A Generator of QCD Parton Model for the Study of Cosmic Ray Ultrahigh Energy Interactions

Cao Zhen; Ding Linkai

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1994, Vol. 18> Issue(11) : 961-969

A Generator of QCD Parton Model for the Study of Cosmic Ray Ultrahigh Energy Interactions

Cao Zhen ^, ,
Ding Linkai

Institute of High Energy Physics,Academia Sinica,Beijing,100039

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Abstract：
A parton model based on perturbative QCD is developed for the description of ultrahigh energy interaction between cosmic rays and air nuclei.A LLA QCD calculation of jet production cross sections in proton-proton scattering and a hadronization scheme based on independent fragmentation model are presented.A number of parameters in the hadronization scheme are so selected that the basic features of hadronic production in e⁺e^－ collision covering C.M.energy region from 14 GeV to 91 GeV can be reproduced. A Monte Carlo generator is constructed to reproduce the basic characteristics of proton-antiproton scattering in the C.M.energy region from 60 GeV to 1800 GeV and to extrapolate smoothly to ultrahigh energy region extending to 22 TeV.

References

[1]

C.M.C.Lattes et al,Phys.Rep,65（1980）151.[2]J.R.Ren et al,Phys.Rev,D38（1988）1404.[3]汪敬儒等，高能物理与核物理，13（1989）77990.[4]Q.Q.Zhuetal.,J.Phys,G16（1990）295.[5]曹臻、丁林垲，高能物理与核物理，18（1994）990.[6]Siegried Betkke,CERN-PPE/91-36.[7]MarfinJ.G.and Tung W.K.Z.Phys,G52（1991）13.[8]R.P.Feynman,R.D.Field and G.C.Fox,Phys.Rev,D18（1978）3320.[9]UA1Coll,G.Arnison et al,Phys.Lett,172B（1986）461.[10]CDF Call,Fermilab-conf,90/91-E.[11]UA2 Coll,J.Alitti.etal,PhysLett,257B（1991）232.[12]UA1 Coll,Nucl.Phys.B309（1988）405.[13]F.Halzen,Proc.21st Intl.Cosmic Ray Conf.Adelaide,12（1990）101.[14]M.Bentsson and T.Sjostrand,Phys Lett,185B（1987）435.[15]T.Sjostrand and M.Bentsson,Comput.Phys.Comm,43（1987）367.[16]G.AltariliandG.Parisi,Nucl.Phys,B126（1977）298.[17]A.Alietal,DESY Internal Report T-80/01.[18]Mark-ⅡColl.,Pettersen et al.,Phys.Rev.,D37（1988）1.[19]TASSO Coll.,M.Alth off et al.,Z.Phys.,C22（1984）307;TASSO Coll.,W.Braunschwerg et al.,Z.Phys.,C45（1989）193.[20]ALEPH Coll,D.Decahpetal,PhysLett,234B（1990）209.[21]May Coll,Y.K.Lietal,Phys.Rev,D41（1990）2675;MayColl,H.W.Zhangetal,Phys.Rev,D42（1990）737.

[1]	LUO Shi-Yu , SHAO Ming-Zhu , HU Xi-Duo . Interaction of Charged Particles with Superlattice, and Identification of Particles with Ultra-high Energy. Chinese Physics C, 2007, 31(3): 320-323.
[2]	BAI Yun-Xiang , XIAO Gang , CAO Zhen . Performance of CRTNT Fluorescence Light Detector for Sub-EeV Cosmic Ray Observation. Chinese Physics C, 2006, 30(9): 824-827.
[3]	LUO Yan-An , PAN Feng , NING Ping-Zhi , Jerry P . SD-Pair Shell Model and Proton-Neutron Interacting Boson Model. Chinese Physics C, 2004, 28(S1): 87-89.
[4]	PENG Qiu-He . Where Do the Extra High Energy Cosmic Rays Come From A Model of Active Galactic Nuclei With Magnetic Monopoles. Chinese Physics C, 2002, 26(S1): 104-111.
[5]	FENG CunFeng , ZHANG XueYao , KONG FanMin , HE Mao , FU Yu , DAI ZhiQiang , ZHANG NaiJian . Relation between Interactive Models and Identification of Primary Cosmic Ray Components at the “Knee”. Chinese Physics C, 2000, 24(6): 467-472.
[6]	Xu Chunxian , Dai Hongyue . A Statistic Model for Galactic Cosmic Rays. Chinese Physics C, 1997, 21(6): 486-493.
[7]	DENG Wei-Zhen , YANG Ze-Sen , WANG Yu-Cheng . A Non-Hermitian Approach of Dyson Boson Expansion to Interacting Boson Model. Chinese Physics C, 1993, 17(10): 907-911.
[8]	FAN Xiao-Ling , ZHANG Chun-Sheng . Application of Hadron-Hadron Nuclear Interaction Parametrization Model in the Study of Superhigh Energy Cosmic Rays. Chinese Physics C, 1992, 16(4): 289-296.
[9]	DING Lin-Kai . ON THE INELASTICITY OF SUPERHIGH ENERGY COSMIC RAY INTERACTIONS. Chinese Physics C, 1990, 14(6): 486-489.
[10]	WANG Yun-Xin . ENERGY SPECTRUM OF SUPER HIGH ENERGY COSMIC RAY MUON SHOWERS OF LARGE ZENITH ANGLES. Chinese Physics C, 1986, 10(2): 245-248.
[11]	ZOU Bao-Tang , WANG Cheng-Rui , REN Jing-Ru . A COSMIC RAY SUPER HIGH ENERGY MULTIJET FAMILY EVENT. Chinese Physics C, 1986, 10(4): 393-399.
[12]	DI Yao-Min . F-SPIN BREAKING IN IBM. Chinese Physics C, 1985, 9(4): 461-466.
[13]	YANG Ze-Sen(Tse-sen Yang) . DYSON'S BOSON EXPANSION AND THE INTERACTING BOSON MODEL. Chinese Physics C, 1985, 9(3): 341-348.
[14]	ZHU Pei-Yu , CAO Yu-Fang , WU You-Shi . THE SPIN (6) LIMIT OF INTERACTING BOSON-FERMION MODEL Ⅱ. Chinese Physics C, 1985, 9(2): 154-160.
[15]	ZHANG Chun-Sheng , REN Jing-Ru , KUANG Hao-Huai , LU Sui-Ling , LI Ming-Xiang , SU Shi , WANG Yun-Xin , WANG Dian-Chen , FAN Hai-Kun , XUE Yong-Gui , HUO An-Xiang . A STUDY ON THE CHARACTERISTICS OF COSMIC RAY HADRONS AT MT. KAMBALA. Chinese Physics C, 1985, 9(6): 649-652.
[16]	XU Chun-Xian . THE ANISOTROPY OF COSMIC RAY PARTICLES IN THE ENERGY RANGE 10¹¹—10¹⁹eV. Chinese Physics C, 1985, 9(4): 385-390.
[17]	XU Gong-Ou , YANG Ya-Tian , GU Jin-Nan . COMPARISON BETWEEN THE BOHR-MOTTELSON MODEL AND THE INTERACTING BOSON MODEL. Chinese Physics C, 1984, 8(3): 352-360.
[18]	ZHANG XI-ZHEN , LI CHU-HSIA , . INTERACTING BOSON-FERMION MODEL AND. Chinese Physics C, 1982, 6(3): 347-354.
[19]	WU RUA-CHUAN . INTERACTING BOSON MODEL FOR ROTATIONAL STATES OF NEGATIVE PARITY. Chinese Physics C, 1982, 6(5): 601-608.
[20]	HUO AN-XIANG , REN JING-RU , LU SUI-LING , KUANG HAO-HUAI , SU SHI , WANG CHENG-RUI , CAO PEI-YUAN , LI JIN-YU . THE ENERGY SPECTRA OF COSMIC RAY HADRONS AT MT.KAMBALA 5500m ABOVE SE LEVEL. Chinese Physics C, 1982, 6(6): 778-780.

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Cao Zhen and Ding Linkai. A Generator of QCD Parton Model for the Study of Cosmic Ray Ultrahigh Energy Interactions[J]. Chinese Physics C, 1994, 18(11): 961-969.

Cao Zhen and Ding Linkai. A Generator of QCD Parton Model for the Study of Cosmic Ray Ultrahigh Energy Interactions[J]. Chinese Physics C, 1994, 18(11): 961-969. shu

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Received: 1900-01-01
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

A Generator of QCD Parton Model for the Study of Cosmic Ray Ultrahigh Energy Interactions

Cao Zhen ^,
Ding Linkai

Corresponding author: Cao Zhen,

Institute of High Energy Physics,Academia Sinica,Beijing,100039

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1994-11-05

Abstract: A parton model based on perturbative QCD is developed for the description of ultrahigh energy interaction between cosmic rays and air nuclei.A LLA QCD calculation of jet production cross sections in proton-proton scattering and a hadronization scheme based on independent fragmentation model are presented.A number of parameters in the hadronization scheme are so selected that the basic features of hadronic production in e⁺e^－ collision covering C.M.energy region from 14 GeV to 91 GeV can be reproduced. A Monte Carlo generator is constructed to reproduce the basic characteristics of proton-antiproton scattering in the C.M.energy region from 60 GeV to 1800 GeV and to extrapolate smoothly to ultrahigh energy region extending to 22 TeV.