共查询到20条相似文献,搜索用时 15 毫秒
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《Physics letters. [Part B]》1986,173(1):107-110
The binary X-ray source Cyg X-3, a known gamma ray emitter, was recently seen to be emmitting a new type of neutral radiation producing muons detected in deep underground experiments. Here an explanation is offered for the deviation of the observed muon directions from that of Cyg X-3. A new underground experiment is suggested to verify the explanation. The new observations enjoying reduced backgrounds will help establish the phenomenon with enormously improved statistical significance. The nature of the neutral radiation, however, remains obscure. 相似文献
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Kochocki JA Allison WW Alner GJ Ambats I Ayres DS Balka LJ Barr GD Barrett WL Benjamin D Border P Brooks CB Cobb JH Cockerill DJ Coover K Courant H Dahlin B DasGupta U Dawson JW Edwards VW Fields TH Kirby-Gallagher LM Garcia-Garcia C Giles RH Goodman MC Heller K Heppelman S Hill N Hoftiezer JH Jankowski DJ Johns K Joyce T Kafka T Litchfield PJ Lopez FV Lowe M Mann WA Marshak ML May EN McMaster L Milburn RH Miller W Napier A Oliver WP Pearce GF Perkins DH Peterson EA Price LE Roback D Rosen DB 《Physical review D: Particles and fields》1990,42(9):2967-2973
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Becker-Szendy R Bratton CB Cady R Casper D Dye ST Gajewski W Goldhaber M Haines TJ Halverson PG Jones TW Kielczewska D Kropp WR Learned JG LoSecco JM Matsuno S McGrew C Mudan MS Price L Reines F Schultz J Sobel HW Stone JL Sulak LR Svoboda R Wittel F 《Physical review D: Particles and fields》1991,43(4):1413-1415
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《Physics letters. [Part B]》1986,174(4):441-444
The explanation of the Cygnus X-3 events which involves a strange-quark star emitting the doubly strange H dibaryon requires the H to have a lifetime of greater than ten years. We calculate the ΔS=2 H→ NN for an H bound below ΛN threshold, and find τH⪅6 days. 相似文献
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Timmer J Schwarz U Voss HU Wardinski I Belloni T Hasinger G van Der Klis M Kurths J 《Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics》2000,61(2):1342-1352
We analyze the variability in the x-ray lightcurves of the black hole candidate Cygnus X-1 by linear and nonlinear time series analysis methods. While a linear model describes the overall second order properties of the observed data well, surrogate data analysis reveals a significant deviation from linearity. We discuss the relation between shot noise models usually applied to analyze these data and linear stochastic autoregressive models. We debate statistical and interpretational issues of surrogate data testing for the present context. Finally, we suggest a combination of tools from linear and nonlinear time series analysis methods as a procedure to test the predictions of astrophysical models on observed data. 相似文献
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Amenomori M Cao Z Ding LK Feng ZY Hibino K Hotta N Huang Q Huo AX Jia HY Jiang GZ Jiao SQ Kajino F Kasahara K Labaciren Mei DM Meng L Meng XR Mimaciren Mizutani K Mu J Nanjo H Nishizawa M Nusang Oguro A Ohnishi M Ohta I Ren JR Saito T Sakata M Shi ZZ Shibata M Shirai T Sugimoto H Sun XX Tai A Taira K Tan YH Tateyama N Torii S Wang H Wen CZ Yamamoto Y Yao XY Yu GC Yuan P Yuda T Zeng JG Zhang CS Zhang HM Zhang L Zhasang Zhaxiciren Zhou WD 《Physical review letters》1992,69(17):2468-2471
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Ramon Pascual 《Zeitschrift fur Physik C Particles and Fields》1986,32(3):401-403
The possibility that the underground muons arriving from Cygnus X-3 are due to a flux of sneutrinos is analyzed. Crude approximations show that the muons can be due to a resonance production of light charged gauginos produced in sneutrino-electron collisions. 相似文献
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DING Lin-Kai HE Zuo-Xiu HUO An-Xiang JING Cai-Liu KUANG Hao-Huai LEI Yu LI Li MA Xin-Hua MA Yu-Qian QING Cheng-Rui WANG Rui-Guang YAO Zhi-Guo YU Zhong-Qiang ZHANG Chao ZHANG Feng ZHANG Jing ZHU Qing-Qi 《中国物理C(英文版)》2009,33(9)
An effort to search for Kolar-like events within the data set of the L3+C experiment is reported. From a total of 0.89×1010 triggered events there are no reliable two-prong Kolar-like events observed. The some reasonable assumptions. 相似文献
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An effort to search for Kolar-like events within the data set of the L3+C experiment is reported. From a total of 0.89×10^10 triggered events there are no reliable two-prong Kolar-like events observed. The corresponding event flux upper limit 7.1 × 10^-13 cm^-2. s^-1 . sr^-1 at 90% confidence level is deduced based on some reasonable assumptions. 相似文献