The Belle II physics book › Обзор исследований

Standard

The Belle II physics book. / Belle II Collaboration; Эйдельман, Семен Исаакович; Кроковный, Павел Петрович и др.

в: Progress of Theoretical and Experimental Physics, Том 2019, № 12, ARTN 123C01, 12.2019.

Результаты исследований: Научные публикации в периодических изданиях › обзорная статья › Рецензирование

Harvard

Belle II Collaboration, Эйдельман, СИ, Кроковный, ПП & Ремнев, МА 2019, 'The Belle II physics book', Progress of Theoretical and Experimental Physics, Том. 2019, № 12, ARTN 123C01. https://doi.org/10.1093/ptep/ptz106

APA

Belle II Collaboration, Эйдельман, С. И., Кроковный, П. П., & Ремнев, М. А. (2019). The Belle II physics book. Progress of Theoretical and Experimental Physics, 2019(12), [ARTN 123C01]. https://doi.org/10.1093/ptep/ptz106

Vancouver

Belle II Collaboration, Эйдельман СИ, Кроковный ПП , Ремнев МА. The Belle II physics book. Progress of Theoretical and Experimental Physics. 2019 дек.;2019(12):ARTN 123C01. doi: 10.1093/ptep/ptz106

Author

Belle II Collaboration ; Эйдельман, Семен Исаакович ; Кроковный, Павел Петрович и др. / The Belle II physics book. в: Progress of Theoretical and Experimental Physics. 2019 ; Том 2019, № 12.

BibTeX

@article{182539c61a8d483883a420e923441e54,

title = "The Belle II physics book",

abstract = "The Belle II detector will provide a major step forward in precision heavy flavor physics, quarkonium and exotic states, searches for dark sectors, and many other areas. The sensitivity to a large number of key observables can be improved by about an order of magnitude compared to the current measurements, and up to two orders in very clean search measurements. This increase in statistical precision arises not only due to the increased luminosity, but also from improved detector efficiency and precision for many channels. Many of the most interesting observables tend to have very small theoretical uncertainties that will therefore not limit the physics reach. This book has presented many new ideas for measurements, both to elucidate the nature of current anomalies seen in flavor, and to search for new phenomena in a plethora of observables that will become accessible with the Belle II dataset. The simulation used for the studiesinthis book was state ofthe artat the time, though weare learning a lot more about the experiment during the commissioning period. The detector is in operation, and working spectacularly well.",

keywords = "NONLEPTONIC-B-DECAYS, X-S-GAMMA, MINIMAL FLAVOR VIOLATION, FINAL-STATE INTERACTIONS, PION FORM-FACTOR, FORWARD-BACKWARD ASYMMETRY, HEAVY-QUARKONIUM SPECTRUM, LEFT-RIGHT SYMMETRY, TO-LEADING-ORDER, FLUX-TUBE MODEL",

author = "{Belle II Collaboration} and E. Kou and P. Urquijo and W. Altmannshofer and F. Beaujean and G. Bell and M. Beneke and Bigi, {I. I.} and F. Bishara and M. Blanke and C. Bobeth and M. Bona and N. Brambilla and Braun, {V. M.} and J. Brod and Buras, {A. J.} and Cheng, {H. Y.} and Chiang, {C. W.} and M. Ciuchini and G. Colangelo and A. Crivellin and H. Czyz and A. Datta and {De Fazio}, F. and T. Deppisch and Dolan, {M. J.} and J. Evans and S. Fajfer and T. Feldmann and S. Godfrey and M. Gronau and Y. Grossman and Guo, {F. K.} and U. Haisch and C. Hanhart and S. Hashimoto and S. Hirose and J. Hisano and L. Hofer and M. Hoferichter and D. Epifanov and N. Gabyshev and A. Garmash and S. Gribanov and A. Korobov and A. Kuzmin and D. Matvienko and B. Shwartz and Y. Usov and A. Vinokurova and V. Zhulanov and Эйдельман, {Семен Исаакович} and Кроковный, {Павел Петрович} and Ремнев, {Михаил Анатольевич}",

note = "Publisher Copyright: {\textcopyright} The Author(s) 2019. Published by Oxford University Press on behalf of the Physical Society of Japan.",

year = "2019",

month = dec,

doi = "10.1093/ptep/ptz106",

language = "English",

volume = "2019",

journal = "Progress of Theoretical and Experimental Physics",

issn = "2050-3911",

publisher = "Oxford University Press",

number = "12",

}

RIS

TY - JOUR

T1 - The Belle II physics book

AU - Belle II Collaboration

AU - Kou, E.

AU - Urquijo, P.

AU - Altmannshofer, W.

AU - Beaujean, F.

AU - Bell, G.

AU - Beneke, M.

AU - Bigi, I. I.

AU - Bishara, F.

AU - Blanke, M.

AU - Bobeth, C.

AU - Bona, M.

AU - Brambilla, N.

AU - Braun, V. M.

AU - Brod, J.

AU - Buras, A. J.

AU - Cheng, H. Y.

AU - Chiang, C. W.

AU - Ciuchini, M.

AU - Colangelo, G.

AU - Crivellin, A.

AU - Czyz, H.

AU - Datta, A.

AU - De Fazio, F.

AU - Deppisch, T.

AU - Dolan, M. J.

AU - Evans, J.

AU - Fajfer, S.

AU - Feldmann, T.

AU - Godfrey, S.

AU - Gronau, M.

AU - Grossman, Y.

AU - Guo, F. K.

AU - Haisch, U.

AU - Hanhart, C.

AU - Hashimoto, S.

AU - Hirose, S.

AU - Hisano, J.

AU - Hofer, L.

AU - Hoferichter, M.

AU - Epifanov, D.

AU - Gabyshev, N.

AU - Garmash, A.

AU - Gribanov, S.

AU - Korobov, A.

AU - Kuzmin, A.

AU - Matvienko, D.

AU - Shwartz, B.

AU - Usov, Y.

AU - Vinokurova, A.

AU - Zhulanov, V.

AU - Эйдельман, Семен Исаакович

AU - Кроковный, Павел Петрович

AU - Ремнев, Михаил Анатольевич

PY - 2019/12

Y1 - 2019/12

N2 - The Belle II detector will provide a major step forward in precision heavy flavor physics, quarkonium and exotic states, searches for dark sectors, and many other areas. The sensitivity to a large number of key observables can be improved by about an order of magnitude compared to the current measurements, and up to two orders in very clean search measurements. This increase in statistical precision arises not only due to the increased luminosity, but also from improved detector efficiency and precision for many channels. Many of the most interesting observables tend to have very small theoretical uncertainties that will therefore not limit the physics reach. This book has presented many new ideas for measurements, both to elucidate the nature of current anomalies seen in flavor, and to search for new phenomena in a plethora of observables that will become accessible with the Belle II dataset. The simulation used for the studiesinthis book was state ofthe artat the time, though weare learning a lot more about the experiment during the commissioning period. The detector is in operation, and working spectacularly well.

AB - The Belle II detector will provide a major step forward in precision heavy flavor physics, quarkonium and exotic states, searches for dark sectors, and many other areas. The sensitivity to a large number of key observables can be improved by about an order of magnitude compared to the current measurements, and up to two orders in very clean search measurements. This increase in statistical precision arises not only due to the increased luminosity, but also from improved detector efficiency and precision for many channels. Many of the most interesting observables tend to have very small theoretical uncertainties that will therefore not limit the physics reach. This book has presented many new ideas for measurements, both to elucidate the nature of current anomalies seen in flavor, and to search for new phenomena in a plethora of observables that will become accessible with the Belle II dataset. The simulation used for the studiesinthis book was state ofthe artat the time, though weare learning a lot more about the experiment during the commissioning period. The detector is in operation, and working spectacularly well.

KW - NONLEPTONIC-B-DECAYS

KW - X-S-GAMMA

KW - MINIMAL FLAVOR VIOLATION

KW - FINAL-STATE INTERACTIONS

KW - PION FORM-FACTOR

KW - FORWARD-BACKWARD ASYMMETRY

KW - HEAVY-QUARKONIUM SPECTRUM

KW - LEFT-RIGHT SYMMETRY

KW - TO-LEADING-ORDER

KW - FLUX-TUBE MODEL

UR - http://www.scopus.com/inward/record.url?scp=85082462408&partnerID=8YFLogxK

U2 - 10.1093/ptep/ptz106

DO - 10.1093/ptep/ptz106

M3 - Review article

AN - SCOPUS:85082462408

VL - 2019

JO - Progress of Theoretical and Experimental Physics

JF - Progress of Theoretical and Experimental Physics

SN - 2050-3911

IS - 12

M1 - ARTN 123C01

ER -

ID: 24331014