GSC 1085: Karlsruhe School of Elementary Particle and Astroparticle Physics: Science and Technology (KSETA)

GSC 1085：卡尔斯鲁厄基本粒子和天体粒子物理学院：科学与技术（KSETA）

• 批准号: 194668631
• 金额: --
• 依托单位: Scientific Computing Center (SCC)
• 依托单位国家: 德国
• 项目类别: Graduate Schools
• 财政年份: 2012
• 资助国家: 德国
• 起止时间: 2011-12-31 至 2018-12-31
• 项目状态: 已结题
• 来源: https://gepris.dfg.de/gepris/projekt/194668631?language=en
• 关键词: GSC; 1085; Karlsruhe; Elementary; Particle

The Karlsruhe School of Elementary Particle and Astroparticle Physics: Science and Technology (KSETA) is the Graduate School of the KIT Center Elementary Particle and Astroparticle Physics (KCETA). The Graduate School covers the fields of elementary particle physics, astroparticle physics and related advanced technologies. The Graduate Schools distinguishing feature is the joint doctoral research of young physicists and engineers on thesis topics centred around large-scale projects of particle and astroparticle physics. This concept builds on - and in turn strengthens - the key feature of the Karlsruhe Institute of Technology (KIT), which combines the vivid academic environment of a university with the "big science" infrastructure of a national research centre. An important characteristic of the Graduate School is the international, multicultural environment that originates from our leading participations in the AMS, Auger, Belle, Belle-II, CDF, CMS, EDELWEISS, JEM-EUSO, KASCADE and KATRIN collaborations and from the large number of foreign scientists in the KIT Center KCETA. The leitmotif of the Graduate School is the optimal training of young researchers for careers in science and industry through research within international interdisciplinary large-scale projects. The doctoral researchers may enter the Graduate School with a master or diploma degree in physics, electrical engineering, informatics/computer science or another degree qualifying her or him for research in KCETA. Our training programme for doctoral researchers follows the motto "deeper - broader - better": First, the doctoral researchers shall learn the state-of-the-art of their individual fields of research ("deeper"). Second, the Graduate School shall bridge the gaps of knowledge between physicists and engineers to build a strong basis for their common research ("broader"). We intend to open this part of the programme to external participants in form of the recurring "KSETA Topical Courses on Physics and Technology". Third, the Graduate School shall improve the individual and social skills of its members ("better"). Our preferred means of teaching are block courses, which are time-efficient and well suited to attract excellent external lecturers. We aim at an overall number of 120 doctoral researchers in the Graduate School, including those financed from other sources. KSETA builds on the decade-long experience of our 43 physicists and engineers contributing to the Graduate School. We have supervised 210 dissertations in the past five years within several coordinated programmes.

卡尔斯鲁厄基本粒子和天体粒子物理：科学与技术学院（KSETA）是卡尔斯鲁厄大学基本粒子和天体粒子物理中心（KCETA）的研究生院。研究生院涵盖基本粒子物理、天体粒子物理及相关先进技术领域。研究生院的特色是年轻物理学家和工程师围绕粒子和天体粒子物理学大型项目的论文主题进行联合博士研究。这一概念建立在卡尔斯鲁厄理工学院（KIT）的关键特征之上，并反过来加强了这一特征，它将大学生动的学术环境与国家研究中心的“大科学”基础设施相结合。研究生院的一个重要特点是国际化，多元文化的环境，这源于我们在AMS， Auger, Belle, Belle- ii， CDF， CMS， EDELWEISS, JEM-EUSO， KASCADE和KATRIN合作中的领先参与，以及KIT中心KCETA的大量外国科学家。研究生院的主题是通过国际跨学科大型项目的研究，为科学和工业领域的年轻研究人员提供最佳培训。具有物理学、电气工程、信息学、计算机科学等专业的硕士或硕士以上学历，或具有从事本中心研究工作资格的其他专业学位，可进入研究生院。我们的博士研究人员培训计划遵循“更深-更广-更好”的座右铭：首先，博士研究人员应学习各自研究领域的最新技术（“更深”）。第二，研究生院应弥合物理学家和工程师之间的知识差距，为他们的共同研究（“更广泛的”）建立坚实的基础。我们打算以定期举办的“KSETA物理与技术专题课程”的形式向外部参与者开放这部分课程。第三，研究生院应提高其成员的个人和社会技能（“更好”）。我们首选的教学方式是分组课程，这种课程既省时又适合吸引优秀的外部讲师。我们的目标是研究生院的博士研究人员总数达到120人，包括其他来源资助的研究人员。KSETA建立在我们43名物理学家和工程师为研究生院做出贡献的十年经验之上。在过去的五年里，我们在几个协调的项目中指导了210篇论文。

项目成果

Overview of Progress on the EU DEMO Reactor Magnet System Design

• DOI: 10.1109/tasc.2016.2536755
• 发表时间: 2016-03
• 期刊: IEEE Transactions on Applied Superconductivity
• 影响因子: 1.8
• 作者: L. Zani;C. Bayer;M. E. Biancolini;R. Bonifetto;P. Bruzzone;C. Brutti;D. Ciazynski;M. Coleman;I. Ďuran;M. Eisterer;W. Fietz;P. V. Gade;E. Gaio;F. Giorgetti;W. Goldacker;F. Gomory;X. Granados;R. Heller;P. Hertout;C. Hoa;A. Kario;B. Lacroix;M. Lewandowska;A. Maistrello;L. Muzzi;A. Nijhuis;F. Nunio;A. Panin;T. Petrisor;J. Poncet;R. Prokopec;M. Sanmarti Cardona;L. Savoldi;S. Schlachter;K. Sedlák;B. Stepanov;I. Tiseanu;A. Torre;S. Turtu;R. Vallcorba;M. Vojenčiak;K. Weiss;R. Wesche;K. Yagotintsev;R. Zanino

First observation of CP violation and improved measurement of the branching fraction and polarization of B0→D*+D*- decays

首次观察到 CP 破坏并改进了 B0âD* D*- 衰变的支化分数和极化的测量

• DOI: 10.1103/physrevd.86.071103
• 发表时间: 2012
• 期刊: Physical Review D
• 影响因子: 5
• 作者: The Belle Collaboration Collaboration;Adachi;I.KSETA: Kronenbitter
• 通讯作者: I.KSETA: Kronenbitter

Magnetization behavior of RE123 bulk magnets bearing twin seed-crystals in pulsed field magnetization processes

脉冲场磁化过程中带有孪晶的 RE123 块体磁体的磁化行为

• DOI: 10.1088/0953-2048/29/2/024003
• 发表时间: 2016
• 期刊: Superconductor Science and Technology
• 影响因子: 3.6
• 作者: T. Oka;T. Miyazaki;J. Ogawa;S. Fukui;T. Sato;K. Yokoyama
• 通讯作者: K. Yokoyama

Microbunching instability in relativistic electron bunches: direct observations of the microstructures using ultrafast YBCO detectors.

相对论电子束中的微聚束不稳定性：使用超快 YBCO 探测器直接观察微观结构

• DOI: 10.1103/physrevlett.113.094801
• 发表时间: 2014
• 期刊: Physical review letters
• 影响因子: 8.6
• 作者: E. Roussel;C. Evain;C. Szwaj;S. Bielawski;J. Raasch;P. Thoma;A. Scheuring;M. Hofherr;K. Ilin;S. Wünsch;M. Siegel;M. Hosaka;N. Yamamoto;Y. Takashima;H. Zen;T. Konomi;M. Adachi;S. Kimura;M. Katoh
• 通讯作者: M. Katoh

Search for PeVatrons at the Galactic Center using a radio air-shower array at the South Pole

使用南极的无线电风淋室阵列在银河系中心搜索 PeVatrons

• DOI: 10.1140/epjc/s10052-018-5537-2
• 发表时间: 2018
• 期刊: The European Physical Journal C
• 作者: A. Balagopal V;A. Haungs;T. Huege;F. G. Schröder
• 通讯作者: F. G. Schröder