期刊文献+
共找到2篇文章
< 1 >
每页显示 20 50 100
Mechanical properties of friction stir welded armor grade Al-Zn-Mg alloy joints 被引量:6
1
作者 c.sharma V.UPADHYAY +1 位作者 D.K.DWIVEDI P.KUMAR 《Transactions of Nonferrous Metals Society of China》 SCIE EI CAS CSCD 2017年第3期493-506,共14页
The influence of different welding speeds and rotary speeds on the formation and mechanical properties of friction stirweld joints of armor grade aluminum alloy was presented.The developed weld joints were characteriz... The influence of different welding speeds and rotary speeds on the formation and mechanical properties of friction stirweld joints of armor grade aluminum alloy was presented.The developed weld joints were characterized by bend tests,micro-hardness tests,tensile tests,optical and scanning electron microscopies.Mechanical properties(i.e.,micro-hardness,ultimatetensile strength and elongation to fracture)increased with the increase in rotary speed or decrease in welding speed.The effect ofwelding speed on micro-hardness of heat affected zones was more profound than the rotary speeds.The welding speeds and rotaryspeeds influenced the mechanical properties and their effects on various mechanical properties of the friction stir welded joints canbe predicted with the help of regression models. 展开更多
关键词 friction stir welding welding parameters mechanical properties FRACTOGRAPHY regression modeling
在线阅读 下载PDF
Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle Ⅱ experiment
2
作者 I.Adachi L.Aggarwal +407 位作者 H.Ahmed J.K.Ahn H.Aihara N.Akopov A.Aloisio N.Althubiti N.Anh Ky D.M.Asner H.Atmacan T.Aushev V.Aushev M.Aversano R.Ayad V.Babu H.Bae S.Bahinipati P.Bambade Sw.Banerjee M.Barrett J.Baudot A.Baur A.Beaubien F.Becherer J.Becker J.V.Bennett F.U.Bernlochner V.Bertacchi M.Bertemes E.Bertholet M.Bessner S.Bettarini B.Bhuyan F.Bianchi L.Bierwirth T.Bilka D.Biswas A.Bobrov D.Bodrov J.Borah A.Boschetti A.Bozek P.Branchini T.E.Browder A.Budano S.Bussino Q.Campagna M.Campajola L.Cao G.Casarosa C.Cecchi J.Cerasoli M.-C.Chang P.Chang R.Cheaib P.Cheema B.G.Cheon K.Chilikin K.Chirapatpimol H.-E.Cho K.Cho S.-J.Cho S.-K.Choi S.Choudhury J.Cochran L.Corona J.X.Cui S.Das E.De La Cruz-Burelo S.A.De La Motte G.de Marino G.De Nardo G.De Pietro R.de Sangro M.Destefanis S.Dey R.Dhamija A.Di Canto F.Di Capua J.Dingfelder Z.Doležal I.Domínguez Jiménez T.V.Dong K.Dort D.Dossett S.Dubey K.Dugic G.Dujany P.Ecker D.Epifanov J.Eppelt P.Feichtinger T.Ferber T.Fillinger C.Finck G.Finocchiaro A.Fodor F.Forti A.Frey B.G.Fulsom A.Gabrielli E.Ganiev M.Garcia-Hernandez R.Garg G.Gaudino V.Gaur A.Gaz A.Gellrich G.Ghevondyan D.Ghosh H.Ghumaryan G.Giakoustidis R.Giordano A.Giri P.Gironella B.Gobbo R.Godang O.Gogota P.Goldenzweig W.Gradl E.Graziani D.Greenwald Z.Gruberová T.Gu K.Gudkova I.Haide S.Halder Y.Han K.Hara T.Hara C.Harris K.Hayasaka H.Hayashii S.Hazra C.Hearty M.T.Hedges A.Heidelbach I.Heredia de la Cruz M.Hernández Villanueva T.Higuchi M.Hoek M.Hohmann R.Hoppe P.Horak C.-L.Hsu T.Humair T.Iijima K.Inami N.Ipsita A.Ishikawa R.Itoh M.Iwasaki W.W.Jacobs D.E.Jaffe E.-J.Jang Q.P.Ji S.Jia Y.Jin A.Johnson K.K.Joo H.Junkerkalefeld M.Kaleta D.Kalita J.Kandra K.H.Kang G.Karyan T.Kawasaki F.Keil C.Kiesling C.-H.Kim D.Y.Kim J.-Y.Kim K.-H.Kim Y.-K.Kim Y.J.Kim H.Kindo K.Kinoshita P.Kodyš T.Koga S.Kohani K.Kojima A.Korobov S.Korpar E.Kovalenko R.Kowalewski P.Križan P.Krokovny T.Kuhr R.Kumar K.Kumara A.Kuzmin Y.-J.Kwon S.Lacaprara Y.-T.Lai K.Lalwani T.Lam L.Lanceri J.S.Lange M.Laurenza K.Lautenbach R.Leboucher M.J.Lee C.Lemettais P.Leo D.Levit P.M.Lewis C.Li L.K.Li S.X.Li W.Z.Li Y.Li Y.B.Li Y.P.Liao J.Libby J.Lin M.H.Liu Q.Y.Liu Z.Q.Liu D.Liventsev S.Longo T.Lueck C.Lyu Y.Ma M.Maggiora S.P.Maharana R.Maiti S.Maity G.Mancinelli R.Manfredi E.Manoni M.Mantovano D.Marcantonio S.Marcello C.Marinas C.Martellini A.Martens A.Martini T.Martinov L.Massaccesi M.Masuda K.Matsuoka D.Matvienko S.K.Maurya J.A.McKenna R.Mehta F.Meier M.Merola C.Miller M.Mirra S.Mitra K.Miyabayashi G.B.Mohanty S.Mondal S.Moneta H.-G.Moser R.Mussa I.Nakamura M.Nakao Y.Nakazawa M.Naruki D.Narwal Z.Natkaniec A.Natochii M.Nayak G.Nazaryan M.Neu C.Niebuhr S.Nishida S.Ogawa Y.Onishchuk H.Ono P.Pakhlov G.Pakhlova E.Paoloni S.Pardi K.Parham H.Park J.Park K.Park S.-H.Park B.Paschen A.Passeri S.Patra T.K.Pedlar R.Peschke R.Pestotnik L.E.Piilonen G.Pinna Angioni P.L.M.Podesta-Lerma T.Podobnik S.Pokharel C.Praz S.Prell E.Prencipe M.T.Prim H.Purwar P.Rados G.Raeuber S.Raiz N.Rauls M.Reif S.Reiter M.Remnev L.Reuter I.Ripp-Baudot G.Rizzo S.H.Robertson M.Roehrken J.M.Roney A.Rostomyan N.Rout S.Sandilya L.Santelj Y.Sato V.Savinov B.Scavino M.Schnepf C.Schwanda A.J.Schwartz Y.Seino A.Selce K.Senyo J.Serrano C.Sfienti W.Shan c.sharma C.P.Shen X.D.Shi T.Shillington T.Shimasaki J.-G.Shiu D.Shtol B.Shwartz A.Sibidanov F.Simon J.B.Singh J.Skorupa R.J.Sobie M.Sobotzik A.Soffer A.Sokolov E.Solovieva W.Song S.Spataro B.Spruck M.Starič P.Stavroulakis S.Stefkova R.Stroili Y.Sue M.Sumihama K.Sumisawa W.Sutcliffe N.Suwonjandee H.Svidras M.Takahashi M.Takizawa U.Tamponi K.Tanida F.Tenchini A.Thaller O.Tittel R.Tiwary E.Torassa K.Trabelsi I.Ueda K.Unger Y.Unno K.Uno S.Uno P.Urquijo Y.Ushiroda S.E.Vahsen R.van Tonder K.E.Varvell M.Veronesi A.Vinokurova V.S.Vismaya L.Vitale V.Vobbilisetti R.Volpe A.Vossen M.Wakai S.Wallner E.Wang M.-Z.Wang Z.Wang A.Warburton S.Watanuki C.Wessel E.Won X.P.Xu B.D.Yabsley S.Yamada W.Yan S.B.Yang J.Yelton J.H.Yin K.Yoshihara C.Z.Yuan L.Zani B.Zhang V.Zhilich J.S.Zhou Q.D.Zhou X.Y.Zhou V.I.Zhukova R.Zlebcík The Belle Ⅱ Collaboration 《Chinese Physics C》 2025年第1期7-18,共12页
series of data samples was collected with the Belle Ⅱ detector at the SuperKEKB collider from March 2019 to June 2022.We determine the integrated luminosities of these data samples using three distinct methodologies ... series of data samples was collected with the Belle Ⅱ detector at the SuperKEKB collider from March 2019 to June 2022.We determine the integrated luminosities of these data samples using three distinct methodologies involving Bhabha(e^(+)e^(-)→e^(+)e^(-)(ny),digamma(e^(+)e^(-)→γγ(nγ),and dimuon(e^(+)e^(-)→μ^(+)μ^(-)(nγ)events.The total integrated luminosity obtained with Bhabha,digamma,and dimuon events is(426.88±0.03±2.61)fb^(-1),(429.28±0.03±2.62)fb^(-1),and(423.99±0.04±3.83)fb^(-1),where the first uncertainties are statistical and the second are systematic.The resulting total integrated luminosity obtained from the combination of the three methods is(427.87±2.01)fb^(-1). 展开更多
关键词 integrated luminosity Bhabha digamma dimuon BelleⅡ
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部