不如屎壳郎 发表于 2025-4-1 02:59:13

C. de Marzo,M. de Palma,C. Favuzzi,G. Maggi,E. Nappi,F. Posa,A. Ranieri,G. Selvaggi,P. Spinelli,A. Butions to rate or differential equations. However, often we need to do just the opposite, to differentiate or find the slope or rate of change of a variable. The main reason that we would want to find a rate of change in STELLA II is to be able to identify the maximum or minimum value of a variable.

HUMP 发表于 2025-4-1 06:24:22

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发微光 发表于 2025-4-1 10:28:00

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脱水 发表于 2025-4-1 15:40:48

D. Treilleutions to rate or differential equations. However, often we need to do just the opposite, to differentiate or find the slope or rate of change of a variable. The main reason that we would want to find a rate of change in STELLA II is to be able to identify the maximum or minimum value of a variable.

泛滥 发表于 2025-4-1 21:23:08

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FLIRT 发表于 2025-4-2 02:04:36

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查看完整版本: Titlebook: QCD Hard Hadronic Processes; Bradley Cox (Chairman) Book 1988 Springer Science+Business Media New York 1988 Boson.CERN.Lepton.Particle Phy