標(biāo)題: Titlebook: Current Aspects of Neutrino Physics; David O. Caldwell Book 2001 Springer-Verlag Berlin Heidelberg 2001 Beta decay.Lepton.Neutrino.Particl [打印本頁] 作者: 美麗動(dòng)人 時(shí)間: 2025-3-21 19:28
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作者: 集合 時(shí)間: 2025-3-21 23:34 作者: MORT 時(shí)間: 2025-3-22 01:25
Direct Measurements of Neutrino Mass,ly limited. There are two key questions that have important consequences at the most basic level of our understanding of neutrinos. Do neutrinos have nonzero masses? And if so, what are their mass values? The answers to these questions are important both for our theoretical understanding of fundamen作者: 赤字 時(shí)間: 2025-3-22 06:53 作者: Essential 時(shí)間: 2025-3-22 12:21
The Atmospheric Neutrino Anomaly: Muon Neutrino Disappearance,ld atmospheric neutrino anomaly moved from a possible indication of neutrino oscillations to an almost inescapable implication. In this chapter the evidence is reviewed, and indications are presented that the oscillations are probably between muon and tau neutrinos with maximal mixing. Implications 作者: Graduated 時(shí)間: 2025-3-22 13:10
Studies of Neutrino Oscillations at Reactors,roversy in the early 1980s, results from the reactors at ILL [6.2] in 1981, Goesgen [6.3] in 1986 and Bugey [6.4] in 1995 have shown no evidence for neutrino oscillations involving reactor .. More recently, the Chooz [6.5] and Palo Verde [6.6, 6.7] experiments have confirmed these findings with grea作者: Graduated 時(shí)間: 2025-3-22 20:19 作者: 我邪惡 時(shí)間: 2025-3-22 22:15 作者: BROOK 時(shí)間: 2025-3-23 04:05 作者: 我要沮喪 時(shí)間: 2025-3-23 06:07 作者: irreducible 時(shí)間: 2025-3-23 09:49 作者: FACET 時(shí)間: 2025-3-23 16:19 作者: Transfusion 時(shí)間: 2025-3-23 21:33
High Energy Neutrino Astronomy: Towards Kilometer-Scale Detectors,t cataclysmic high-energy processes. Copiously produced in high-energy collisions, traveling at the velocity of light and not deflected by magnetic fields, neutrinos meet the basic requirements for astronomy. Their unique advantage arises from a fundamental property: they are affected only by the we作者: myocardium 時(shí)間: 2025-3-24 01:39
,Pauli’s Ghost: The Conception and Discovery of Neutrinos, electron mass and . . . not larger than 0.01 proton mass.” They would be electromag-netically bound within nuclei by virtue of an anomalous magnetic moment, and they might have “about 10 times the penetrating capacity of a gamma ray.” He could account for the continuous beta decay spectrum by assum作者: CURT 時(shí)間: 2025-3-24 03:40
rties, such as structure functions and the nature of the weak interaction, at present this is not the thrust of most research and hence is not covered in this book. Rather, the topics are those currently of most interest at the frontier of particle physics.978-3-642-07424-0978-3-662-04597-8作者: 和諧 時(shí)間: 2025-3-24 07:56 作者: 大量殺死 時(shí)間: 2025-3-24 13:58
https://doi.org/10.1007/978-3-030-10644-7 electron mass and . . . not larger than 0.01 proton mass.” They would be electromag-netically bound within nuclei by virtue of an anomalous magnetic moment, and they might have “about 10 times the penetrating capacity of a gamma ray.” He could account for the continuous beta decay spectrum by assum作者: sphincter 時(shí)間: 2025-3-24 17:37 作者: cortex 時(shí)間: 2025-3-24 20:35
and scientist alike.Brings hitherto unpublished results.PoiThis is a particularly exciting time for neutrino physics. Now providing the first experimental evidence for new physics beyond the Standard Model of particle physics, neutrino studies are leading that larger field in new direc- tions. As a作者: 天文臺(tái) 時(shí)間: 2025-3-24 23:20
Anthony Aguirre,Brendan Foster,Zeeya Meralif the neutrino with other elementary-particles required to explain the nuclear beta decay observations, and neutrinos became an inseparable part of elementary particle physics. The discussion of their discovery and the rest of the history of neutrinos is the subject of the previous chapter.作者: 你敢命令 時(shí)間: 2025-3-25 06:16
Anthony Aguirre,Brendan Foster,Zeeya Meralinonzero masses? And if so, what are their mass values? The answers to these questions are important both for our theoretical understanding of fundamental interactions of nuclei and particles and because the answers have significant astrophysical and cosmological implications.作者: blithe 時(shí)間: 2025-3-25 08:18
https://doi.org/10.1007/978-3-030-11385-8eutrino oscillations involving reactor .. More recently, the Chooz [6.5] and Palo Verde [6.6, 6.7] experiments have confirmed these findings with greater sensitivity. The purpose of this chapter is to highlight the developments involving reactor neutrinos and to outline the current status and future studies.作者: 使人煩燥 時(shí)間: 2025-3-25 12:09 作者: 強(qiáng)制性 時(shí)間: 2025-3-25 17:56
Adalat Muradov,Yadulla Hasanli,Nazim Hajiyevctions suggested by Sudarshan, Marshak, Feynman and Gell-Mann; evidence for the neutral-current interactions in the early 1970s provided brilliant confirmation of the successful gauge unification of the weak and electromagnetic interactions proposed by Glashow, Salam and Weinberg.作者: multiply 時(shí)間: 2025-3-25 23:45
Adalat Muradov,Yadulla Hasanli,Nazim Hajiyevncurrently, we are undergoing a fantastic increase in the capabilities of observational astronomy, and this promises to provide new insights into the evolution of the Universe. Tantalizingly, these two great trends in science are synergistically linked, at least when it comes to neutrinos!作者: Integrate 時(shí)間: 2025-3-26 01:51
Studies in History and Philosophy of Scienceelds, neutrinos meet the basic requirements for astronomy. Their unique advantage arises from a fundamental property: they are affected only by the weakest of nature’s forces (but for gravity) and are therefore essentially unabsorbed as they travel cosmological distances between their origin and us.作者: Meditative 時(shí)間: 2025-3-26 04:24 作者: 旁觀者 時(shí)間: 2025-3-26 11:54 作者: 大方一點(diǎn) 時(shí)間: 2025-3-26 15:04
Neutrino Oscillations and the Solar Neutrino Problem,Standard Model of electroweak interactions. I shall describe the work that defined the solar neutrino problem, the likelihood that its resolution is connected with massive neutrinos and the hopes we have for future experiments.作者: 圍裙 時(shí)間: 2025-3-26 18:54 作者: 結(jié)束 時(shí)間: 2025-3-26 20:59
https://doi.org/10.1007/978-3-030-11428-2table consequences. A combination of particle physics, nuclear physics and astrophysics is needed for a full determination of the fundamental properties of neutrinos. This chapter reviews what has been achieved thus far and the future prospects for understanding the nature of neutrino masses and mixing.作者: kidney 時(shí)間: 2025-3-27 01:53
Neutrino Mixing Schemes,table consequences. A combination of particle physics, nuclear physics and astrophysics is needed for a full determination of the fundamental properties of neutrinos. This chapter reviews what has been achieved thus far and the future prospects for understanding the nature of neutrino masses and mixing.作者: FECK 時(shí)間: 2025-3-27 07:16
The Nature of Massive Neutrinos,f the neutrino with other elementary-particles required to explain the nuclear beta decay observations, and neutrinos became an inseparable part of elementary particle physics. The discussion of their discovery and the rest of the history of neutrinos is the subject of the previous chapter.作者: hidebound 時(shí)間: 2025-3-27 11:22
Direct Measurements of Neutrino Mass,nonzero masses? And if so, what are their mass values? The answers to these questions are important both for our theoretical understanding of fundamental interactions of nuclei and particles and because the answers have significant astrophysical and cosmological implications.作者: Institution 時(shí)間: 2025-3-27 17:18
Studies of Neutrino Oscillations at Reactors,eutrino oscillations involving reactor .. More recently, the Chooz [6.5] and Palo Verde [6.6, 6.7] experiments have confirmed these findings with greater sensitivity. The purpose of this chapter is to highlight the developments involving reactor neutrinos and to outline the current status and future studies.作者: 熱情贊揚(yáng) 時(shí)間: 2025-3-27 20:17 作者: Pde5-Inhibitors 時(shí)間: 2025-3-28 01:21 作者: ESPY 時(shí)間: 2025-3-28 02:37
Neutrino Flavor Transformation in Supernovae and the Early Universe,ncurrently, we are undergoing a fantastic increase in the capabilities of observational astronomy, and this promises to provide new insights into the evolution of the Universe. Tantalizingly, these two great trends in science are synergistically linked, at least when it comes to neutrinos!作者: 憂傷 時(shí)間: 2025-3-28 09:14
High Energy Neutrino Astronomy: Towards Kilometer-Scale Detectors,elds, neutrinos meet the basic requirements for astronomy. Their unique advantage arises from a fundamental property: they are affected only by the weakest of nature’s forces (but for gravity) and are therefore essentially unabsorbed as they travel cosmological distances between their origin and us.作者: glacial 時(shí)間: 2025-3-28 13:21 作者: 牲畜欄 時(shí)間: 2025-3-28 17:25
http://image.papertrans.cn/d/image/241126.jpg作者: ABASH 時(shí)間: 2025-3-28 20:24
https://doi.org/10.1007/978-3-662-04597-8Beta decay; Lepton; Neutrino; Particle Physics; Supernova; astronomy; cosmology; early universe; elementary 作者: 平躺 時(shí)間: 2025-3-29 00:32
978-3-642-07424-0Springer-Verlag Berlin Heidelberg 2001作者: Vasoconstrictor 時(shí)間: 2025-3-29 05:46 作者: Uncultured 時(shí)間: 2025-3-29 10:56 作者: 陪審團(tuán) 時(shí)間: 2025-3-29 12:36 作者: MORT 時(shí)間: 2025-3-29 19:02
Anthony Aguirre,Brendan Foster,Zeeya Merali beta decay processes since the time of their discovery. Soon after Pauli’s suggestion, Fermi wrote down the Hamiltonian describing the interactions of the neutrino with other elementary-particles required to explain the nuclear beta decay observations, and neutrinos became an inseparable part of el作者: 緩和 時(shí)間: 2025-3-29 23:09 作者: Arboreal 時(shí)間: 2025-3-30 03:33 作者: 印第安人 時(shí)間: 2025-3-30 04:02 作者: 合同 時(shí)間: 2025-3-30 08:29
https://doi.org/10.1007/978-3-030-11385-8roversy in the early 1980s, results from the reactors at ILL [6.2] in 1981, Goesgen [6.3] in 1986 and Bugey [6.4] in 1995 have shown no evidence for neutrino oscillations involving reactor .. More recently, the Chooz [6.5] and Palo Verde [6.6, 6.7] experiments have confirmed these findings with grea作者: paragon 時(shí)間: 2025-3-30 15:19
Derivation of Fronting in Turkishnciples, there is no preferred region in the Δ..-sin..parameter space, and therefore the whole has to be investigated experimentally.” Using a two-flavor oscillation, sin.. is the mixing angle giving the amplitude of the oscillation, and . determines the oscillation length, ..
