李洪蕾，王少江，张阳，苏伟(chair)

地方会务组：苏伟，黄永盛，李志兵，韩成成，肖明磊，冯劼，蔡成丰，张林，吴天伟

会议联系人：苏伟 (suwei26@mail.sysu.edu.cn)，
侯超 (houch27@mail.sysu.edu.cn，0755-23260090），
邮件请注明主题：第五届粒子物理前沿研讨会。

Participants

Bin Wang
Bin Yan
bingfang yang
changhong li
Cheng Li
Chengcheng Han
Chengfeng Cai
Di Chen
Fei Huang
feng huang
Hai-Bin Zhang
Haipeng An
Hao Zhang
Hong Zhang
Honglei Li
HongXing Li
Hua Zhou
Huan-Yu Bi
Huayang Song
hui liu
Huiling Liu
Jia Liu
Jia-Jun Wu
Jia-Shu Niu
Jibo HE
Jie Feng
Jin Min Yang
Jingqiang Ye
Jingwei Lian
Junjie Cao
Junmou Chen
Ke-Pan Xie
lang liu
lei wang
Lei Wu
Li Zuhao
Liangchen Liu
Lin Zhang
Liu Bingxuan
Liu Chunmei
Liu Yandong
Lu Huang
lu zhang
Man Yuan
Manqi Ruan
Mengchao Zhang
Ming-Lei Xiao
Mingshui Chen
Ngoc Khanh Vu
Oleg Popov
pengwei zhao
Qing Luo
QING YU
Qing-Hong Cao
Rui Zhu
Ruifeng Leng
Sai Wang
Shao-Feng (韶锋) Ge (葛)
Shao-Jiang Wang
Shu Li
Sida Lu
Song He
Song Li
Sun Tong
Takaaki Nomura
Tao Liu
Teng Ma
Tianjun Li
Tingting Ge
Wei Su
WEIMIN SONG
Wu Yusheng
Xi-Jie Zhan
Xiao-Dong Ma
Xiao-Rui Wang
Xiaohu SUN
Xiaojun Bi
Xiaokang Du
Xiaoping Wang
Xin Zhang
Xing-Gang Wu
Xinyi Zhang
Yang Xiao
Yang Zhang
Yong Tang
Yongcheng Wu
yuanping Wang
Yun Jiang
yusi Pan
Zhang Honghao
Zhang zhenghua
zhao liuxin
zhao mubai
zhaofeng kang
Zhenmin Zeng
Zhi-Hui Guo
Zhi-Zhang Peng
zhiyuan chen
Zhong-Zhi Xianyu
Zihao Wu
Zong-Guo Si
Zong-Kuan Guo
Zongyang Lu
丁溢罗
东苹傅
亦蕾汤
仁晖覃
兆兴樊
光宇王
兴博袁
利娜吴
剑波程
发朋黄
天伟吴
学文刘
学文陈
安刘
应凯张
徐万伦
新恒郭
昊琳王
歆然曾
江闫
泽涵李
洪泰李
海军王
瑞珈张
田志方
祥赵
科盛孙
红生侯
翔肖
至勇王
范红杰
莹高
迅薛
郭怀珂
金葆王
钊焕余
锦汉梁
阿里木(Alim) 肉孜(Ruzi)
霁宁唐
靖皓单
龙斌陈

Friday, 12 April
- 09:30 → 17:30
  
  Registration 8h
Saturday, 13 April
- 08:00 → 08:20
  
  致辞 20m
- 08:20 → 08:45
  
  LHAASO观测和相关新物理研究 25m
  
  TBD
  
  Speaker: Xiaojun Bi (IHEP)
  
  LHAASO科学研究（深圳）.pptx
- 08:45 → 09:10
  
  Consequences of phase transitions happened during inflation 25m
  
  TBD
  
  Speaker: Haipeng An (Tsinghua University)
  
  shenzhen2024_HaipengAN.pdf
- 09:10 → 09:35
  
  Highlights of Recent Physics Results from the ATLAS experiment 25m
  
  This talk will present some of interesting physics results recently acheived by the ATLAS experiment. The focus will be on measurements of Standard Model processes and Higgs properties, but examples of new physics searches will be covered as well. Methodologies and possible future directions will also be discussed.
  
  Speaker: Prof. Yusheng Wu
  
  Highlight%20of%20Recent%20ATLAS%20Results%20-%202024.4.13.pptx
- 09:35 → 10:00
  
  Higgs and beyond at the CMS experiment 25m
  
  TBD
  
  Speaker: Prof. Xiaohu Sun
  
  HiggsAndBeyondCMS- Xiaohu SUN.pdf
- 10:00 → 10:30
  
  茶歇/合影 30m
- 10:30 → 10:55
  
  Family tree decomposition of cosmological correlators 25m
  
  The correlation functions of large-scale fluctuations are crucial observables in modern cosmology. There have been considerable efforts in the analytical study of cosmological correlators in recent years. In this talk, I will introduce the basic structure of cosmological correlators and several analytical methods we recently proposed for computing them. In particular, I will describe the family tree decomposition of arbitrary nested time integrals. With this method, we largely solve the problem of analytical computation of massive tree amplitudes in dS and conformal scalar tree amplitudes in a power-law FRW universe.
  
  Speaker: Prof. Xianyu Zhong-Zhi (Tsinghua University)
  
  FamilyTree_Shenzhen_PNG.pdf
- 10:55 → 11:20
  
  Primordial black holes and non-Gaussianity in the gravitational-wave era 25m
  
  近期脉冲星计时阵列合作组发现了纳赫兹引力波背景的关键证据。学术界掀起有关引力波源的诸多讨论，除超大质量黑洞外，宇宙学源也受到强烈关注。本报告将着重介绍次级引力波的研究进展。我们将探讨原初非高斯性对次级引力波的重要贡献，并在此基础上分析纳赫兹引力波探测数据，进而尝试解决原初黑洞的过量产生问题。进一步地，我们提出表征次级引力波各向异性的角功率谱可作为原初非高斯性的有力探针。我们预期引力波探针将在原初黑洞暗物质和宇宙起源研究中扮演重要角色。
  
  Speaker: Prof. Sai 赛 Wang 王 (IHEP-CAS)
  
  Sai_Wang_Apr13.pdf
- 11:20 → 11:45
  
  耗散效应作为宇宙相变的新观测量 25m
  
  宇宙一阶相变引力波提供了粒子物理研究的新手段，在国内和国际上得到了广泛的研究。
  在这一报告中，我将介绍此前很少被考虑的相变中的耗散效应，并讨论强耗散效应下相
  变图像及引力波发生的改变。
  
  Speaker: Huaike Guo (University of Chinese Academy of Sciences)
  
  Huaike_Guo.pdf
- 11:45 → 12:10
  
  Primordial black hole formation in slow phase transitions 25m
  
  -
  
  Speaker: Ke-Pan (柯盼) Xie (谢) (Beihang University)
  
  SYSU-Shenzhen.pdf
- 12:10 → 14:00
  
  午餐 1h 50m
- 14:00 → 15:40
  Parallel session I
  
  中山大学深圳校区西教学楼 201
  - 14:00
    
    Novel methods for analytic Feynman integral computation based on algebraic geometry 25m
    
    Feynman integrals are key objects in quantum field theory. They are crucial for the perturbative evaluation of scattering amplitudes, which leads to observables in high-energy experiments. Recently, multi-loop Feynman integral computation has become a popular field. It corresponds to high-precision predictions for experiments. Thus, they are very important for higher-order validation of the Standard Model (SM) and in the search for clues to new physics beyond the SM. Nowadays, multi-loop Feynman integral evaluation is facing challenges brought by its heavy computation. These challenges prevent us from evaluating the Feynman integrals necessary for high-precision experimental processes. In this talk, I will introduce some efforts that we have made to face these challenges. I will demonstrate that some new mathematical tools, like algebraic geometry, are very helpful in developing new algorithms, which, in a great manner, decrease the computation expense for some bottleneck steps in Feynman integral computations. I will also show the latest development of new packages based on these algorithms.
    
    Speaker: Dr Zihao Wu
    
    Novel methods for Feynman integral computation based oncomputational algebraic geometry.pptx
  - 14:25
    
    When scalar-induced gravitational waves meet pulsar timing arrays 25m
    
    The recently released data by pulsar timing array collaborations present strong evidence for a stochastic signal consistent with a gravitational-wave background. In this talk, I will discuss some implications for scalar-induced gravitational waves with pulsar timing arrays.
    
    Speaker: Dr lang liu (Beijing Normal University)
    
    PTA and SIGW.pdf
  - 14:50
    
    Axion-pion scattering at finite temperature in chiral perturbation theory and its influence in axion thermalization 25m
    
    Axion-pion scattering amplitudes at finite temperatures are calculated within SU(2) chiral perturbation theory up to one loop level. Unitarization procedure is implemented to these amplitudes in order to extend the applicable range of energy and temperature. The influence of the thermal axion-pion scattering amplitudes on the $a\pi\to\pi\pi$ cross sections and the axion thermalization rate is investigated, with the emphasis on the comparison with the zero-temperature-amplitude case. A brief discussion on the cosmological implication of the axion thermalization rate, that is calculated by using the $a\pi\to\pi\pi$ amplitudes at finite temperatures, is also given. The thermal corrections to the axion-pion scattering amplitudes can cause around a 10% shift of the determination of the axion decay constant $f_a$ and its mass $m_a$, comparing with the results by using the $a\pi\to\pi\pi$ amplitudes at zero temperature.
    
    Speaker: 金葆王 (东南大学)
    
    Slide-api to pipi.pdf
  - 15:15
    
    Axions in electromagnetodynamics and their detection 25m
    
    The Witten effect implies the electromagnetic interactions between axions and magnetic monopoles. Based on the quantum electromagnetodynamics, a generic low-energy axion-photon effective field theory was built by introducing two four-potentials ($A^\mu$ and $B^\mu$) to describe a photon. More anomalous axion-photon interactions and couplings ($g_{aAA}$, $g_{aBB}$ and $g_{aAB}$) arise in contrary to the ordinary axion coupling $g_{a\gamma\gamma}aF^{\mu\nu}\tilde{F}_{\mu\nu}$. As a consequence, the conventional axion Maxwell equations are further modified.
    
    In this talk, I mainly discuss the theoretical framework of axion electromagnetodynamics. I will also show two axion searching strategies in the framework of QEMD, and give the corresponding sensitivity of couplings in different axion mass region.
    
    Speaker: Rui-jia Zhang (Nankai University)
    
    张瑞珈_第五届粒子物理深圳2.pptx
- 14:00 → 15:40
  Parallel session II
  
  中山大学深圳校区西教学楼 202
  - 14:00
    
    Complementary LHC searches for UV resonances of 0νββ decay operators 25m
    
    ∆L = 2 lepton number violation at the TeV scale connects $0\nu\beta\beta$ decay (intensity frontier), LHC
    searches (energy frontier), and leptogenesis (cosmic frontier). I will focus on some progress on the
    promising UV completions of $0\nu\beta\beta$ decay operators, which can be diagnosed with complementary
    searches at the HL-LHC and HE-LHC.
    
    Speaker: Mr 祥赵 (中山大学)
    
    第五届粒子物理前沿研讨会-zx.pdf
  - 14:25
    
    Macroscopic States as Dark Matter Candidates 25m
    
    Despite that weakly interacting massive particles are still very well-motivated dark matter candidates, the null-results of direct detection experiments are hints and encouragements that we may need to think of other dark matter paradigms. In this talk, I will discuss the possibility that dark matter consists completely or partially of macroscopic states. It turns out that macroscopic dark matter candidates can arise in many different theories, either fermionic or bosonic. They can be produced in the early universe through a cosmic phase transition, and later evolution may change their masses, sizes and abundance. Given that macroscopic dark matters occupy a very different parameter space from that of particle dark matters, they are in general indifferent to direct detection. While on the other hand, this also enables these large objects to provide unique and interesting signatures for phenomenological studies.
    
    Speaker: Sida Lu (HKUST)
    
    SL_SYSUShenzhen_MDM.pdf
  - 14:50
    
    Recent Dark Matter combination summary from ATLAS 25m
    
    Ref: https://arxiv.org/abs/2306.00641
    
    Results from a wide range of searches targeting different experimental signatures with and without missing transverse momentum ($E^{miss}_T$) are used to constrain a Two-Higgs-Doublet Model (2HDM) with an additional pseudo-scalar mediating the interaction between ordinary and dark matter (2HDM+a). The analyses use up to 139 fb$^{−1}$ of proton-proton collision data at a centre-of-mass energy $\sqrt{s}$ = 13 TeV recorded with the ATLAS detector at the Large Hadron Collider between 2015-2018. The results from three of the most sensitive searches are combined statistically. These searches target signatures with large EmissT and a leptonically decaying Z boson; large $E^{miss}_T$ and a Higgs boson decaying to bottom quarks; and production of charged Higgs bosons in final states with top and bottom quarks, respectively. Constraints are derived for several common as well as new benchmark scenarios within the 2HDM+a.
    
    Speaker: Dr Ngoc Khanh Vu (Tsung-Dao Lee Institute, Shanghai Jiao Tong University)
    
    2HDMa_Khanh.pdf
  - 15:15
    
    phase transition catalyzed by primordial black hole 25m
    
    We investigate the first-order phase transition catalyzed by primordial black holes~(PBHs) in the early Universe. We find that super-horizon curvature perturbations generated in this scenario lead to the production of gravitational waves when the scalar modes re-enter the horizon. If PBHs with masses about $10^{-13}M_{\odot}$ constitute all dark matter, the first-order electroweak phase transition catalyzed by PBHs can explain the gravitational wave signal observed by pulsar timing array collaborations without the overproduction of PBHs.
    
    Speaker: Mr Zeng Zhenmin (ITP-CAS)
    
    Phase transition catalyzed by primordial black holes_sz.pptx Phase transition catalyzed by primordial black holes_zssz.pptx
- 15:40 → 16:00
  
  茶歇 20m
- 16:00 → 21:00
  
  乘车晚宴 5h
Sunday, 14 April
- 08:30 → 08:55
  
  Indirect search for new physics at LHCb 25m
  
  In this talk, I will review indirect searches for new physics at LHCb.
  
  Speaker: Jibo HE (University of Chinese Academy of Sciences)
  
  20240414_NPatLHCb.pdf
- 08:55 → 09:20
  
  伽玛对撞机及综合束流设施 25m
  
  Speaker: Prof. 永盛黄 (中山大学)
  
  伽玛光子对撞机及其产业化规划-20240414-物理版.pdf
- 09:20 → 09:45
  
  Neutrino Mass Measurement with Cosmic Gravitational Focusing 25m
  
  We thoroughly explore the cosmic gravitational focusing of cosmic neutrino fluid (CνF) by dark matter (DM) halo using both general relativity for a point source of gravitational potential and Boltzmann equations for continuous overdensities. Derived in the most general way for both relativistic and non-relativistic neutrinos, our results show that the effect has fourth power dependence on the neutrino mass and temperature. With nonlinear mass dependence which is different from the cosmic microwave background (CMB) and large scale structure (LSS) observations, the cosmic gravitational focusing can provide an independent cosmological way of measuring the neutrino mass and ordering. We take DESI as an example to illustrate that the projected sensitivity as well as its synergy with existing terrestrial neutrino oscillation experiments and other cosmological observations can significantly improve the neutrino mass measurement.
  
  Speaker: Shao-Feng (韶锋) Ge (葛) (Tsung-Dao Lee Institute (TDLI), Shanghai Jiao Tong University (SJTU))
  
  240414_深圳.pdf
- 09:45 → 10:10
  
  超轻暗物质粒子唯象学研究 25m
  
  TBD
  
  Speaker: Prof. Xiaoping Wang
  
  XPWang-2024-4-14.pdf
- 10:10 → 10:30
  
  茶歇 20m
- 10:30 → 10:55
  
  AMS最新实验物理结果 25m
  
  TBD
  
  Speaker: Prof. Zuhao Li (IHEP)
- 10:55 → 11:20
  
  Probing Ultralight Dark Matter with Laser Interferometers in Space 25m
  
  Ultralight bosonic fields (ULBFs) are predicted by various theories beyond the standard model of particle physics and are viable candidates of cold dark matter. There have been increasing interests to search for the ULBFs in physical and astronomical experiments. In this paper, we investigate the sensitivity of several planned space-based gravitational-wave interferometers to ultralight scalar and vector fields. Using time-delay interferometry (TDI) to suppress the overwhelming laser frequency noise, we derive the averaged transfer functions of different TDI combinations to scalar and vector fields, and estimate the impacts of bosonic field's velocities. We obtain the sensitivity curves for LISA, Taiji and TianQin, and explore their projected constraints on the couplings between ULBFs and standard model particles, illustrating with the ULBFs as dark matter.
  
  Speaker: Yong Tang (University of Chinese Academy of Sciences)
  
  DM_GW_Yong_Tang.pdf
- 11:20 → 11:45
  
  Axion Bose-Einstein Condensate 25m
  
  Axions, or in general axion-like particles, are popular dark matter candidates. They could form Bose-Einstein condensate in our universe. In this talk, I will discuss two different types of condensates: axion stars and black-hole superradiantaxion clouds. These condensates could emit radio-frequency photons as well as gravitational waves. The unique signatures of these signals will also be discussed.
  
  Speaker: Prof. Hong Zhang
  
  Hong_Zhang_20240414.pdf
- 11:45 → 12:10
  
  Neutrino Mass Sum Rules from Modular A4 Symmetry 25m
  
  Modular symmetries offer a dynamic approach to understanding the flavour structure of leptonic mixing. Using the modular A4 flavour symmetry integrated in a type-II seesaw, we propose a simple and minimalistic model that restricts the neutrino oscillation parameter space and, most importantly, introduces a sum rule in the physical neutrino masses. When combined with the mass squared differences observed in neutrino oscillations, this sum rule determines the absolute neutrino mass scale. This has significant implications for cosmology, neutrinoless double beta decay experiments and direct neutrino mass measurements. In particular, the model predicts $\sum_i m_i \approx 0.1$ eV for both normal and inverted ordering, and thus can be fully probed by the current generation of cosmological probes in the upcoming years.
  
  Speaker: Prof. Oleg Popov
  
  Popov_5FPP_2024.pdf
- 12:10 → 14:00
  
  午餐 1h 50m
- 14:00 → 14:25
  
  Evaluating Feynman integrals by hypergeometric function method 25m
  
  We evaluate Feynman integrals by hypergeometric function method.
  
  Speaker: Prof. Hai-Bin Zhang (Hebei University)
  
  Evaluating Feynman integrals by hypergeometric function__ method.pdf
- 14:25 → 14:50
  
  Helicity amplitudes without gauge cancellation for electroweak processes 25m
  
  Multiple EW vector boson amplitudes are known to have bad energy behavior for individual Feynman diagrams, which causes many problems for numerical and theoretical analysis. Based on Goldstone equivalence theorem(GET), we introduce a new representation of Feynman rules that makes GET manifest, while reproduces the exact results of the amplitudes. The new helicity has no subtle gauge cancellation, every diagram has a specific physical interpretation, when the pole approaches on-shell. We implement this new Feynman rules into numerical codes of HELAS (Helicity Amplitude Subroutines) and study several process with the new HELAS.
  
  Speaker: Junmou Chen (Jinan University)
  
  HELAS-EW-SZ.pdf
- 14:50 → 15:15
  
  电弱修正计算研究 25m
  
  本次报告将介绍近期的电弱修正计算。
  
  Speaker: Prof. Chen Long-Bin
  
  Chen-Higgs414v1.pptx
- 15:15 → 15:40
  
  Electroweak corrections to double Higgs production at the LHC 25m
  
  We present the results for the complete next-to-leading order electroweak corrections to pp → HH at the Large Hadron Collider, focusing on the dominant gluon-gluon fusion process. While the corrections at the total cross-section level are approximately −4%, those near the energy of HH production threshold exceed +15%, and corrections at the high-energy region are around −10%, leading to a shape distortion for the differential distributions. Our findings substantially diminish the theoretical uncertainties associated with this pivotal process, providing valuable input for understanding the shape of the Higgs boson potential upon comparison with experimental measurements.
  
  Speaker: Huan-Yu Bi
  
  pp-HH.pdf
- 15:40 → 16:00
  
  茶歇 20m
- 16:00 → 16:25
  
  Bootstrapping the Chiral Anomaly at Large Nc 25m
  
  TBD
  
  Speaker: Prof. Teng Ma (UCAS)
  
  粒子物理研讨会__ talk.pdf
- 16:25 → 16:50
  
  电弱相变动力学的精确计算 25m
  
  TBD
  
  Speaker: Fa Peng Huang (Sun Yat-sen University)
  
  电弱相变动力学的精确计算v2.pdf
- 16:50 → 17:15
  
  近简并Z/Z'粒子系统的探测 25m
  
  通常文献中对于Z'粒子的探测都假定Z'与Z玻色子的共振峰相距甚远。当Z'与Z粒子近简并且可能有强烈混合时，文献中缺乏详细的讨论。在这种情况下，Z'和Z的共振峰可能很难分开，过去对撞机上的探测结论都失效了。针对这种情况，我们模拟了一种类似LEP的探测器，通过探测Z'-Z重叠共振峰的形状，讨论了这种探测器对于Z'粒子探测的敏感度。我们进一步以CEPC为例，讨论了有关探测器的敏感度。
  
  Speaker: Yi-Lei Tang (中山大学)
  
  NearlyDegenerateVector.pdf
- 17:15 → 18:30
  
  晚宴+自由讨论 1h 15m
Monday, 15 April
- 08:30 → 08:55
  
  X-ray polarimetric features of Gamma-ray Bursts across varied redshifts and hints for Axion-Like-Particles 25m
  
  The study of polarimetric features during the prompt phase of Gamma-ray Bursts (GRBs) has been essential for elucidating the debated emission mechanisms and gaining insight into the inner structure of GRBs. However, the potential impact of photon-Axion-Like-Particles (ALPs) mixing in extragalactic magnetic fields, leading to significant modifications in the initial polarization, has been overlooked in discussions concerning prompt phase constraints. In this article, we first examine the statistical characteristics of linear polarization degree ($\Pi_{L}$) in GRBs, utilizing data from updated polarimetric missions focusing on sub-MeV emissions. Our analysis, conducted with a restricted sample of GRBs spanning various redshifts, reveals a diverse distribution of $\Pi_{L}$, which currently shows no correlation with spectral parameters or properties of candidate host galaxies. Furthermore, we explore alternations to the initial $\Pi_{L}$ due to photon-ALP mixing within a domain-like structure of the intergalactic magnetic field (${\bf B}_{\rm IGM} $), considering various parameter sets associated with ALPs and ${\bf B}_{\rm IGM}$. With the existence of ALPs with mass $m_{a}$$~$$\lesssim$$~$$10^{-14}$$~$eV and photon-ALP coupling constant $g_{a\gamma}$$\simeq$$0.5\times10^{-11}$$~$GeV$^{-1}$, we show that for GRBs with redshifts above approximately 1, fully linearly polarized photons may experience a polarization reduction of up to $20\%$, whereas for unpolarized photons, the mixing can increase polarization by up to ~$40\%$. To ensure that the effect of mixing is small enough to be negligible, there is a strong constraint on the mixing term $\Delta_{a\gamma}$ should be less than $1.5\times 10^{-4}\rm Mpc^{-1}$. Currently, the number of GRBs with both sub-MeV polarization measurements and redshift confirmation remains very limited. Harf of the GRBs with available polarization data have a $\Pi_{L}$ of less than 30\%. Certification of redshift for this subset of GRBs would aid in further constraining the parameter space of low-mass ALPs or providing an independent means to determine the upper limit on ${\bf B}_{\rm IGM}$
  
  Speaker: Dr Feng Huang (Xiamen University)
  
  HF20240415-SZ.pdf
- 08:55 → 09:20
  
  Matter Asymmetry Genesis in the $Z_N$-companion Dark Matter Models 25m
  
  Ref.~\cite{Guo:2021rre} proposes a class of $Z_{N\geq 3}$-symmetric WIMP dark matter characterized by the semi-annihilation into the companion of dark matter, evading the stringent direct detection constraint. In this work, we point out that such kind of models naturally provides the three Sakharov elements necessary for dark matter asymmetry, and moreover this asymmetry can be transferred to the visible sector with a proper link to the leptonic or quark sector. In our minimal $Z_3$ example, the migration to the leptonic sector is via the asymmetric companion decay into neutrinos, and the lepton asymmetry can be further transferred to the quark sector for heavy dark matter ($\gtrsim 3$TeV). In particular, the CP violation parameter in our model is suppressed in the limit of static annihilation of dark matter, and we, for the first time, study the lift from thermal motion. We make a preliminary numerical analysis based on the Boltzmann equations, to find that both correct relic density of dark matter and baryon asymmetry can be accommodated.
  
  Speaker: Zhaofeng Kang
  
  matter asymmetry 深圳.pdf
- 09:20 → 09:45
  
  Explaining the CDF W-mass shift and (g-2) mu in a Z prime scenario and its implications for the b to s llprocesses 25m
  
  TBD
  
  Speaker: Xing-Bo Yuan (Central China Normal University)
  
  slides_upload.pdf
- 09:45 → 10:10
  
  The new physics implication for the recent Belle II observation of B^+ → K^+ νν ̄ 25m
  
  no.
  
  Speaker: Xiao-Dong Ma (scnu)
  
  20240415-Shenzhen-Ma.pdf
- 10:10 → 10:30
  
  茶歇 20m
- 10:30 → 10:55
  
  Possible Dark Matter Signals from White Dwarfs 25m
  
  In our galaxy, the white dwarfs (WDs) will inevitably capture the dark matter (DM) particles streaming through them, if there exist interactions between DM particles and nuclei/electrons. At the same time, these DM particles can also be evaporated by the nuclei/electrons in a WD if they have proper mass and the WD is not too cold. The evaporation of DM particles will lead to a faster cooling evolution than that predicted by the stellar evolution theory.
  In this work, we ascribe the faster cooling evolution of three observed WDs to the capture and evaporation of DM particles, and get the possible DM particle's mass and DM-electron cross section.
  The results are beyond the detection capabilities of current direct detection experiments and should be cross checked by more novel scenarios in the future.
  
  Speaker: Jia-Shu Niu (Shanxi University)
  
  Niu_20240415.pdf
- 10:55 → 11:20
  
  Search for dark matter with XENONnT 25m
  
  The XENONnT experiment, located in Laboratori Nazionali del Gran Sasso (LNGS), is a direct detection experiment designed to search for Weakly Interacting Massive Particles (WIMPs) using a dual-phase time projection chamber with 8.5 tonnes of xenon. The experiment began collecting science data in 2021 and is currently in operation. In its first science run (SR0), the experiment achieved an electronic recoil background of 15.8 events/(tonne-year-keV) below 30 keVee, establishing a new benchmark as the lowest background recorded in a dark matter detector. This achievement was made possible by reducing the amounts of radioactive Kr-85 and Rn-222 to an unprecedented low level. With the SR0 data, XENONnT has excluded new physics interpretations of the XENON1T excess and released the first WIMP search results. In this talk, I will present the first two results from XENONnT and the experiment's outlook.
  
  Speaker: Prof. Jingqiang Ye (The Chinese University of Hong Kong, Shenzhen)
  
  xenonnt_shenzen_ye.pdf
- 11:20 → 11:45
  
  $\alpha$ generalized no-scale inflation 25m
  
  ...
  
  Speaker: Lina Wu (Xi’an Technological University)
  
  lina_Wu0415.pdf
- 11:45 → 12:10
  
  Analysis of the top-quark pair production via the $e^{+} e^{-}$ annihilation near the threshold region using the Principle of Maximum Conformality 25m
  
  We present an improved analysis of the top-quark pair production via the process $ e^{+}e^{-} \to \gamma^{*} \to t\bar{t}$ near the threshold region up to next-to-next-to-next-to-leading order (N$^{3}$LO) QCD corrections. Near the threshold region, the top-quark velocity $v$ tends to zero, leading to Coulomb singularity. To achieve a reasonable prediction in the threshold region, we reconstruct the analytical expression for the Coulomb-terms up to N$^{3}$LO accuracy by using the PSLQ lgorithm, whose numerical values agree well with the previous N$^{3}$LO-level calculations. It is found that the N$^{3}$LO series still has sizable renormalization scale dependence, and to improve the precision of the series, we apply the Principle of Maximum Conformality to eliminate such scale dependence. After that, the Coulomb part is resummed into a Sommerfeld-Gamow-Sakharov factor, which finally leads to a much more reasonable behavior near the threshold region.
  
  Speaker: Jiang Yan (Chongqing University)
  
  Principle of maximum conformality.pptx
- 12:10 → 14:00
  
  午餐 1h 50m
- 14:00 → 14:25
  
  Bubble-free first-order phase transitions 25m
  
  Traditionally a cosmic first-order phase transition proceeds by nucleating handful of bubbles through quantum tunneling. However, the presence of domain walls during the transition may greatly enrich the way phase transitions are completed. In this talk we develop the bubble-free mechanism, which constitutes a competing means of accomplishing the phase transition where bubble nucleation is inefficient or absolutely prohibited.
  
  Speaker: Yun Jiang (Sun Yat-sen University)
- 14:25 → 14:50
  
  利用有效场论研究电弱相变 25m
  
  我们利用基于重整化理论的Dimensional Reduction来研究SMEFT模型下的一阶相变。我们展示了不同阶Dimensional Reduction计算结果对重整化能标的依赖性，以及化学势对该系统的影响。我们发现在两圈的精度下，Dimensional Reduction的结果对重整化能标的依赖性相对于树图和一圈而言可以忽略。此外，化学势对临界温度和成核温度的影响很弱，但会使相变强度和sphaleron energy明显降低。我们的结果显示，计算至两圈的Dimensional Reduction可以有效降低由重整化能标导致的理论不确定性，同时化学势的存在会明显影响实验对模型参数的限制。
  
  Speaker: 仁晖覃 (重庆大学)
  
  20240415-Finite temperature effective theory for Electroweak phase transition.pptx
- 14:50 → 15:15
  
  Non-thermal leptogenesis from inflaton decay 25m
  
  There is growing evidence that the early Universe experienced inflationary expansion, yet no consensus has been drawn on the details. Meanwhile, neutrino physics is entering a precision era, making more information on masses and mixings available. We consider a neutrino path to the early Universe confronting the situation above. With right-handed neutrinos (RHNs) coupling to the inflaton, the baryon-antibaryon asymmetry may connect to inflationary observables, leading to a testable framework for particle physics and cosmology. We investigate non-thermal leptogenesis from inflaton decays in the type-I seesaw model, where a complex scalar is introduced to generate the Majorana mass of the RHNs. We find four characteristic limits with working conditions to identify them and show the combined parameter space.
  
  Speaker: Prof. Xinyi Zhang (Hebei University)
  
  ntlep-XYZ.pdf
- 15:15 → 15:40
  
  Recent progress of Dark SHINE R&D 25m
  
  Dark SHINE is a newly proposed fixed-target experiment at SHINE (Shanghai high repetition rate XFEL and extreme light facility, being the 1st hard X-ray FEL in China) under construction targeting completion in 2026. Dark SHINE aims to search for the new mediator, Dark Photon, bridging the Dark sector and the ordinary matter. In this work and presentation, we present the idea of this new project and 1st prospective study in search for Dark Photon decaying into light dark matter. It also provides the opportunity to incorporate broader scope of BSM search ideas such as ALP, utilizing the fixed-target experiment of this type.
  
  Speaker: Dr Tong Sun (TDLI, SJTU)
  
  DarkSHINE20240415-suntong .pdf
- 15:40 → 16:00
  
  茶歇 20m
- 16:00 → 16:25
  
  Higgs properties and new physics beyond the SM 25m
  
  The discovery of the Higgs boson at the Large Hadron Collider (LHC) has opened a new era in particle physics. Precise measurements of the properties of the Higgs boson are crucial for addressing several fundamental questions
  in the field. These include understanding the mechanism behind electroweak symmetry breaking, unraveling the origin of particle masses, and exploring potential sources of CP violation that could explain the matter-antimatter asymmetry in the universe, and so on. In this talk, I will provide an overview of the recent advancements in Higgs physics, both within the framework of the Standard Model (SM) and beyond. By examining the latest research, we will gain insights into the properties and behavior of the Higgs boson,
  shedding light on the fundamental workings of the universe.
  
  Speaker: Prof. Bin Yan (IHEP)
  
  Higgs_BY.pdf
- 16:25 → 16:50
  
  第六届简介 25m
  
  Speaker: 松何 (吉林大学)
  
  粒子物理研讨会-深圳.pdf
- 16:50 → 17:15
  
  自由讨论 25m
- 17:15 → 18:30
  
  晚餐 1h 15m