V. Kadansky
RWTH Aachen University
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Featured researches published by V. Kadansky.
Physics Letters B | 1979
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; K. Lübelsmeyer; P. Mättig; H.-U. Martyn; G. Peise; J. Rimkus; H.G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; W. Korbach; P. Leu; B. Löhr; F. Roth; W. Rühmer; R. Wedemeyer; N. Wermes; M. Wollstadt; R. Buhring; R. Fohrmann
Abstract Hadron jets produced in e+e− annihilation between 13 GeV and 31.6 GeV in c.m. at PETRA are analyzed. The transverse momentum of the jets is found to increase strongly with c.m. energy. The broadening of the jets is not uniform in azimuthal angle around the quark direction but tends to yield planar events with large and growing transverse momenta in the plane and smaller transverse momenta normal to the plane. The simple q q collinear jet picture is ruled out. The observation of planar events shows that there are three basic particles in the final state. Indeed, several events with three well-separated jets of hadrons are observed at the highest energies. This occurs naturally when the outgoing quark radiates a hard noncollinear gluon, i.e., e + e − → q q g with the quarks and the gluons fragmenting into hadrons with limited transverse momenta.
Physics Letters B | 1979
R. Brandelik; J. C. Hart; J. Proudfoot; D. Heyland; H.G. Sander; E. Hilger; R. Fohrmann; Jorg Pyrlik; D. H. Saxon; W. Braunschweig; H. Hultschig; A. Ladage; P.J. Dornan; S. L. Lloyd; H.-U. Martyn; D. Revel; G. Mikenberg; H. M. Fischer; Roger J Cashmore; O. Römer; H. Boerner; D. Trines; M. Wollstadt; B. Löhr; Kenneth Watson Bell; G. Poelz; M. Ogg; Roger Barlow; D. A. Garbutt; R. Wedemeyer
Abstract We have observed e + e − hadrons at C.M. energies of 13 GeV and 17 GeV at PETRA using the TASSO detector. We find R (13 GeV) = 5.6 ± 0.7 and R (17 GeV) = 4.0 ± 0.7. The additional systematic uncertainty is 20%. Comparing inclusive charged hadron spectra we observe scaling between 5 GeV and 17 GeV for x = p / p beam > 0.2; however the 13 GeV cross section is above the 17 GeV cross section for smaller x . This may be due to copious bb production. The events become increasingly jet like at high energies as evidenced by a shrinking sphericity distribution with increasing energy.
Physics Letters B | 1980
R. Brandelik; A. Pevsner; J. Proudfoot; D. G. Cassel; D. Heyland; H.G. Sander; S. Yarker; E. Hilger; D. R. Quarrie; R. Fohrmann; Jorg Pyrlik; D. H. Saxon; W. Braunschweig; H. Hultschig; A. Ladage; P.J. Dornan; Peter Mattig; H.-U. Martyn; J.K. Sedgbeer; D. Revel; G. Mikenberg; H. M. Fischer; W. Chinowsky; O. Römer; H. Boerner; D. Trines; M. Wollstadt; B. Löhr; Kenneth Watson Bell; G. Poelz
Abstract Hadron production by e + e − annihilation has been studied for c.m. energies W between 13 and 31.6 GeV. As a function of 1n W the charged particle multiplicity grows faster at high energy than at lower energies. This is correlated with a rise in the plateau of the rapidity distribution. The cross section s d σ /d x is found to scale within ±30% for x > 0.2 and 5 ⩽ W ⩽ 31.6 GeV.
Physics Letters B | 1980
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; F. J. Kirschfink; K. Lübelsmeyer; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; L. Koepke; H. Kolanoski; P. Leu; B. Löhr; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; D. G. Cassel; D. Heyland
High-energy e+e--annihilation events obtained in the TASSO detector at PETRA have been used to determine the spin of the gluon in the reaction e+e- → qqg. We analysed angular correlations between the three jet axes. While vector gluons are consistent with the data (55% confidence limit), scalar gluons are disfavoured by 3.8 standard deviations, corresponding to a confidence level of about 10-4. Our conclusion is free of possible biases due to uncertainties in the fragmentation process or in determining the qqg kinematics from the observed hadrons.
Physics Letters B | 1980
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; K. Lübelsmeyer; P. Mättig; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; L. Koepke; H. Kolanoski; G. Knop; P. Leu; B. Löhr; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; D. G. Cassel; D. Heyland
Abstract Production of pions, kaons, protons and antiprotons has been studied in e + e − annihilations at 12 and 30 GeV centre of mass energy using time of flight techniques. The fractional yield of charged kaons and baryons appears to rise with outgoing particle momentum. At our highest energy at least 40% of e + e − annihilations into hadrons are estimated to contain baryons.
European Physical Journal A | 1980
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; K. Lübelsmeyer; P. Mättig; H.-U. Martyn; G. Peise; J. Rimkus; H.G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; P. Leu; B. Löhr; R. Wedemeyer; N. Wermes; M. Wollstadt; D. G. Cassel; D. Heyland; H. Hultschig; P. Joos; W. Koch
AbstractMeasurements ofR, sphericity and thrust are presented for c.m. energies between 12 and 31.6 GeV. A possible contribution of at
Archive | 1980
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; K. Lübelsmeyer; P. Mättig; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; L. Koepke; H. Kolanoski; G. Knop; P. Leu; B. Löhr; R. Wedemeyer; N. Wermes; M. Wollstadt; D. G. Cassel; D. Heyland; H. Hultschig
Physics Letters B | 1980
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; K. Lübelsmeyer; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; L. Koepke; H. Kolanoski; P. Leu; B. Löhr; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; D. G. Cassel; D. Heyland; H. Hultschig
\bar t
Physics Letters B | 1981
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; F. J. Kirschfink; K. Lübelsmeyer; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; L. Koepke; H. Kolanoski; P. Leu; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; D. G. Cassel; D. Heyland; H. Hultschig
Physics Letters B | 1981
R. Brandelik; W. Braunschweig; K. Gather; V. Kadansky; F. J. Kirschfink; K. Lübelsmeyer; H.-U. Martyn; G. Peise; J. Rimkus; H. G. Sander; D. Schmitz; A. Schultz von Dratzig; D. Trines; W. Wallraff; H. Boerner; H. M. Fischer; H. Hartmann; E. Hilger; W. Hillen; G. Knop; L. Koepke; H. Kolanoski; P. Leu; R. Wedemeyer; N. Wermes; M. Wollstadt; H. Burkhardt; D. G. Cassel; D. Heyland; H. Hultschig
continuum can be ruled out for c.m. energies between 16 and 31 GeV.