guest ::
| Home > Publications database > The Algebraic method > print |
| Home > Publications database > The Algebraic method > print |
| 001 | 321045 | ||
| 005 | 20250804154241.0 | ||
| 024 | 7 | _ | |a 10.1016/S0550-3213(01)00303-0 |2 doi |
| 024 | 7 | _ | |a 0550-3213 |2 ISSN |
| 024 | 7 | _ | |a 1873-1562 |2 ISSN |
| 024 | 7 | _ | |a WOS:000171085100009 |2 WOS |
| 024 | 7 | _ | |a inspire:552700 |2 inspire |
| 024 | 7 | _ | |a openalex:W2151654771 |2 openalex |
| 037 | _ | _ | |a PUBDB-2017-02315 |
| 041 | _ | _ | |a English |
| 082 | _ | _ | |a 530 |
| 088 | 1 | _ | |a hep-ph/0102005; NYU-TH-00-09-09; CERN-TH-2001-002; DESY-01-008 |
| 088 | _ | _ | |a hep-ph/0102005 |2 arXiv |
| 088 | _ | _ | |a NYU-TH-00-09-09 |2 Other |
| 088 | _ | _ | |a CERN-TH-2001-002 |2 CERN |
| 088 | _ | _ | |a DESY-01-008 |2 DESY |
| 100 | 1 | _ | |a Grassi, P. A. |0 P:(DE-HGF)0 |b 0 |
| 245 | _ | _ | |a The Algebraic method |
| 260 | _ | _ | |a Amsterdam |c 2001 |b North-Holland Publ. Co. |
| 336 | 7 | _ | |a article |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Journal article |2 DataCite |
| 336 | 7 | _ | |a Report |0 PUB:(DE-HGF)29 |2 PUB:(DE-HGF) |m report |
| 336 | 7 | _ | |a Journal Article |b journal |m journal |0 PUB:(DE-HGF)16 |s 1497439676_468 |2 PUB:(DE-HGF) |
| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
| 336 | 7 | _ | |a JOURNAL_ARTICLE |2 ORCID |
| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a Theorie |
| 520 | _ | _ | |a Combining the effect of an intermediate renormalization prescription (zero momentum subtraction) and the background field method (BFM), we show that the algebraic renormalization procedure needed for the computation of radiative corrections within non-invariant regularization schemes is drastically simplified. The present technique is suitable for gauge models and, here, is applied to the Standard Model. The use of the BFM allows a powerful organization of the counterterms and avoids complicated Slavnov–Taylor identities. Furthermore, the Becchi–Rouet–Stora–Tyutin (BRST) variation of background fields plays a special role in disentangling Ward–Takahashi identities (WTI) and Slavnov–Taylor identities (STI). Finally, the strategy to be applied to physical processes is exemplified for the process b → sγ . |
| 536 | _ | _ | |a 899 - ohne Topic (POF3-899) |0 G:(DE-HGF)POF3-899 |c POF3-899 |f POF III |x 0 |
| 588 | _ | _ | |a Dataset connected to CrossRef, INSPIRE |
| 650 | _ | 7 | |a gauge field theory: SU(3) x SU(2) x U(1) |2 INSPIRE |
| 650 | _ | 7 | |a renormalization |2 INSPIRE |
| 650 | _ | 7 | |a background field |2 INSPIRE |
| 650 | _ | 7 | |a Ward identity |2 INSPIRE |
| 650 | _ | 7 | |a Slavnov identity |2 INSPIRE |
| 650 | _ | 7 | |a bottom: radiative decay |2 INSPIRE |
| 650 | _ | 7 | |a quantization |2 INSPIRE |
| 650 | _ | 7 | |a invariance: Becchi-Rouet-Stora |2 INSPIRE |
| 650 | _ | 7 | |a two-point function |2 INSPIRE |
| 650 | _ | 7 | |a bibliography |2 INSPIRE |
| 693 | _ | _ | |0 EXP:(DE-MLZ)NOSPEC-20140101 |5 EXP:(DE-MLZ)NOSPEC-20140101 |e No specific instrument |x 0 |
| 700 | 1 | _ | |a Hurth, T. |0 P:(DE-HGF)0 |b 1 |
| 700 | 1 | _ | |a Steinhauser, M. |0 P:(DE-HGF)0 |b 2 |
| 773 | _ | _ | |a 10.1016/S0550-3213(01)00303-0 |g Vol. B610, no. 1-2, p. 215 - 250 |0 PERI:(DE-600)1466567-0 |n 1-2 |p 215 - 250 |t Nuclear physics |v 610 |y 2001 |x 0550-3213 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/321045/files/0102005.pdf |y Restricted |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/321045/files/0102005.gif?subformat=icon |x icon |y Restricted |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/321045/files/0102005.jpg?subformat=icon-1440 |x icon-1440 |y Restricted |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/321045/files/0102005.jpg?subformat=icon-180 |x icon-180 |y Restricted |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/321045/files/0102005.jpg?subformat=icon-640 |x icon-640 |y Restricted |
| 909 | C | O | |p VDB |o oai:bib-pubdb1.desy.de:321045 |
| 913 | 1 | _ | |a DE-HGF |b Programmungebundene Forschung |l ohne Programm |1 G:(DE-HGF)POF3-890 |0 G:(DE-HGF)POF3-899 |2 G:(DE-HGF)POF3-800 |v ohne Topic |x 0 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 915 | _ | _ | |a Nationallizenz |0 StatID:(DE-HGF)0420 |2 StatID |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0300 |2 StatID |b Medline |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0501 |2 StatID |b DOAJ Seal |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0500 |2 StatID |b DOAJ |
| 915 | _ | _ | |a Creative Commons Attribution CC BY (No Version) |0 LIC:(DE-HGF)CCBYNV |2 V:(DE-HGF) |b DOAJ |
| 915 | _ | _ | |a JCR |0 StatID:(DE-HGF)0100 |2 StatID |b NUCL PHYS B : 2015 |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0200 |2 StatID |b SCOPUS |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0600 |2 StatID |b Ebsco Academic Search |
| 915 | _ | _ | |a Peer Review |0 StatID:(DE-HGF)0030 |2 StatID |b ASC |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0199 |2 StatID |b Thomson Reuters Master Journal List |
| 915 | _ | _ | |a WoS |0 StatID:(DE-HGF)0110 |2 StatID |b Science Citation Index |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)0150 |2 StatID |b Web of Science Core Collection |
| 915 | _ | _ | |a WoS |0 StatID:(DE-HGF)0111 |2 StatID |b Science Citation Index Expanded |
| 915 | _ | _ | |a DBCoverage |0 StatID:(DE-HGF)1150 |2 StatID |b Current Contents - Physical, Chemical and Earth Sciences |
| 915 | _ | _ | |a IF < 5 |0 StatID:(DE-HGF)9900 |2 StatID |
| 920 | 1 | _ | |0 I:(DE-H253)DESY_-2012_-20170516 |k DESY(-2012) |l DESY Retrocat |x 0 |
| 980 | _ | _ | |a journal |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a report |
| 980 | _ | _ | |a I:(DE-H253)DESY_-2012_-20170516 |
| 980 | _ | _ | |a UNRESTRICTED |
| Library | Collection | CLSMajor | CLSMinor | Language | Author |
|---|