BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Positivity bounds in effective field theories
DTSTART;VALUE=DATE-TIME:20190630T090000Z
DTEND;VALUE=DATE-TIME:20190630T093000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-24@indico.itp.ac.cn
DESCRIPTION:Speakers: 周 双勇  (ICTS\, USTC)\nLocality\, unitarity and 
 analyticity are some of the most fundamental properties of quantum field t
 heory. I will show how requiring a local\, analytic\, unitary UV completio
 n for a low energy effective theory (EFT) can impose positivity bounds on 
 the Wilson coefficients of the EFT. These positivity bounds take the form 
 of constraints on combinations of the pole subtracted scattering amplitude
  and its derivatives. I will first demonstrate the main idea with the simp
 le case of a massive scalar field\, and then discuss the technical subtlet
 ies that arise when generalising to cases with nonzero spins. These positi
 vity pounds can be applied to any EFTs. As an illustration\, I will apply 
 these positivity bounds to a few well-known EFTs\, including galileon\, st
 andard model effective field theory and massive gravity.\n\nhttps://indico
 .itp.ac.cn/event/1/contributions/24/
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/24/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Neutron star configurations confronting dark matter and neutron li
 fetime anomaly
DTSTART;VALUE=DATE-TIME:20190629T095000Z
DTEND;VALUE=DATE-TIME:20190629T100500Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-12@indico.itp.ac.cn
DESCRIPTION:Speakers: 楊 家威 (台灣師範大學)\nThe nature of dark 
 matter (DM) has been one of major problems in physic. The stability and ab
 undance of dark matter suggest possibility that the DM may play an importa
 nt role for compact stellar objects. Confronting the recent neutron lifeti
 me anomaly measurement in laboratories in Beam experiments and Bottle expe
 riments. We propose the neutron decays into a DM and a new scalar boson to
  resolve the anomaly. The new scalar boson and a new U(1) dark gauge symme
 try are the portals with dark sectors and visible sectors. We study the st
 ability and formation of neutron star result from the interplay between DM
  and neutrons. The DM mass and mediator mass suggest different mass-radius
  relation of the two components neutron star. We further investigate its t
 idal deformability and the corresponding gravational waveforms. The result
 s might help to reveal the nature of underlying physics in the future grav
 itational wave detection.\n\nhttps://indico.itp.ac.cn/event/1/contribution
 s/12/
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/12/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Quantum Correlation\, Coherence & Uncertainty
DTSTART;VALUE=DATE-TIME:20190701T090000Z
DTEND;VALUE=DATE-TIME:20190701T093000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-35@indico.itp.ac.cn
DESCRIPTION:Speakers: 费 少明 (首都师范大学)\nQuantum correlation
 s\, quantum coherence and quantum uncertainty relations play significant r
 oles in quantum information processing such as quantum communication and c
 omputation. The operational characterization of quantum correlations and q
 uantum coherence are also the important aspects of the corresponding resou
 rce theory. We introduce some recent results on the theory of quantum enta
 nglement\; coherence quantifier\; the relations among entanglement\, coher
 ence and particle-wave duality\; as well as the related quantum uncertaint
 y relations.\n\nhttps://indico.itp.ac.cn/event/1/contributions/35/
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/35/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Ultrahigh Energy Cosmic Rays
DTSTART;VALUE=DATE-TIME:20190701T083000Z
DTEND;VALUE=DATE-TIME:20190701T090000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-34@indico.itp.ac.cn
DESCRIPTION:Speakers: 马 伯强 (Peking University)\nI report the assoica
 tion of ultrahigh energy cosmic neutrinos with gamma ray bursts\, and from
  which on what we can obtain for the Lorentz invariance violation and CPT 
 violation.\n\nhttps://indico.itp.ac.cn/event/1/contributions/34/
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/34/
END:VEVENT
BEGIN:VEVENT
SUMMARY:xi and ˆpi as with Noncommutative Coordinates of the Quantum Phys
 ical/Phase Space
DTSTART;VALUE=DATE-TIME:20190701T080000Z
DTEND;VALUE=DATE-TIME:20190701T083000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-33@indico.itp.ac.cn
DESCRIPTION:Speakers: 江 祖永  (台灣中央大學)\nThe proper model o
 f our physical space behind quantum mechanics is the (projective) Hilbert 
 space which is also the phase space. The key difference between quantum me
 chanics and classical mechanics is just the different phase space\, an inf
 inite dimensional curved space instead of a six dimensional flat space. Th
 e latter is amazing the classical approximation of the former. We obtained
  all those results from a relativity symmetry perspective. Here\, I give a
  much more intuitive picture about that. I will discuss\, in the talk\, ho
 w the quantum physical/phase space can be seen also as a noncommutative ge
 ometry with six noncommutative coordinates and each as a quantum/noncommut
 ative observable has the information content or value of infinite number o
 f real numbers. That provide a complete resolution of the Einstein-Bohr de
 bate which Einstein probably would like. The result has important implicat
 ions for the physics and mathematics of quantum spacetime in general.\n\nh
 ttps://indico.itp.ac.cn/event/1/contributions/33/
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/33/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Dark photon enlighten by kinetic mixing
DTSTART;VALUE=DATE-TIME:20190701T052000Z
DTEND;VALUE=DATE-TIME:20190701T055000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:Thermodynamics of f (R) Gravity with Disformal Transformation
DTSTART;VALUE=DATE-TIME:20190630T105000Z
DTEND;VALUE=DATE-TIME:20190630T110500Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-26@indico.itp.ac.cn
DESCRIPTION:Speakers: 盧 致融  (台灣清華大學)\nhttps://indico.itp
 .ac.cn/event/1/contributions/26/
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/26/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Holographic entanglement entropy and its bit-thread interpretation
DTSTART;VALUE=DATE-TIME:20190630T102000Z
DTEND;VALUE=DATE-TIME:20190630T105000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-25@indico.itp.ac.cn
DESCRIPTION:Speakers: 舒 富文 (南昌大学)\nhttps://indico.itp.ac.cn/
 event/1/contributions/25/
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/25/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Thermodynamical study on universal horizons in higher $D$-dimensio
 nal spacetime and aether waves
DTSTART;VALUE=DATE-TIME:20190630T083000Z
DTEND;VALUE=DATE-TIME:20190630T090000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-23@indico.itp.ac.cn
DESCRIPTION:Speakers: 丁 持坤 (湖南人文科技学院)\nWe investigat
 e behaviors of the $D$-dimensional gravity coupled to a dynamical unit tim
 elike vector\, the aether\, present two kinds of exact charged solutions a
 nd study the linearized wave spectrum of this theory. There is an universa
 l horizon behind the Killing horizon in these aether black holes. We find 
 that in the uncharged case\, one can construct a Smarr formula and the (sl
 ightly modified) first law of black hole mechanics at the universal horizo
 ns for both kinds of black holes. An entropy can be associated with the un
 iversal horizon and a temperature can be defined there. For the second kin
 d aether black hole and for the first kind one in the extremal higher dime
 nsions\, the charge should be severely constrained that $\\bar Q\\ll \\bar
  r_0/2$. In this way\, one can still construct such first law. For aether 
 wave\, our results show that the spin-1 and spin-2 modes are the same as t
 hose in 4-dimensional spacetime\, and only the spin-0 one is different and
  dependant on the dimension number $n$.\n\nhttps://indico.itp.ac.cn/event/
 1/contributions/23/
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/23/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Charge Emission from Charged Black Holes
DTSTART;VALUE=DATE-TIME:20190630T080000Z
DTEND;VALUE=DATE-TIME:20190630T083000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-21@indico.itp.ac.cn
DESCRIPTION:Speakers: 陳 江梅 (台灣中央大學)\nThe spontaneous pai
 r production of charged scalars from near-extremal rotating\, electrically
  and/or magnetically charged black holes is discussed. Analytical expressi
 ons for pair production\, vacuum persistence and absorption cross section 
 are found\, and the spectral distribution is given a thermal interpretatio
 n. The associated holographical correspondence is confirmed at the 2-point
  function level by comparing the absorption cross section ratio as well as
  the pair production rate both from the gravity and the conformal field th
 eories. A special case of charge emission from non-extremal black hole is 
 studied.\n\nhttps://indico.itp.ac.cn/event/1/contributions/21/
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/21/
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:Charmed baryon Three-body decays with SU(3) flavor symmetry
DTSTART;VALUE=DATE-TIME:20190629T102000Z
DTEND;VALUE=DATE-TIME:20190629T103500Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-14@indico.itp.ac.cn
DESCRIPTION:Speakers: 蔡 典學 (台灣清華大學)\nhttps://indico.itp.
 ac.cn/event/1/contributions/14/
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/14/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Antitriplet charmed baryon decays with SU(3) flavor symmetry
DTSTART;VALUE=DATE-TIME:20190629T100500Z
DTEND;VALUE=DATE-TIME:20190629T102000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-13@indico.itp.ac.cn
DESCRIPTION:Speakers: 刘 佳韦 (台湾清华大学)\nhttps://indico.itp.
 ac.cn/event/1/contributions/13/
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/13/
END:VEVENT
BEGIN:VEVENT
SUMMARY:A possible connection of the broken power law between electron- an
 d proton- spectra
DTSTART;VALUE=DATE-TIME:20190629T090000Z
DTEND;VALUE=DATE-TIME:20190629T093000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-11@indico.itp.ac.cn
DESCRIPTION:Speakers: 阮 建红 (East China Normal University)\nUsing the
  gluon condensation (GC) model\, we predict a possible connection between 
 the energy spectra of electron and proton. When GC occuring\, large amount
  of gluons accumulate near the GC threshold\, this phenomenon provides a p
 ossible source of the power rule broken in the energy spectra of cosmic ra
 ys\, and also it predicts the connections between them.\n\nhttps://indico.
 itp.ac.cn/event/1/contributions/11/
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/11/
END:VEVENT
BEGIN:VEVENT
SUMMARY:暗物质与宇宙线反氦-3
DTSTART;VALUE=DATE-TIME:20190629T083000Z
DTEND;VALUE=DATE-TIME:20190629T090000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-10@indico.itp.ac.cn
DESCRIPTION:Speakers: 周 宇峰 (ITP-CAS)\nhttps://indico.itp.ac.cn/event
 /1/contributions/10/
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/10/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Prepotential approach: A unified approach to exactly\,quasi-exactl
 y\,and rationally extended solvable quantal systems
DTSTART;VALUE=DATE-TIME:20190629T080000Z
DTEND;VALUE=DATE-TIME:20190629T083000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-9@indico.itp.ac.cn
DESCRIPTION:Speakers: 何 俊麟  (淡江大學)\nWe would like to demonst
 rate how all the known 1D exactly solvable\, quasi-exactly solvable\, and 
 the recently discovered rationally extended solvable potentials\, includin
 g those related to the exceptional orthogonal polynomials\, can be constru
 cted in a direct and systematic way\, which we called the prepotential app
 roach. In this approach\, the prepotential\, the deforming function\, the 
 potential\, the eigenfunctions and eigenvalues are all derivable within th
 e same framework\, without the need of supersymmetry\, shape invariance\, 
 or Darboux-Crum transformations.\n\nhttps://indico.itp.ac.cn/event/1/contr
 ibutions/9/
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/9/
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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:20260609T131620Z
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
BEGIN:VEVENT
SUMMARY:Closing
DTSTART;VALUE=DATE-TIME:20190701T093000Z
DTEND;VALUE=DATE-TIME:20190701T100000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-36@indico.itp.ac.cn
DESCRIPTION:Speakers: 周 宇峰 ()\, 薛 迅 ()\nhttps://indico.itp.ac.cn
 /event/1/contributions/36/
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/36/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Reception
DTSTART;VALUE=DATE-TIME:20190629T120000Z
DTEND;VALUE=DATE-TIME:20190629T130000Z
DTSTAMP;VALUE=DATE-TIME:20260609T131620Z
UID:indico-contribution-1-15@indico.itp.ac.cn
DESCRIPTION:https://indico.itp.ac.cn/event/1/contributions/15/
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/15/
END:VEVENT
END:VCALENDAR