BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Dark photon enlighten by kinetic mixing
DTSTART;VALUE=DATE-TIME:20190701T052000Z
DTEND;VALUE=DATE-TIME:20190701T055000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-32@indico.itp.ac.cn
DESCRIPTION:Speakers: 何 小刚 (上海交大/台湾大学)\nI will revie
 w the current status of B anomalies and discuss possible new physics assoc
 iated.\n\nhttps://indico.itp.ac.cn/event/1/contributions/32/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/32/
END:VEVENT
BEGIN:VEVENT
SUMMARY:A study of the pentaquark states
DTSTART;VALUE=DATE-TIME:20190701T045000Z
DTEND;VALUE=DATE-TIME:20190701T052000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-31@indico.itp.ac.cn
DESCRIPTION:Speakers: 肖 楮文 (Central South Univesity)\nThe LHCb colla
 boration has reported recently three pentaquark states found in the J/ψN 
 mass distribution. Based on the constraints of the heavy quark spin symmet
 ry combined with the local hidden gauge symmetry\, we investigate the D(
 ∗)Σ(∗) interactions\, together with J/ψN and other coupled channels\
 , using a coupled channel approach. From the poles found in the second Rie
 mann sheets\, we dynamically reproduce the three states identified with th
 e masses and the widths. Thus\, we determine their quantum numbers and app
 roximate molecular structure as 1/2− D ̄Σc\, 1/2− D ̄∗Σc\, and 3
 /2− D ̄∗Σc\, and isospin I = 1/2. In our research procedure\, we als
 o predict some other states: (1) one 3/2− D ̄Σ∗c state with the mass
  of around 4374 MeV\, for which indications appear in the experimental spe
 ctrum\; (2) two other near degenerate states of 1/2− D ̄∗Σ∗c and 3
 /2− D ̄∗Σ∗c\, found around 4520 MeV\; (3) a 5/2− D ̄∗Σ∗c s
 tate\, appeared at the same energy. Our findings also serve as a guide for
  further experimental studies.\n\nhttps://indico.itp.ac.cn/event/1/contrib
 utions/31/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/31/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Threshold resummation at subleading power
DTSTART;VALUE=DATE-TIME:20190701T042000Z
DTEND;VALUE=DATE-TIME:20190701T045000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-30@indico.itp.ac.cn
DESCRIPTION:Speakers: 王 健 (山东大学)\nWe derive a threshold resumm
 ation formula at next-to-leading power employing the soft-collinear effect
 ive theory. The anomalous dimensions of subleading-power soft functions ar
 e calculated directly. As a result\, we resum the leading logarithms near 
 the kinematic threshold. Expansion of the resummed result leads to the lea
 ding logarithms at fixed orders\, providing new results at the five-loop o
 rder and beyond.\n\nhttps://indico.itp.ac.cn/event/1/contributions/30/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/30/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Interactions between two heavy mesons within chiral perturbation t
 heory
DTSTART;VALUE=DATE-TIME:20190701T033000Z
DTEND;VALUE=DATE-TIME:20190701T040000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-29@indico.itp.ac.cn
DESCRIPTION:Speakers: 刘 占伟  (兰州大学)\nWe have studied the inte
 ractions between two heavy mesons [D^(*)-D^(*) or B^(*)-B^(*)] within heav
 y meson chiral effective field theory. The effective potentials are calcul
 ated with Weinberg's scheme up to one-loop level. At the leading order\, f
 our body contact interactions and one pion exchange contributions are cons
 idered. In addition to two pion exchange diagrams\, we include the one-loo
 p chiral corrections to contact terms and one pion exchange diagrams at th
 e next-to-leading order. The behaviours of effective potentials both in mo
 mentum space and coordinate space are investigated and discussed extensive
 ly. We notice the contact terms play important roles in determining the ch
 aracteristics of the total potentials. The possible molecular states are a
 lso investigated and the binding energies are provided by solving the Schr
 odinger equation.\n\nhttps://indico.itp.ac.cn/event/1/contributions/29/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/29/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The QCD trace anomaly in the hadron
DTSTART;VALUE=DATE-TIME:20190701T030000Z
DTEND;VALUE=DATE-TIME:20190701T033000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-28@indico.itp.ac.cn
DESCRIPTION:Speakers: 杨 一玻  (中科院理论物理所)\nThe QCD trac
 e anomaly is the basic anomaly to make the massless hadron in the chiral l
 imit to be massive. Its contribution to the hadron is predicted by the sum
  rule\, while the direct calculation or experimental determination is abse
 nt util recently. I will show the theoretical progress and discuss the pos
 sible experimental opportunities.\n\nhttps://indico.itp.ac.cn/event/1/cont
 ributions/28/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/28/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Direct CP violation in charmed meson decays
DTSTART;VALUE=DATE-TIME:20190701T023000Z
DTEND;VALUE=DATE-TIME:20190701T030000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-27@indico.itp.ac.cn
DESCRIPTION:Speakers: 鄭 海揚  (中央研究院物理研究所)\nIn 201
 2 Cheng-Wei Chiang and I have studied direct CP violation in singly Cabibb
 o-suppressed D decays within the topological diagram approach. We conclude
 d that the direct CP asymmetry difference \\Delta A_{CP} between D0 -> K+ 
 K- and D0 -> pi+ pi- is about (-0.139+/- 0.004)\\% and (-0.151+/-0.004)\\%
  for the two solutions of W-exchange amplitudes\, respectively. The first 
 observation of CP violation in the charm sector was recently announced by 
 LHCb with the result \\Delta A_{CP}=(-0.154+/-0.029)\\%. This is a great t
 riumph of the standard model. In this talk I'll discuss its implications a
 nd present new predictions in other D -> PP and VP modes (P: pseudoscalar 
 meson\, V: vector meson).\n\nhttps://indico.itp.ac.cn/event/1/contribution
 s/27/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/27/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Extension of scalar-tensor theories and spatially covariant gravit
 y
DTSTART;VALUE=DATE-TIME:20190630T045000Z
DTEND;VALUE=DATE-TIME:20190630T052000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-20@indico.itp.ac.cn
DESCRIPTION:Speakers: 高 显 (中山大学)\nIn order to explain the acce
 lerated expansion of our universe in its early stage and today\, the most 
 popular approach is to introduce a scalar field to drive the inflation or 
 to act as dark energy. This is the so-called scalar-tensor theory of gravi
 ty. In this talk\, we first review the development of the scalar-tensor th
 eories with higher derivatives in the recent years. Then we introduce the 
 idea of constructing gravity theories respecting only the spatial symmetry
 \, which propagate a single scalar degree of freedom and thus correspond t
 o even larger class of healthy scalar-tensor theories with higher derivati
 ves. Finally we discuss the propagation of gravitational waves in our fram
 ework.\n\nhttps://indico.itp.ac.cn/event/1/contributions/20/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/20/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gravitational waves and extra dimensions: a short review
DTSTART;VALUE=DATE-TIME:20190630T033000Z
DTEND;VALUE=DATE-TIME:20190630T040000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-18@indico.itp.ac.cn
DESCRIPTION:Speakers: 刘 玉孝 (兰州大学)\nhttps://indico.itp.ac.cn/
 event/1/contributions/18/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/18/
END:VEVENT
BEGIN:VEVENT
SUMMARY:空间引力波探测“太极计划”
DTSTART;VALUE=DATE-TIME:20190630T030000Z
DTEND;VALUE=DATE-TIME:20190630T033000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-17@indico.itp.ac.cn
DESCRIPTION:Speakers: 乔 从丰  (中国科学院大学)\n介绍中国空
 间引力波“太极计划”研究进展状况。\n\nhttps://indico.itp.
 ac.cn/event/1/contributions/17/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/17/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Gravitational waves induced by scalar perturbations
DTSTART;VALUE=DATE-TIME:20190630T023000Z
DTEND;VALUE=DATE-TIME:20190630T030000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-16@indico.itp.ac.cn
DESCRIPTION:Speakers: 蔡 荣根 (中科院理论物理所)\nhttps://indic
 o.itp.ac.cn/event/1/contributions/16/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/16/
END:VEVENT
BEGIN:VEVENT
SUMMARY:The Quest for Neutrino Mass Ordering
DTSTART;VALUE=DATE-TIME:20190629T045000Z
DTEND;VALUE=DATE-TIME:20190629T052000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-8@indico.itp.ac.cn
DESCRIPTION:Speakers: 王 为 (中山大学)\nNeutrino mass is currently t
 he only sign of new physics beyond the Standard Model (SM) of particle phy
 sics. Unfortunately\, due to the challenges in measuring the three absolut
 e neutrino masses\, we currently only know the two mass-squared difference
 s manifested in neutrino oscillation data. The mass ordering is very likel
 y to be the first experimental handle we could have on physics related to 
 neutrino mass. A concrete experimental measurement could provide invaluabl
 e clues to the fundamental questions in particle physics. In this talk\, w
 e will give a general review on neutrino physics\, the discovery of neutri
 no oscillation and its recent experimental progresses\, and explain the di
 fferent experimental efforts of measuring neutrino mass ordering. We will 
 then focus more on the only reactor neutrino oscillation experiment resolv
 ing neutrino mass ordering: the Jiangmen Underground Neutrino Observatory 
 (JUNO)\, which takes the advantage of the powerful nuclear reactors in Gua
 ngdong Province of China. We will explain its design\, recent progresses a
 nd its physics opportunities.\n\nhttps://indico.itp.ac.cn/event/1/contribu
 tions/8/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/8/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Light Fermionic WIMP Dark Matter with Light Scalar Mediator
DTSTART;VALUE=DATE-TIME:20190629T042000Z
DTEND;VALUE=DATE-TIME:20190629T045000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-7@indico.itp.ac.cn
DESCRIPTION:Speakers: 蔡 岳霖  (中央研究院物理研究所)\nhttps:
 //indico.itp.ac.cn/event/1/contributions/7/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/7/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Effective Quintessence Potential from Landscape
DTSTART;VALUE=DATE-TIME:20190629T035000Z
DTEND;VALUE=DATE-TIME:20190629T042000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-6@indico.itp.ac.cn
DESCRIPTION:Speakers: 薛 迅 (华东师范大学/新疆大学)\nhttps://i
 ndico.itp.ac.cn/event/1/contributions/6/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/6/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Fundamental oscillation modes of self-interacting bosonic dark sta
 rs
DTSTART;VALUE=DATE-TIME:20190629T030000Z
DTEND;VALUE=DATE-TIME:20190629T033000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-5@indico.itp.ac.cn
DESCRIPTION:Speakers: 陳 樫旭 (淡江大學)\nWe perform a detailed ana
 lysis of the fundamental f-mode frequencies and damping times of nonrotati
 ng stellar-mass boson stars in general relativity by solving the nonradial
  perturbation equations. Two parameters which govern the microscopic prope
 rties of the bosonic condensates\, namely the self-coupling strength and t
 he mass of the scalar particle\, are explored. These two quantities charac
 terize oscillations of boson stars. Specifically\, we reexamine some empir
 ical relations that describe the f-mode parameters in terms of the mass an
 d radius of boson stars.\n\nhttps://indico.itp.ac.cn/event/1/contributions
 /5/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/5/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Review on Charmed Baryon Decays
DTSTART;VALUE=DATE-TIME:20190629T023000Z
DTEND;VALUE=DATE-TIME:20190629T030000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-4@indico.itp.ac.cn
DESCRIPTION:Speakers: 耿 朝强 (新竹清華大學)\nhttps://indico.itp.
 ac.cn/event/1/contributions/4/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/4/
END:VEVENT
BEGIN:VEVENT
SUMMARY:开幕式、合影
DTSTART;VALUE=DATE-TIME:20190629T020000Z
DTEND;VALUE=DATE-TIME:20190629T023000Z
DTSTAMP;VALUE=DATE-TIME:20260521T005228Z
UID:indico-contribution-1-3@indico.itp.ac.cn
DESCRIPTION:蔡荣根，蒲钔，天文台台长王娜，新大物理学
 院书记吕国梁等，\n\nhttps://indico.itp.ac.cn/event/1/contributions
 /3/
LOCATION:新疆乌鲁木齐金谷大酒店 三楼会议室
URL:https://indico.itp.ac.cn/event/1/contributions/3/
END:VEVENT
END:VCALENDAR
