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SU(3) ISOSCALAR FACTORS AND RePReSeNTATION MATRICeS

Chinese Physics C 2014年第9期38卷 506-506页

作者： K.A.Olive K.Agashe C.Amsler M.Antonelli J.-F.Arguin D.M.Asner H.Baer H.R.Band R.M.Barnett T.Basaglia C.W.Bauer J.J.Beatty v.I.Belousov J.Beringer G.Bernardi S.Bethke H.Bichsel O.Biebe e.Blucher S.Blusk G.Brooijmans O.Buchmueller v.Burkert M.A.Bychkov R.N.Cahn M.Carena A.Ceccucci A.Cerr D.Chakraborty M.-C.Chen R.S.Chivukula K.Copic G.Cowan O.Dahl G.D'Ambrosio T.Damour D.de Florian A.de Gouvea T.deGrand P.de Jong G.Dissertor B.A.Dobrescu M.Doser M.Drees H.K.Dreiner D.A.edwards S.eidelman J.erler v.v.ezhela W.Fetscher B.D.Fields B.Foster A.freitas T.K.Gaisser H.Gallagher L.Garren H.-J.Gerber G.Gerbier T.Gershon T.Gherghetta S.Golwala M.Goodman C.Grab A.v.Gritsan C.Grojean D.e.Groom M.Grnewald A.Gurtu T.Gutsche H.e.Haber K.Hagiwara C.Hanhart S.Hashimoto Y.Hayato K.G.Hayes M.Heffner B.Heltsley J.J.Hernandez-Rey K.Hikasa A.Hocker J.Holder A.Holtkamp J.Huston J.D.Jackson K.F.Johnson T.Junk M.Kado D.Karlen U.F.Katz S.R.Klein e.Klempt R.v.Kowalewski F.Krauss M.Kreps B.Krusche Yu.v.Kuyanov Y.Kwon O.Lahav J.Laiho P.Langacker A.Liddle Z.Ligeti C.-J.Lin T.M.Liss L.Littenberg K.S.Lugovsky S.B.Lugovsky F.Maltoni T.Mannel A.v.Manohar W.J.Marciano A.D.Martin A.Masoni J.Matthews D.Milstead P.Molaro K.Monig F.Moortgat M.J.Mortonson H.Murayama K.Nakamura M.Narain P.Nason S.Navas M.Neubert P.Nevski Y.Nir L.Pape J.Parsons C.Patrignani J.A.Peacock M.Pennington S.T.Petcov Kavli IPMU A.Piepke A.Pomarol A.Quadt S.Raby J.Rademacker G.Raffel B.N.Ratcliff P.Richardson A.Ringwald S.Roesler S.Rolli A.Romaniouk L.J.Rosenberg J L.Rosner G.Rybka C.T.Sachrajda Y.Sakai G.P.Salam S.Sarkar F.Sauli O.Schneider K.Scholberg D.Scott v.Sharma S.R.Sharpe M.Silari T.Sjostrand P.Skands J.G.Smith G.F.Smoot S.Spanier H.Spieler C.Spiering A.Stahl T.Stanev S.L.Stone T.Sumiyoshi M.J.Syphers F.Takahashi M.Tanabashi J.Terning L.Tiator M.Titov N.P.Tkachenko N.A.Tornqvist D.Tovey G.valencia G.venanzoni M.G.vincter P.vogel A.vogt S.P.Wakely W.Walkowiak C.W.Walter D.R.Ward G.Weiglein D.H.Weinberg e.J.Weinberg M.White L.R.Wiencke C.G.Wohl L.Wolfenstein J.Womersley C.L. University of Minnesota School of Physics and Astronomy116 Church St.S.E.MinneapolisMN 55455USA University of Maryland Department of PhysicsCollege ParkMD 20742-4111USA Albert einstein Center for Fundamental Physics Universitat BernCH-3012 BernSwitzerland Lab.Nazionali di Frascati dell'INFN CP 13via E.Fermi40I-00044 Frascati(Roma)Italy departement de physique Universite de MontrealC.P.6128succ.centre-villeMontreal(Quebec) H3C 3J7Canada Pacific Northwest National Laboratory 902 Battelle BoulevardRichlandWA 99352USA department of Physics and Astronomy University of OklahomaNormanOK 73019USA department of Physics University of WisconsinMadisonWI 53706USA Physics Division Lawrence Berkeley National Laboratory1 Cyclotron RoadBerkeleyCA 94720USA CeRN European Organization for Nuclear ResearchCH-1211 Geneve 23Switzerland department of Physics The Ohio State University191 W.Woodruff Ave.ColumbusOH 43210 COMPAS Group Institute for High Energy PhysicsRU- 142284ProtvinoRussia LPNHe IN2P3-CNRS et Universites de Paris 6 et 7F-75252 ParisFrance Max-Planck-Institute of Physics 80805 MunichGermany department of Physics University of WashingtonSeattleWA 98195USA Ludwig-Maximilians-Universitat Fakultdt für PhysikSchellingstr.4D-80799 MünchenGermany enrico Fermi Institute and department of Physics University of ChicagoChicagoIL 60637-1433USA department of Physics Syracuse UniversitySyracuseNY13244USA department of Physics Columbia University538 W.120th StreetNew YorkNY10027 USA High energy Physics Group Blackett LaboratoryImperial CollegePrince Consort RoadLondon SW7 2AZUK Jefferson Lab 12000 Jefferson Ave.Newport NewsVA 23606USA department of Physics University of VirginiaPO Box 400714CharlottesvilleVA 22904USA Fermi National Accelerator Laboratory P.O.Box 500BataviaIL 60510USA Kavli Institute for Cosmological Physics University of ChicagoChicagoIL 60637-1433USA department of Physics and Astronomy University of SussexFalmerBrighton BN1 9QHUK department o

Written by R.L. Kelly （LBNL）. The most commonly used SU（3） isoscalar factors, corresponding to the singlet, octet, and deeuplet content of 8 8 and 10 8, are shown at the right. The notation uses particle names to identify the coefficients, so that the pattern of relative couplings may be seen at a glance. We illustrate the use of the coefficients below.

关键词： eK SU ISOSCALAR FACTORS AND RePReSeNTATION MATRICeS

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INTeRNATIONAL SYSTeM OF UNITS(SI)

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Chinese Physics C 2014年第9期38卷 112-112页

See ＂The International System of Units （SI）,＂ NIST Special Publication 330, B.N. Taylor, ed. （USGPO, Washington, DC, 1991）; and ＂Guide for the Use of the International System of Units （SI）,＂ NIST Special Pub... 详细信息

关键词： SI NIST INTeRNATIONAL SYSTeM OF UNITS

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SU(n) MULTIPLeTS AND YOUNG DIAGRAMS

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Chinese Physics C 2014年第9期38卷 507-507页

Written by C.G. Wohl （LBNL）. This note tells （1） how SU（n） particle multiplets are identified or labeled, （2） how to find the number of particles in a multiplet from its label, （3） how to draw the Young diagram for a multiplet, and （4） how to use Young diagrams to determine the overall multiplet structure of a composite system, such as a 3-quark or a meson-baryon system.

关键词： SU MULTIPLeTS AND YOUNG DIAGRAMS than

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HIGHLIGHTS OF THe 2014 eDITION OF THe RevIeW OF PARTICLe PHYSICS

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Chinese Physics C 2014年第9期38卷 5-5页

899 new papers with 3283 new measurements Over 330 papers from LHC experiments （ATLAS, CMS, and LHCb）.

关键词： LHC

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PeRIODIC TABLe OF THe eLeMeNTS

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Chinese Physics C 2014年第9期38卷 113-113页

Table *** 2011 by ***（LBNL）,and ***.

关键词： UIP CN PeRIODIC TABLe OF THe eLeMeNTS SI ST

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NeUTRINO BeAM LINeS AT HIGH-eNeRGY PROTON SYNCHROTRONS

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Chinese Physics C 2014年第9期38卷 397-397页

Revised September 2013 with numbers verified by representatives of the synchrotrons （contact C.-J. Lin, LBNL）. For existing （future） neutrino beam lines the latest achieved （design） values are given.

关键词： Graphite eu Be In CeRN Target NeUTRINO BeAM LINeS AT HIGH-eNeRGY PROTON SYNCHROTRONS

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CLeBSCH-GORDAN COeFFICIeNTS,SPHeRICAL HARMONICS,AND d FUNCTIONS

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Chinese Physics C 2014年第9期38卷 505-505页

Note： A square-root sign is to be understood over every coefficient, e.g., for -8/15 read - √8√15.

关键词： CLeBSCH-GORDAN COeFFICIeNTS SPHeRICAL HARMONICS AND d FUNCTIONS

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Residual Feed Intake as a Measure to Select Genetically Productive Beef Cattle: A Review

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Journal of Agricultural Science and Technology(B) 2020年第2期10卷 118-123页

作者： Tiago Neves Pereira valente Andréia Santos Cezário Wallacy Barbacena Rosa dos Santos Jeferson Corrêa Ribeiro eliandra Maria Bianchini Oliveira erico da Silva Lima Bruno Borges deminicis Thasia Martins Macedo Rogério de Carvalho veloso department of Animal Science Instituto Federal Goiano(IFGoiano)Campus PossePosse City73900-000Goiás StateBrasil department of Animal Science Instituto Federal Goiano(IFGoiano)Campus MorrinhosMorrinhos City75650-000Goiás StateBrasil department of Animal Science Faculdades Metropolitanas Unidas(FMU)São Paulo City05607-000São Paulo StateBrazil department of Animal Science Federal University of Southern Bahia(UFSB-BA)Teixeira de Freitas City45613-204Bahia StateBrazil

Measures such as residual feed intake(RFI)have been increasingly considered to select cattle with superior feed efficiency,as it is a characteristic of feed efficiency calculated as the difference between observed intake and estimated intake considering metabolic weight and the weight *** feed intake is obtained through the multiple regression equation of observed consumption on metabolic mean live weight and weight *** standard was shared among animals into one herd selected for low RFI(high efficiency)and compared to the one selected for high RFI(low efficiency).There was no correlated response in weight per year and in weight gain,and the effectiveness of low RFI selection in reducing feed costs was proven without affecting ***,selection of animals with negative RFI is not done by selecting animals directly according to the size of the viscera,rather it is done indirectly,that is,when selecting the most efficient animals and normally these animals already have the smallest viscera *** RFI is a trait that presents genetic variability,selectable to improve and has moderate heritability,between 0.30 and *** RFI is important because it reduces the direct economic impacts of reduced feed intake,as well as the effects of environmental impact on reducing methane emissions from enteric fermentation of ruminants.

关键词： Feed conversion feed efficiency enteric fermentation

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