Study of η and η' Photoproduction at MAMI; Physical Review Letters; Vol. 118, iss. 21

מידע ביבליוגרפי
Parent link:Physical Review Letters: Scientific Journal.— , 1958-
Vol. 118, iss. 21.— 2017.— [212001, 5 p.]
מחבר תאגידי: Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
מחברים אחרים: Kashevarov V. L. Viktor Leonidovich, Ott P., Prakhov S. N., Fiks (Fix) A. I. Alexander Ivanovich
סיכום:Title screen
The reactions γp→ηp and γp→η′p are measured from their thresholds up to the center-of-mass energy W=1.96  GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section for ηphotoproduction at the energies in the vicinity of the η′ threshold, W=1896  MeV (Eγ=1447  MeV). Within the framework of a revised ηMAID isobar model, the cusp, in connection with a steep rise of the η′ total cross section from its threshold, can only be explained by a strong coupling of the poorly known N(1895)1/2− state to both ηp and η′p. Including the new high-accuracy results in the ηMAIDfit to available η and η′ photoproduction data allows the determination of the N(1895)1/2− properties.
Режим доступа: по договору с организацией-держателем ресурса
שפה:אנגלית
יצא לאור: 2017
נושאים:
גישה מקוונת:https://doi.org/10.1103/PhysRevLett.118.212001
פורמט: אלקטרוני Book Chapter
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=658141

MARC

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330 |a The reactions γp→ηp and γp→η′p are measured from their thresholds up to the center-of-mass energy W=1.96  GeV with the tagged-photon facilities at the Mainz Microtron, MAMI. Differential cross sections are obtained with unprecedented statistical accuracy, providing fine energy binning and full production-angle coverage. A strong cusp is observed in the total cross section for ηphotoproduction at the energies in the vicinity of the η′ threshold, W=1896  MeV (Eγ=1447  MeV). Within the framework of a revised ηMAID isobar model, the cusp, in connection with a steep rise of the η′ total cross section from its threshold, can only be explained by a strong coupling of the poorly known N(1895)1/2− state to both ηp and η′p. Including the new high-accuracy results in the ηMAIDfit to available η and η′ photoproduction data allows the determination of the N(1895)1/2− properties. 
333 |a Режим доступа: по договору с организацией-держателем ресурса 
461 |t Physical Review Letters  |o Scientific Journal  |d 1958- 
463 |t Vol. 118, iss. 21  |v [212001, 5 p.]  |d 2017 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
701 1 |a Kashevarov  |b V. L.  |g Viktor Leonidovich 
701 1 |a Ott  |b P. 
701 1 |a Prakhov  |b S. N. 
701 1 |a Fiks (Fix)  |b A. I.  |c Physicist  |c Professor of Tomsk Polytechnic University, Doctor of Physical and Mathematical Sciences  |f 1968-  |g Alexander Ivanovich  |3 (RuTPU)RU\TPU\pers\33830  |9 17419 
712 0 2 |a Национальный исследовательский Томский политехнический университет  |b Исследовательская школа физики высокоэнергетических процессов  |c (2017- )  |3 (RuTPU)RU\TPU\col\23551 
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