標(biāo)題: Titlebook: Cosmic Radiations: From Astronomy to Particle Physics; Giorgio Giacomelli,Maurizio Spurio,Jamal Eddine De Book 2001 Springer Science+Busin [打印本頁] 作者: Nixon 時間: 2025-3-21 17:11
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書目名稱Cosmic Radiations: From Astronomy to Particle Physics被引頻次
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書目名稱Cosmic Radiations: From Astronomy to Particle Physics讀者反饋
書目名稱Cosmic Radiations: From Astronomy to Particle Physics讀者反饋學(xué)科排名
作者: 殘忍 時間: 2025-3-21 23:02 作者: 實現(xiàn) 時間: 2025-3-22 00:36
Gravitational Wavess that will soon become operational. These detectors are based on the effect of a propagating gravitational wave to deform space in a quadrupolar form. The characteristics of the deformation are indicated in figure 1.作者: intolerance 時間: 2025-3-22 05:10
Magnetic Monopoles superheavy magnetic monopoles predicted by GUT theories. We also discuss the searches for intermediate mass monopoles (which are predicted by theories in extra dimensions), and for nuclearites and Q-balls.作者: 刺穿 時間: 2025-3-22 10:50
Monopole Catalysis of Nucleon Decay: Theory and Experimental Resultsleon decays into a lepton and one or more mesons. Here we briefly describe the physical process by which the decay takes places, then we summarize the results obtained by previous experiments, and finally we present the analysis of the MACRO. data in the search for the nucleon decay.作者: defendant 時間: 2025-3-22 15:00
Search of Slow Magnetic Monopoles with the Macro Scintillation Detectortance of ~ 10000.sr} to an isotropic flux. It employed three systems: liquid scintillation counters, streamer tubes and nuclear track detectors. The analysis presented here utilizes the scintillation counters and refers to the detection of bare GUT MM of unit Dirac magnetic charge and of 10. <β <4× 作者: defendant 時間: 2025-3-22 18:12
The Prediction of the Atmospheric Neutrino Fluxese existence of some form of “new physics” beyond the standard model. The evidence for the existence of new physics is based on the observation of three effects: (i) a measured μ/e ratio smaller that the expectation, (ii) the detection of a strong up/down asymmetry for μ-like events, and (iii) the di作者: Mortal 時間: 2025-3-22 23:25
Atmosperic Neutrinos and Neutrino Oscillations in the Macro Experimenten the acquisition was stopped. The detector has also measured 415 events with neutrino energy around 4 GeV. The data are in very good agreement with the .. → v. scenario with maximal mixing and Δm. ~ 2.4 · 10. eV.. The .. → v. oscillations with maximum mixing are disfavored at 99% CL.作者: 果仁 時間: 2025-3-23 03:41 作者: 蓋他為秘密 時間: 2025-3-23 06:27 作者: Between 時間: 2025-3-23 12:45 作者: 甜食 時間: 2025-3-23 15:03 作者: 極為憤怒 時間: 2025-3-23 18:01 作者: 刻苦讀書 時間: 2025-3-23 22:19
High Energy Neutrino Astronomy and Wimp Search Resultst larger detectors are needed. They have set upper limits on upward- going muon fluxes which have constrained models on neutrino production at cosmic sources and from WIMP-WIMP annihilation. MACRO results concerning the whole data sample collected since 1989 to December 2000, are at the moment betwe作者: MULTI 時間: 2025-3-24 04:25
The Experimental Program with the CNGS Neutrino Beamsso Laboratory located underground in central Italy 732 km from CERN. The project has been approved by CERN and INFN in 1999, the civil engineering work started in October 2000, and the commissioning is expected in the year 2005.作者: capsule 時間: 2025-3-24 08:46 作者: Campaign 時間: 2025-3-24 13:57 作者: 發(fā)現(xiàn) 時間: 2025-3-24 15:25 作者: LAVE 時間: 2025-3-24 19:56
Book 2001jectsdiscussed include the experiments on long baseline neutrino beams fromCERN to Gran Sasso and Fermilab to the Soudan mine; large underwaterand under-ice experiments; the highest energy cosmic rays;gravitational waves; and the search for new particles and newphenomena.作者: RECUR 時間: 2025-3-25 02:06
1568-2609 search projectsdiscussed include the experiments on long baseline neutrino beams fromCERN to Gran Sasso and Fermilab to the Soudan mine; large underwaterand under-ice experiments; the highest energy cosmic rays;gravitational waves; and the search for new particles and newphenomena.978-1-4020-0120-8978-94-010-0634-7Series ISSN 1568-2609 作者: 本土 時間: 2025-3-25 04:25
1568-2609 s of new results and their interpretations. new guidelinesare also set out for new developments in this and related fields.Discussions are presented of neutrino oscillations, neutrinoastronomy, high energy cosmic rays, gravitational waves, magneticmonopoles and dark matter. The future large-scale re作者: Corroborate 時間: 2025-3-25 11:33
,The Women’s Candidacy Initiative,sso Laboratory located underground in central Italy 732 km from CERN. The project has been approved by CERN and INFN in 1999, the civil engineering work started in October 2000, and the commissioning is expected in the year 2005.作者: 輕浮女 時間: 2025-3-25 11:48 作者: 熱心助人 時間: 2025-3-25 16:41 作者: 事情 時間: 2025-3-25 22:04
https://doi.org/10.1007/978-3-319-79014-5erimental consequence for electro-weak physics if the neutrino is endowed with a mass since it is very small in any case. Direct measurements yield rather strict upper bounds, namely [.]: .. < 5 eV... < 170 keV, .. < 18.2 MeV.作者: 鋼盔 時間: 2025-3-26 01:18 作者: 遵循的規(guī)范 時間: 2025-3-26 06:36 作者: 英寸 時間: 2025-3-26 11:15
Presidents Abroad: Foreign Speeches,s that will soon become operational. These detectors are based on the effect of a propagating gravitational wave to deform space in a quadrupolar form. The characteristics of the deformation are indicated in figure 1.作者: cajole 時間: 2025-3-26 16:29 作者: HOWL 時間: 2025-3-26 18:26 作者: deciduous 時間: 2025-3-26 23:36
The Egalitarian Call of the Qur’āntance of ~ 10000.sr} to an isotropic flux. It employed three systems: liquid scintillation counters, streamer tubes and nuclear track detectors. The analysis presented here utilizes the scintillation counters and refers to the detection of bare GUT MM of unit Dirac magnetic charge and of 10. <β <4× 10..作者: 相一致 時間: 2025-3-27 01:48 作者: hemorrhage 時間: 2025-3-27 08:51 作者: Mundane 時間: 2025-3-27 12:17 作者: 貧困 時間: 2025-3-27 17:16
Presidents Abroad: Foreign Speeches,in physics. They start with puzzles, with phenomena difficult to explain, and which in fact need for explanation the new physics. Are such puzzles existing now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?)作者: frenzy 時間: 2025-3-27 18:10
https://doi.org/10.1007/978-3-319-77968-3r importance has been the confirmation in 1998 by the Super-Kamiokande (SK, for short) collaboration of the zenith-angle-dependent deficit of atmospheric neutrinos. Altogether the data provide a strong evidence for .. and .. conversions, respectively. Neutrino conversions are a natural consequence o作者: 可行 時間: 2025-3-28 01:56 作者: reflection 時間: 2025-3-28 03:05
The Qur’ānic Ethic of the Marital Union superheavy magnetic monopoles predicted by GUT theories. We also discuss the searches for intermediate mass monopoles (which are predicted by theories in extra dimensions), and for nuclearites and Q-balls.作者: REP 時間: 2025-3-28 07:20 作者: 含糊 時間: 2025-3-28 11:53 作者: CRAMP 時間: 2025-3-28 17:03
The Basic Verses on Inheritancee existence of some form of “new physics” beyond the standard model. The evidence for the existence of new physics is based on the observation of three effects: (i) a measured μ/e ratio smaller that the expectation, (ii) the detection of a strong up/down asymmetry for μ-like events, and (iii) the di作者: FORGO 時間: 2025-3-28 20:54 作者: 重力 時間: 2025-3-29 02:47 作者: Airtight 時間: 2025-3-29 05:42 作者: GLEAN 時間: 2025-3-29 09:49
,The Women’s Candidacy Initiative, experiments [., ., .]. Here, we briefly describe the design and the experimental programme of the CNGS beam [.] from the CERN SPS towards the Gran Sasso Laboratory located underground in central Italy 732 km from CERN. The project has been approved by CERN and INFN in 1999, the civil engineering wo作者: 女歌星 時間: 2025-3-29 13:36 作者: 玩笑 時間: 2025-3-29 18:23
W?odzimierz Marszelewski,Bo?ena Piusthe angular distributions compared to Monte Carlo expectations (Super- Kamiokande [., .], MACRO [.-.] and Soudan 2 [.]). The usual way to interpret these data is in terms of neutrino oscillations in vacuum, in particular . ?} ... This could be possible if the flavor eigenstates do not coincide with 作者: ungainly 時間: 2025-3-29 22:30 作者: 先行 時間: 2025-3-30 01:55
https://doi.org/10.1007/978-94-010-0634-7CERN; Cross section; Dark matter; Gravity; Neutrino; Particle Physics; astronomy; astrophysics作者: parasite 時間: 2025-3-30 05:42 作者: Induction 時間: 2025-3-30 08:24 作者: 咒語 時間: 2025-3-30 16:20
Magnetic Monopoles superheavy magnetic monopoles predicted by GUT theories. We also discuss the searches for intermediate mass monopoles (which are predicted by theories in extra dimensions), and for nuclearites and Q-balls.作者: PALMY 時間: 2025-3-30 19:23
Monopole Catalysis of Nucleon Decay: Theory and Experimental Resultsleon decays into a lepton and one or more mesons. Here we briefly describe the physical process by which the decay takes places, then we summarize the results obtained by previous experiments, and finally we present the analysis of the MACRO. data in the search for the nucleon decay.作者: conjunctivitis 時間: 2025-3-30 22:03 作者: 阻擋 時間: 2025-3-31 03:05
Atmosperic Neutrinos and Neutrino Oscillations in the Macro Experimenten the acquisition was stopped. The detector has also measured 415 events with neutrino energy around 4 GeV. The data are in very good agreement with the .. → v. scenario with maximal mixing and Δm. ~ 2.4 · 10. eV.. The .. → v. oscillations with maximum mixing are disfavored at 99% CL.作者: 一個姐姐 時間: 2025-3-31 06:26
Update on Minosnts on all possible oscillation channels relevant to the atmospheric neutrino problem. Construction of the detector and the beamline are underway. Data acquisition with atmospheric neutrinos will begin in 2002 while the first beam neutrinos are expected in 2004.作者: Concrete 時間: 2025-3-31 10:41
“Exotic” Neutrino Oscillationsthe angular distributions compared to Monte Carlo expectations (Super- Kamiokande [., .], MACRO [.-.] and Soudan 2 [.]). The usual way to interpret these data is in terms of neutrino oscillations in vacuum, in particular . ?} ... This could be possible if the flavor eigenstates do not coincide with the mass eigenstates.作者: 紡織品 時間: 2025-3-31 17:02 作者: 最有利 時間: 2025-3-31 18:32
The Shared Responsibility of Men and WomenNuclear track detectors can record the passage of heavily ionizing particles like ions, magnetic monopoles and nuclearites.作者: Efflorescent 時間: 2025-3-31 21:53
The Basic Verses on InheritanceNeutrino oscillations, in a two neutrino mixing scenario, are the most likely solution for the . [.]. Underground experiments unfold the mass difference Δ.. = ... and the mixing angle θ from the measurement of the survival probability .(.. → ..) = 1 ? ..2 θ ..(1.27Δ..../..).作者: 綠州 時間: 2025-4-1 04:56
The Shared Responsibility of Men and WomenAn estimate of the energy of neutrino-induced muons is provided by a Multiple Coulomb Scattering measurement. The MACRO original upward-muon data sample has been subdivided according to the reconstructed muon energy and compared with expected fluxes. The results are interpreted in terms of neutrino oscillations.作者: hemorrhage 時間: 2025-4-1 06:05 作者: Autobiography 時間: 2025-4-1 13:09 作者: anniversary 時間: 2025-4-1 17:20
Estimate of the Energy of Upgoing Muons with Multiple Coulomb ScatteringNeutrino oscillations, in a two neutrino mixing scenario, are the most likely solution for the . [.]. Underground experiments unfold the mass difference Δ.. = ... and the mixing angle θ from the measurement of the survival probability .(.. → ..) = 1 ? ..2 θ ..(1.27Δ..../..).
