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Arthur McDonald

2026-01-31 16:33:49
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Arthur McDonald

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Arthur B McDonald, recipient of the Canadian Medal, Ontario Medal, Nova Scotia Medal, member of the Royal Society of England, registered engineer, and member of the Royal Society of Canada, was born in Sydney, Nova Scotia, Canada. McDonald holds a bachelo
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Arthur B McDonald, recipient of the Canadian Medal, Ontario Medal, Nova Scotia Medal, member of the Royal Society of England, registered engineer, and member of the Royal Society of Canada, was born in Sydney, Nova Scotia, Canada. McDonald holds a bachelor's and master's degree in physics from Dalhousie University, a doctoral degree in physics from the California Institute of Technology, and 12 honorary degrees. From 1969 to 1982, served as a researcher at the Chuck River Nuclear Laboratory of Atomic Energy Canada Limited; From 1982 to 1989, served as a professor at Princeton University; From 1989 to 2013, he served as a professor at Queen's University of Kingston in Canada and became an honorary professor in 2013. Since 1989, he has been serving as the Director of the Sudbury Neutrino Observatory's SNO. McDonald has received numerous honors, including the Canadian Medal of Honor, the 2015 Nobel Prize in Physics, and the 2016 Breakthrough in Basic Physics Award in collaboration with SNO. Currently, he is still working in the underground laboratory of the Sudbury Neutrino Observatory, actively engaged in basic research related to neutrinos and dark matter. Arthur MacDonald was born on August 29, 1943 in Sydney, Nova Scotia, Canada. He is a Canadian physicist and was awarded the 2015 Nobel Prize in Physics for discovering neutrino oscillations, which indicate that neutrinos have mass. He was also awarded the award along with Japanese physicist Kajita Takaaki. McDonald graduated from Dalhousie University with a Bachelor's and Master's degrees in Physics in 1964 and 1965, respectively. In 1969, he obtained a doctoral degree in physics from the California Institute of Technology in Pasadena. In the same year, he returned to Canada and became a postdoctoral researcher at Chalk River Nuclear Laboratories, engaged in nuclear reaction research. In 1980, he became a senior researcher and left the laboratory in 1982 to become a professor at Princeton University. In the mid-1980s, McDonald participated in the establishment of the Sudbury Neutrino Observatory, a neutrino detector located 2100 meters deep in a nickel mine in Ontario, Canada, aimed at investigating neutrinos from Earth, the Sun, and even supernovae. In 1989, he became a professor at Queens University in Canada and became the first director of the Sudbury Neutrino Observatory's SNO. The construction of the observatory began in the 1990s, with its huge plastic spherical core filled with a special liquid called a liquid scintillator. When neutrinos interact with other particles in the detector, they generate light in the liquid scintillator and are captured by extremely sensitive photomultiplier tubes. The observatory must be built deep underground to avoid pollution caused by cosmic rays, which does not hinder the passage of neutrons through the 2100 meter rock layer. There are two proposed solutions to the solar neutrino problem. One is that nuclear reactions inside the sun do not produce neutrinos

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Added: 亚瑟·B·麦克唐纳(Arthur B McDonald),加拿大勋章、安大略勋章、新斯科舍勋章获得者,英国皇家学会会员,注册工程师,加拿大皇家学会会员,出生于加拿大新斯科舍省悉尼。麦克唐纳拥有达尔豪斯大学物理学学士和硕士学位、加州理工学院物理学博士学位以及12个荣誉学位。 1969年至1982年,担任加拿大原子能有限公司查克河核实验室研究员; 1982年至1989年,任普林斯顿大学教授; 1989年至2013年,担任加拿大金斯顿女王大学教授,2013年成为名誉教授。1989年起,担任萨德伯里中微子天文台SNO主任。 McDonald 获得了众多荣誉,包括加拿大荣誉勋章、2015 年诺贝尔物理学奖以及与 SNO 合作的 2016 年基础物理突破奖。目前,他仍在萨德伯里中微子天文台地下实验室工作,积极从事中微子和暗物质相关的基础研究。亚瑟·麦克唐纳 (Arthur MacDonald) 1943 年 8 月 29 日出生于加拿大新斯科舍省悉尼。他是加拿大物理学家,因发现中微子振荡而获得2015年诺贝尔物理学奖,中微子振荡表明中微子具有质量。他还与日本物理学家梶田孝明一起获奖。麦克唐纳分别于1964年和1965年毕业于达尔豪斯大学,获得物理学学士和硕士学位。 1969年,他在帕萨迪纳市的加州理工学院获得物理学博士学位。同年返回加拿大,成为乔克河核实验室博士后研究员,从事核反应研究。 1980年成为高级研究员,1982年离开实验室成为普林斯顿大学教授。 20世纪80年代中期,麦克唐纳参与建立了萨德伯里中微子观测站,这是一座位于加拿大安大略省镍矿深处2100米的中微子探测器,旨在研究来自地球、太阳、甚至超新星的中微子。 1989年,他成为加拿大皇后大学教授,并成为萨德伯里中微子天文台SNO的首任台长。该天文台的建设始于 20 世纪 90 年代,其巨大的塑料球形核心充满了一种称为液体闪烁体的特殊液体。当中微子与探测器中的其他粒子相互作用时,它们会在液体闪烁体中产生光,并被极其灵敏的光电倍增管捕获。天文台必须建在地下深处,以避免宇宙射线造成的污染,这不会阻碍中子穿过2100米岩层。针对太阳中微子问题,有两种建议的解决方案。一是太阳内部的核反应不会产生中微子

Updated: 2026-02-24 07:32:39

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