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Branes, Fluxes and Duality in M(atrix)-Theory
We use the T-duality transformation which relates M-theory on T^3 to M-theory on a second T^3 with inverse volume to test the Banks-Fischler-Shenker-Susskind suggestion for the matrix model description of M-theory. We find evidence that T-duality is realiz
hep-th/9611202,PUPT-1668
Branes,FluxesandDualityinM(atrix)-Theory
arXiv:hep-th/9611202v3 10 Dec 1996OriJ.Ganor,SanjayeRamgoolamandWashingtonTaylorIVDepartmentofPhysics,JadwinHallPrincetonUniversityPrinceton,NJ08544,USAoriga,ramgoola,wati@puhep1.princeton.eduWeusetheT-dualit
Models of solar energetic particle fluxes- the main requirements and development prospects
航天,航天器,航天器环境,空间辐射
AdvancesinSpaceResearch36(2005)
2003–2011
/locate/asr
Modelsofsolarenergeticparticle uxes:Themainrequirements
andthedevelopmentprospects
N.V.Kuznetsov,R.A.Nymmik*,M.I.Panasyuk
SkobeltsynInstituteofNuclearPhysics,MoscowStateUniversity,VorobjovyGory,Moscow119992,Russia
Received19October2002;receivedinrevisedform5May2003;accepted27September2004
Abstract
Themodelsofsolarenergeticparticles(SEP)areintendedforcalculatingtheproton uencesandpeak uxes,whichareexpectedtooccurforagivenperiodatanyknownorpredictedsolaractivitylev
Models of solar energetic particle fluxes- the main requirements and development prospects
航天,航天器,航天器环境,空间辐射
AdvancesinSpaceResearch36(2005)
2003–2011
/locate/asr
Modelsofsolarenergeticparticle uxes:Themainrequirements
andthedevelopmentprospects
N.V.Kuznetsov,R.A.Nymmik*,M.I.Panasyuk
SkobeltsynInstituteofNuclearPhysics,MoscowStateUniversity,VorobjovyGory,Moscow119992,Russia
Received19October2002;receivedinrevisedform5May2003;accepted27September2004
Abstract
Themodelsofsolarenergeticparticles(SEP)areintendedforcalculatingtheproton uencesandpeak uxes,whichareexpectedtooccurforagivenperiodatanyknownorpredictedsolaractivitylev
Fluxes of atmospheric muons underwater depending on the small-x gluon density
The prompt muon contribution to the deep-sea atmospheric muon flux can serve as a tool for probing into the small-x feature of the gluon density inside of a nucleon, if the muon energy threshold could be lifted to 100 TeV. The prompt muon flux underwater i
3
002 ebF 02 1v3812030/hp-pe:hviXraFluxesofatmosphericmuonsunderwaterdependingonthesmall-xgluondensity
AMisaki1,TSSinegovskaya2,SISinegovsky2andNTakahashi3
1WasedaUniversity,Okubo3-4-1,Shinjuku-ku,Tokyo,169-8555Japan2IrkutskStateUniversity,664003Russia3
HirosakiUniversity,036