英语词汇“neutrino”的意思、用法、释义、翻译、读音、例句、短语、词组-英语词典

是什么意思

中微子；

变形

复数：neutrinos

英英释义

neutrino

n.an elementary particle with zero charge and zero mass

学习怎么用

双语例句

用作名词(n.)

This is the solar neutrino problem.
这便是著名的太阳中微子难题。
Neutrino physics is a hot topic in current research in fundamental science.
中微子物理是当今基础研究的一个热点。

权威例句

Neutrino oscillations in matter
Neutrino Mass and Spontaneous Parity Nonconservation
Searching For Dark Matter with Neutrino Telescopes
Direct Evidence for Neutrino Flavor Transformation from Neutral‐Current Interactions in SNO
Direct Evidence for Neutrino Flavor Transformation from Neutral〤urrent Interactions in SNO;
Measurement of the solar electron neutrino flux with the Homestake Chloring detector
Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam.
First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory
The Soft Gamma Repeaters as Very Strongly Magnetized Neutron Stars. II. Quiescent Neutrino, X-Ray, and Alfvén Wave Emission

单词	neutrino
释义	neutrino 听听怎么读英 [nju:?tri:n??] 美 [nu?trino?] 是什么意思 n. 中微子；变形复数：neutrinos 英英释义 neutrino n.an elementary particle with zero charge and zero mass 学习怎么用双语例句用作名词(n.) This is the solar neutrino problem. 这便是著名的太阳中微子难题。 Neutrino physics is a hot topic in current research in fundamental science. 中微子物理是当今基础研究的一个热点。权威例句 Neutrino oscillations in matter Neutrino Mass and Spontaneous Parity Nonconservation Searching For Dark Matter with Neutrino Telescopes Direct Evidence for Neutrino Flavor Transformation from Neutral‐Current Interactions in SNO Direct Evidence for Neutrino Flavor Transformation from Neutral〤urrent Interactions in SNO; Measurement of the solar electron neutrino flux with the Homestake Chloring detector Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam. First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance Direct evidence for neutrino flavor transformation from neutral-current interactions in the Sudbury Neutrino Observatory The Soft Gamma Repeaters as Very Strongly Magnetized Neutron Stars. II. Quiescent Neutrino, X-Ray, and Alfvén Wave Emission
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