Search for a possible spacetime correlation between high energy neutrinos and gammaray bu.pdfVIP
- 1、有哪些信誉好的足球投注网站(book118)网站文档一经付费(服务费),不意味着购买了该文档的版权,仅供个人/单位学习、研究之用,不得用于商业用途,未经授权,严禁复制、发行、汇编、翻译或者网络传播等,侵权必究。。
- 2、本站所有内容均由合作方或网友上传,本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺!文档内容仅供研究参考,付费前请自行鉴别。如您付费,意味着您自己接受本站规则且自行承担风险,本站不退款、不进行额外附加服务;查看《如何避免下载的几个坑》。如果您已付费下载过本站文档,您可以点击 这里二次下载。
- 3、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等,请点击“版权申诉”(推荐),也可以打举报电话:400-050-0827(电话支持时间:9:00-18:30)。
- 4、该文档为VIP文档,如果想要下载,成为VIP会员后,下载免费。
- 5、成为VIP后,下载本文档将扣除1次下载权益。下载后,不支持退款、换文档。如有疑问请联系我们。
- 6、成为VIP后,您将拥有八大权益,权益包括:VIP文档下载权益、阅读免打扰、文档格式转换、高级专利检索、专属身份标志、高级客服、多端互通、版权登记。
- 7、VIP文档为合作方或网友上传,每下载1次, 网站将根据用户上传文档的质量评分、类型等,对文档贡献者给予高额补贴、流量扶持。如果你也想贡献VIP文档。上传文档
查看更多
Search for a possible spacetime correlation between high energy neutrinos and gammaray bu
AA manuscript no. ASTRONOMY (will be inserted by hand later) AND Your thesaurus codes are: 03(02.05.1; 04.19.1; 13.07.1) ASTROPHYSICS Search for a possible space-time correlation between high energy neutrinos and gamma-ray bursts Montaruli T.1 and Ronga F.2 for the MACRO collaboration(∗) 1 INFN, Dipartimento di Fisica, Universit`a di Bari, via Amendola 173, I-70126, Bari, Italy 8 2 INFN, Laboratori Nazionali di Frascati, P.O. Box 13 I-00044, Frascati, Italy 9 9 1 Received February 1, 2008/ Accepted c e D Abstract. We look for space-time correlations between neutrino energy to 1019 eV, improves GRB association 2233 gamma-bursts in the Batse Catalogs and 894 with measured neutrino events in underground detectors 7 upward-going muons produced by neutrino interactions using arrival directions and times, even though expected 1 in the rock below or inside MACRO. Considering a search fluxes are much lower than atmospheric ν background. cone of 10◦ around GRB directions and a time window 1 The MACRO detector, located in the Hall B of the v of ±200 s we find 0 events to be compared to 0.035 ex- Gran Sasso underground laboratories, with a surface of 3 pected background events due to atmospheric neutrinos. 76.6 × 12 m2 and a height of 9 m, can indirectly detect 3 The corresponding upper limit (90% c.l.) is 0.87 × 10−9 neutrinos using a system of ∼ 600 ton of liquid scintilla- 3
您可能关注的文档
- MATLAB在有限差分法中的应用_熊彬.pdf
- MATLAB实验参考答案.doc
- MATLAB环境下的串口通信软件.pdf
- MATLAB算法求解微分方程数值解和解析解.ppt
- MATLAB编程在FDTD算法中的应用.pdf
- MATLAB软件在地球化学数据处理中的应用.pdf
- Matrix Elements between Nuclear Compound States and Dynamical Enhancement of the Weak Inter.pdf
- MaxwellBoltzmann分布函数的推导.doc
- MATLAB编程实现连续断层工业CT图像的三维重建_张爱东.pdf
- MBR与NF联用净化微污染水源水研究.pdf
- Search for a Ridge Structure Origin with Shower Broadening and Jet Quenching.pdf
- Search for Baryonic Resonances Decaying to Xi pi in DeepInelastic Scattering at HERA.pdf
- Search for Baryonic Resonances Decaying to Xi ssin DeepInelastic Scattering at HERA.pdf
- Search for charged Higgs decays of the top quark using hadronic tau decays.pdf
- Search for compositeness and leptophobic gauge bosons (with polarized beams).pdf
- Search for Correlations between Nearby AGNs and Ultrahigh Energy Cosmic Rays.pdf
- Search for Cosmic Axions using an Optical Interferometer.pdf
- Search for Doublycharged Higgs Boson Production in the Decay H++H mu+mu+mumu with th.pdf
- Search for Fermion Actions on Hyperdiamond Lattices.pdf
- Search for Hidden Dimensions in Run I Tevatron Data.pdf
文档评论(0)