国家自然科学基金(11203018)

作品数：5被引量：0H指数：0
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相关机构：新疆大学更多>>
相关期刊：《中国西部科技》《Chinese Physics C》《Research in Astronomy and Astrophysics》更多>>
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The optical/UV excess of X-ray-dim isolated neutron star Ⅱ.Nonuniformity of plasma on a strangeon star surface
《Research in Astronomy and Astrophysics》2018年第7期81-92,共12页Wei-Yang Wang Yi Feng Xiao-Yu Lai Yun-Yang Li Ji-Guang Lu Xuelei Chen Ren-Xin Xu 
support of MoST(2016YFE0100300);the National Natural Science Foundation of China(NSFC,Nos.11473044,11633004,11653003);CAS(QYZDJ-SSW-SLH017);supported by the Open Project Program of the Key Laboratory of FAST,Chinese Academy of Sciences(CAS);supported by the West Light Foundation(XBBS-2014-23); NSFC(No.11203018);supported by NSFC(No.11225314);the Open Project Program of the Key Laboratory of Radio Astronomy,CAS;supported by the National Key R&D Program of China(No.2017YFA0402602);NSFC(Nos.11673002 and U1531243);the Strategic Priority Program of CAS(No.XDB23010200);supported by Special Funding for Advanced Users,budgeted and administrated by the Center for Astronomical Mega-Science,Chinese Academy of Sciences(CAMS).
Several X-ray-dim isolated neutron stars （XDINSs）, also known as the Magnificent Seven, exhibit a Planck-like soft X-ray spectrum. In the optical/ultraviolet （UV） band, there is an excess of radiation compared to ...
关键词：X-rays stars - stars neutron - stars individual 
Spontaneous magnetization of solid quark-cluster stars
《Chinese Physics C》2016年第9期75-81,共7页来小禹 徐仁新 
Supported by 973 Program(2012CB821801);West Light Foundation(XBBS-2014-23);National Natural Science Foundation of China(11203018,11225314,11365022);Science Project of Universities in Xinjiang(XJEDU2012S02);Doctoral Science Foundation of Xinjiang University(BS120107)
Pulsar-like compact stars usually have strong magnetic fields, with strengths from -10^8 to -10^12 G on the surface. How such strong magnetic fields can be generated and maintained is still an unsolved problem,which i...
关键词：PULSARS strange stars magnetic fields 
Small glitches: the role of strange nuggets?
《Research in Astronomy and Astrophysics》2016年第3期91-98,共8页Xiao-Yu Lai Ren-Xin Xu 
supported by the National Natural Science Foundation of China (11203018);the West Light Foundation (XBBS-2014-23);the Science Project of Universities in Xinjiang (XJEDU2012S02);the Doctoral Science Foundation of Xinjiang University (BS120107)
Pulsar glitches, i.e. the sudden spin-ups of pulsars, have been detected for most known pulsars.The mechanism giving rise to this kind of phenomenon is uncertain, although a large data set has been built.In the framew...
关键词：pulsars -- glitches -- quark-cluster stars -- strange nuggets 
A corresponding-state approach to quark-cluster matter
《Chinese Physics C》2014年第5期38-47,共10页郭彦君 来小禹 徐仁新 
Supported by National Basic Research Program of China(2012CB821800);National Natural Science Foundation of China(11225314,11203018);National Fund for Fostering Talents of Basic Science(NFFTBS)(J1030310/J1103205)
The state of super-dense matter is essential for us to understand the nature of pulsars; however, non- perturbative quantum chromodynamics makes it very difficult to make direct calculations of the state of cold matte...
关键词：PULSARS neutron stars elementary particles 
如何培养学习物理的兴趣
《中国西部科技》2013年第3期101-102,106,共3页来小禹 
中国自然科学基金(11203018);新疆维吾尔自治区高校科研计划(XJEDU2012S02)
提高学生的学习兴趣是教师应当首要关心的问题。本文阐述了在物理教学的过程中可能影响学生物理学习兴趣的一些因素,例如教师的作用,课堂教学的生动和启发性,教师对课堂教学节奏的控制,以及在讲课中穿插讲一些科学故事的作用。
关键词：物理教学 学习兴趣 
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