標題: Titlebook: QCD Hard Hadronic Processes; Bradley Cox (Chairman) Book 1988 Springer Science+Business Media New York 1988 Boson.CERN.Lepton.Particle Phy [打印本頁] 作者: T-cell 時間: 2025-3-21 18:46
書目名稱QCD Hard Hadronic Processes影響因子(影響力)
書目名稱QCD Hard Hadronic Processes影響因子(影響力)學科排名
書目名稱QCD Hard Hadronic Processes網(wǎng)絡公開度
書目名稱QCD Hard Hadronic Processes網(wǎng)絡公開度學科排名
書目名稱QCD Hard Hadronic Processes被引頻次
書目名稱QCD Hard Hadronic Processes被引頻次學科排名
書目名稱QCD Hard Hadronic Processes年度引用
書目名稱QCD Hard Hadronic Processes年度引用學科排名
書目名稱QCD Hard Hadronic Processes讀者反饋
書目名稱QCD Hard Hadronic Processes讀者反饋學科排名
作者: 暗指 時間: 2025-3-21 20:58
Preliminary Results from CDF on ,,, Production at the Tevatron Collider series of papers to be published.(Reference2) The full detector was operational for the 1987 Collider run with the exception of the higher level triggers and half of the sampling layers in the forward hadron calorimeters.作者: 膽大 時間: 2025-3-22 01:27 作者: 材料等 時間: 2025-3-22 07:51 作者: Collision 時間: 2025-3-22 12:05
Direct Photons at Large ,, from Hadronic Collisions: A Short Review Based on the QCD Analysis Beyond for proton induced production one has to note the large coverage in .(20 – 630GeV) and . (5 – 80GeV/.). although the experiments are rather difficult because of the low rates, e.g. prompt photon/hadronic jet < ...作者: 軌道 時間: 2025-3-22 14:00 作者: 中止 時間: 2025-3-22 18:50 作者: 言行自由 時間: 2025-3-23 00:42 作者: mosque 時間: 2025-3-23 02:31 作者: acrophobia 時間: 2025-3-23 06:13 作者: GLUE 時間: 2025-3-23 10:18
Direct Photon Production in pp and ,p Collisionsce .q annihilation is clearly more important in .p than pp, due to the valence . quarks, R is expected to be larger than one, and since the gluon structure function is known to be relatively soft so that .q should become increasingly favoured over qg as p. increases, R is expected to increase with the p. of the emitted gamma ray.作者: 高興一回 時間: 2025-3-23 15:56 作者: DECRY 時間: 2025-3-23 21:50 作者: 面包屑 時間: 2025-3-24 00:45
QCD in the Limit , → 1 as Studied in the Reaction π,, → ,,,,,f quarks in pions allows us the study the QCD subprocess . → .... in the kinematic limit . → 1. The data are consistent with many of the features of a higher-twist analysis, particulary the departure of the muon-pair angular distribution from the standard form 1+cos.... Analysis of .) and .’ product作者: Rct393 時間: 2025-3-24 06:17
Summary of Direct Lepton Session and Round Tablere some differences between the E615 and the NA10 cross sections for Drell-Yan at large .. Experiment and theory disagree on the angular distribution of the muons. In the round table discussion, most of the time went to discussing the question of whether experiments should or should not make a corre作者: Neutropenia 時間: 2025-3-24 09:20
Direct Photons at Large ,, from Hadronic Collisions: A Short Review Based on the QCD Analysis Beyondse momentum (.)”. Indeed since then an impressive number of experiments. confirmed the production of prompt photons in hadronic collisions. Especially for proton induced production one has to note the large coverage in .(20 – 630GeV) and . (5 – 80GeV/.). although the experiments are rather difficult作者: MODE 時間: 2025-3-24 11:48 作者: 凹處 時間: 2025-3-24 16:29 作者: Breach 時間: 2025-3-24 19:13 作者: 沙文主義 時間: 2025-3-25 01:07 作者: milligram 時間: 2025-3-25 03:50 作者: falsehood 時間: 2025-3-25 08:20 作者: ANTIC 時間: 2025-3-25 12:44
Certain Uncertainties in QCD Theory Predictions for Large-,, Photons and Other Processesng coupling ..(.) (related with the renormalization procedure), and the factorization scale . entering the structure functions .(.,.) (determining the scale violations). Until recently, for large transverse momentum ..) processes, simplicity suggested the choice . where α = positive and of 0(1), or 作者: 燦爛 時間: 2025-3-25 16:39
Direct Photons at the CERN ISRjet and study of the recoil jet will thus be a study of quark fragmentation. Further, it would be expected that there will be no accompanying (same-side) jet, and a measurement of the direct photon cross section will measure the gluon structure function in the interacting protons (modulo soft gluon 作者: Collar 時間: 2025-3-25 22:41
Book 1988 theoretical developments in the particular area and concluded with a round table which discussed the various information presented in the course of the discussions. A session of the workshop was devoted to the direct production of high transverse momentum photons in hadronic interactions. Data from作者: chandel 時間: 2025-3-26 02:17 作者: paltry 時間: 2025-3-26 05:37
W. C. Carithersapproach is not suitable to model the longitudinal correlations. The book has exploited the random effects carefully only to model the correlations of the familial data. Subsequently, this book has modelled the correlations of the longitudinal data collected from the members of a large number of ind作者: Overstate 時間: 2025-3-26 10:43
Kirk T. McDonaldapproach is not suitable to model the longitudinal correlations. The book has exploited the random effects carefully only to model the correlations of the familial data. Subsequently, this book has modelled the correlations of the longitudinal data collected from the members of a large number of ind作者: 串通 時間: 2025-3-26 16:03 作者: irradicable 時間: 2025-3-26 20:24
Flavio Costantinihe econometric profiles in the forefront of dynamic modelling. For this purpose, we decided to add a new section where the reader can find the stochastic rationale of vector autoregressive specifications in econometrics. The third (and last) chapter improves on that of the first edition by re- ing t作者: Barter 時間: 2025-3-27 00:53 作者: Spinal-Fusion 時間: 2025-3-27 02:26 作者: 未成熟 時間: 2025-3-27 05:44 作者: Palpate 時間: 2025-3-27 09:30 作者: mucous-membrane 時間: 2025-3-27 13:38
Ewald Paulsired condition has been found. For example, we may be modeling a firm that attempts to maximize its profits. We will start the firm off with a low output per time period and calculate the corresponding profit. Then, we incrementally increase output over time, thereby increasing revenues from sale o作者: 事物的方面 時間: 2025-3-27 20:07
Bernard G. Popesired condition has been found. For example, we may be modeling a firm that attempts to maximize its profits. We will start the firm off with a low output per time period and calculate the corresponding profit. Then, we incrementally increase output over time, thereby increasing revenues from sale o作者: Lamina 時間: 2025-3-28 01:38 作者: 輕信 時間: 2025-3-28 03:56 作者: WAG 時間: 2025-3-28 08:54 作者: gusher 時間: 2025-3-28 13:04 作者: 打包 時間: 2025-3-28 14:34 作者: Dungeon 時間: 2025-3-28 19:48
A. P. Contogourisd condition has been found. For example, we may be modeling a firm that attempts to maximize its profits. We will start the firm off with a low output per time period and calculate the corresponding profit. Then we incrementally increase output over time, thereby increasing revenues from sale ofthat作者: 代理人 時間: 2025-3-28 23:24 作者: 金絲雀 時間: 2025-3-29 05:43 作者: POLYP 時間: 2025-3-29 08:00
Klaus Freudenreiche random effects carefully only to model the correlations of the familial data. Subsequently, this book has modelled the correlations of the longitudinal data collected from the members of a large number of ind978-1-4614-2801-5978-1-4419-8342-8Series ISSN 0172-7397 Series E-ISSN 2197-568X 作者: intimate 時間: 2025-3-29 13:21 作者: 織物 時間: 2025-3-29 16:55 作者: chemoprevention 時間: 2025-3-29 23:35 作者: 有組織 時間: 2025-3-30 01:18
W. C. Caritherssting books, this book uses a class of auto-correlation structures to model the longitudinal correlations for the repeated discrete data that accommodates all possible Gaussian type auto-correlation models as special cases including the equi-correlation models. This new dynamic modelling approach is作者: 輕推 時間: 2025-3-30 06:56 作者: collagen 時間: 2025-3-30 12:11 作者: Insufficient 時間: 2025-3-30 13:08
J. C. Collins,K. Freudenreichsting books, this book uses a class of auto-correlation structures to model the longitudinal correlations for the repeated discrete data that accommodates all possible Gaussian type auto-correlation models as special cases including the equi-correlation models. This new dynamic modelling approach is作者: 安裝 時間: 2025-3-30 17:35
Rudolf Baieries.Step by step guidance to a thorough understanding.IncludThis second edition sees the light three years after the first one: too short a time to feel seriously concerned to redesign the entire book, but sufficient to be challenged by the prospect of sharpening our investigation on the working of 作者: 粗魯?shù)娜?nbsp; 時間: 2025-3-30 22:19
Flavio Costantiniicient to be challenged by the prospect of sharpening our investigation on the working of econometric dynamic models and to be inclined to change the title of the new edition by dropping the “Topics in” of the former edition. After considerable soul searching we agreed to include several results rel作者: Carcinogen 時間: 2025-3-31 02:26
P. T. Coxons to rate or differential equations. However, often we need to do just the opposite, to differentiate or find the slope of a curve or rate of change of a variable. The main reason that we would want to find a rate of change in STELLA is to be able to identify the maximum or minimum value of a vari作者: 觀察 時間: 2025-3-31 05:43 作者: 責怪 時間: 2025-3-31 09:38 作者: llibretto 時間: 2025-3-31 16:43
Beno?t Moursons to rate or differential equations. However, often we need to do just the opposite, to differentiate or find the slope of a curve or rate of change of a variable. The main reason that we would want to find a rate of change in STELLA is to be able to identify the maximum or minimum value of a vari作者: 東西 時間: 2025-3-31 19:50 作者: 亞當心理陰影 時間: 2025-3-31 22:40 作者: 不如屎殼郎 時間: 2025-4-1 02:59
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.作者: HUMP 時間: 2025-4-1 06:24 作者: 發(fā)微光 時間: 2025-4-1 10:28 作者: 脫水 時間: 2025-4-1 15:40
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.作者: 泛濫 時間: 2025-4-1 21:23 作者: FLIRT 時間: 2025-4-2 02:04
