时间:9月12日,周三,19:00-20:30

地点:玉泉园区,教学楼,阶一6教室

报告题目:知心系列讲座:正念减压,提高幸福感

     正念减压疗法是基于名为“正念”修心养性的方法,借助系统化的方法,正念训练帮助练习者培养清晰的洞察力和理解力。在个人身心健康方面,正念训练着重让练习者做自己的主人,通过不断的练习、探索与体验,了解心灵与身体的相互关系,从而更好地照顾与爱护自己。麻省大学与全球采用正念减压疗法的医学中心,在三十年来的科学研究证明,正念疗法的修炼,能深远地影响参与者,让他们减少疾病,身心更加健康,生活更加自在与丰盛。

主讲人:刘兴华副教授

     北京大学心理学系临床心理学博士毕业,现任首都师范大学应用心理研究所副所长,中国心理学会临床与自信专业委员会委员,首都医科大学临床心理系系务委员会委员。从事正念训练的研究以及开展对于临床病人和正常人的正念干预,已发表相关论文多篇。

主办:国科大心里健康教育中心

承办:国科大心理协会

报告题目:A HIGH-ENERGY REVOLUTION IN THE SKY

报告人:Prof. G.F. Bignami 

主持人:张双南 研究员

时间:2012年9月13日(周四)上午10:00

地点:高能所化学楼三楼阶梯教室C305

 

报告内容简介 

It all started 50 years ago, as soon as space astronomy came of age. X-ray astronomy started in 1962, with the first detection of an extrasolar X-ray source, ScoX-1. The first gamma-ray map of the sky, produced by OSO-3, was published in 1972 when the SAS-2 satellite was launched.

Now are are living through a golden age of high-energy astrophysics with a very successful series of X-and gamma-ray observatories operational in orbit. The accomplishements of XMM-Newton, Chandra, Integral, Swift, Agile and Fermi will be highlighted with special enphasis on the recent results on Neutron Stars (NSs)

NSs emit the vast majority of their energy in gamma-rays, more so than in X-rays. Not only that: after the first case of Geminga, the Fermi Observatory is telling us  that many, maybe the majority, of NSs in our Galaxy emit only in gamma-rays and are invisible at other wavelengths. Such a high-energy revolution will lead us to the understanding of NS physics. 

 

报告人简介

G.F. Bignami is a well-known professor of Astronomy, Istituto Universitario di Studi Superiori, Pavia, and an Associate Scientist, INAF, Milan, Italy. He is the current president of COSPAR, the largest international organization on space research. 2003-2007: Director of the Centre d’Etude Spatiale des Rayonnements, an “Unitè Mixte de Recherche” of the French CNRS and of the University of Toulouse. 2004-2007: Chair of ESA’s Space Science Advisory Committee.

2007-2009: President of the Italian Space Agency.

2009-now: President of the Scientific Council of the “Groupment d’Interet Scientifique” called “Physique des deuxInfinis”, composed by 19 astronomy and physics Institutes in the Ile de France region around Paris.

 

欢迎参加!!!

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报告题目:The Dark Side of the Universe

报 告 人:Edward W. Kolb(University of Chicago)

主 持 人:王贻芳所长

时 间:2012年9月4(周二)下午3:00

地 点:高能所主楼C305会议室

 

报告内容简介

Ninety-five percent of the universe is missing!  Astronomical observations suggest that most of the mass of the universe is in a mysterious form called dark matter and most of the energy in the universe is in an even more mysterious form called dark energy. Unlocking the secrets of dark matter and dark energy will illuminate the nature of space and time and connect the quantum with the cosmos.

 

报告人简介

Edward W. Kolb, usually known as Rocky Kolb, is a cosmologist and a professor at the University of Chicago. He has worked on many aspects of the big bang cosmology, including baryogenesis, nucleosynthesis and dark matter. He is author, with Michael Turner, of the popular textbook The Early Universe (Addison-Wesley, 1990). Additionally, alongside his co-author Michael Turner, Kolb was awarded the 2010 Dannie Heineman Prize for Astrophysics.

 

高能所科研计划处、党政联合办、研究生部

2012年8月29日

6th International Conference on Nanotoxicology

September 4-7,2012,Beijing Friendship Hotel, Beijing, China

 

Nature Nanotechnology session

Nature Nanotechnology currently does not have any formal guidelines or requirements for reporting nanotoxicology papers specifically and we have received feedback from our authors/readers asking for these. Our position is that characterization should be done based on relevance to the study but there are a number of parameters that are quite standard and should be included in all papers. The aim of this 2 hr session, which consists of four speakers, is to consult the community so a formal set of characterization requirements for reporting nanotoxicology papers can be established. Nature Nanotechnology will offer to disseminate this information and/of revise our Guide to Authors. Please join the dialogue.

 

Data: September 5, 2012

Time: 2:00-4:00 pm

Venue: Room 1, Second Floor, Rui Bin(building No,7), Friendship Hotel

2012年9月5日,下午2:00-4:00,北京友谊宾馆,瑞宾楼,2层,1号会议室

Speakers:

1. Justin Teeguarden, Pacific Northwest National Laboratory

2. Michael Winchester, National Institute of standards and Technology

3. Rick Pleus, Intertox Inc. representing ISO/TC 229

4. Hakan Wallin, Editor-in-chief of nanotoxicology

 

Moderator: Ai Lin Chun, Senior Editor nature Nanotechnology

*please visit poster”0” in conference room2, Ruibin(Building No. 7)for a draft of the Guidelines for reporting Nanotoxicology Research. Comments and feedback welcomed at 该Email地址已收到反垃圾邮件插件保护。要显示它您需要在浏览器中启用JavaScript。 (closing date: November 30, 2012)

 

This 6th international Conference on Nanotoxicology, September 4-7, 2012, Beijing, China

Contact information: Conference Chair, Prof. Yuliang Zhao; 该Email地址已收到反垃圾邮件插件保护。要显示它您需要在浏览器中启用JavaScript。

Secretary General, Prof. Chunying Chen; 该Email地址已收到反垃圾邮件插件保护。要显示它您需要在浏览器中启用JavaScript。; 该Email地址已收到反垃圾邮件插件保护。要显示它您需要在浏览器中启用JavaScript。

 

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报告题目:The EXO Double-beta Decay Program
报 告 人:Prof. Giorgio Gratta ( Stanford University, USA)
主 持 人:王贻芳 所长
时 间:2012年8月22日(周四)上午10:30
地 点:高能所化学楼三楼阶梯教室


报告内容简介
Prof. Giorgio Gratta will present new results from the EXO-200 experiment that has been taking low background data for a first year and plans to run for up to 5 years. EXO-200 discovered the 2 neutrino double-beta decay in 136Xe in the first 2 months of operation and is now attacking the more interesting neutrinoless double beta decay mode.
Prof. Giorgio Gratta will also discuss the R&D for a future, larger detector and the plans towards the construction of such a detector.


报告人简介
Prof. Giorgio Gratta got his PH.D from university of Rome (Italy) in 1986, then was elected as a fellow in Italian Institute for Nuclear Research during 1987-1989, as a research fellow in Caltech during 1989-1992 and as a senior research fellow in Caltech during 1992-1995.Then he was an associate professor in Stanford during 1995-2004 and as a professor in Stanford since 2005.
His research interests are research relevant to the understanding of fundamental particles and interactions. His group is operating the largest double-beta decay experiment in the world (EXO-200) that is producing high sensitivity results on the mass of neutrinos and on the question of whether or not neutrinos are described by a 4-component wave function like all other fermions (neutrinos may be “Majorana” particles, described by 2-component wave functions, instead of Dirac particles.)
Also within the EXO program they are developing a new method to extend the sensitivity of a future experiment. This work involves the identification of the Ba atom produced in the double-beta decay of Xe using AMO techniques.
They also have a program to develop imaging detectors for gamma-ray astronomy as well as novel radiation detectors for application in homeland security and medical physics.