First Observation of Excited ωb- States

Standard

First Observation of Excited ωb- States. / The LHCb Collaboration.

In: Physical Review Letters, Vol. 124, No. 8, 082002, 25.02.2020.

Research output: Contribution to journal › Article › peer-review

Harvard

The LHCb Collaboration 2020, 'First Observation of Excited ωb- States', Physical Review Letters, vol. 124, no. 8, 082002. https://doi.org/10.1103/PhysRevLett.124.082002

APA

The LHCb Collaboration (2020). First Observation of Excited ωb- States. Physical Review Letters, 124(8), [082002]. https://doi.org/10.1103/PhysRevLett.124.082002

Vancouver

The LHCb Collaboration. First Observation of Excited ωb- States. Physical Review Letters. 2020 Feb 25;124(8):082002. doi: 10.1103/PhysRevLett.124.082002

Author

The LHCb Collaboration. / First Observation of Excited ωb- States. In: Physical Review Letters. 2020 ; Vol. 124, No. 8.

BibTeX

@article{abaeaf0e4bcc4b4ba23882b9f12bab68,

title = "First Observation of Excited ωb- States",

abstract = "We report four narrow peaks in the Ξb0K- mass spectrum obtained using pp collisions at center-of-mass energies of 7, 8, and 13 TeV, corresponding to a total integrated luminosity of 9 fb-1 recorded by the LHCb experiment. Referring to these states by their mass, the mass values are m[ωb(6316)-]=6315.64±0.31±0.07±0.50 MeV, m[ωb(6330)-]=6330.30±0.28±0.07±0.50 MeV, m[ωb(6340)-]=6339.71±0.26±0.05±0.50 MeV, m[ωb(6350)-]=6349.88±0.35±0.05±0.50 MeV, where the uncertainties are statistical, systematic, and the last is due to the knowledge of the Ξb0 mass. The natural widths of the three lower mass states are consistent with zero, and the 90% confidence-level upper limits are determined to be Γ[ωb(6316)-]<2.8 MeV, Γ[ωb(6330)-]<3.1 MeV and Γ[ωb(6340)-]<1.5 MeV. The natural width of the ωb(6350)- peak is 1.4-0.8+1.0±0.1 MeV, which is 2.5σ from zero and corresponds to an upper limit of 2.8 MeV. The peaks have local significances ranging from 3.6σ to 7.2σ. After accounting for the look-elsewhere effect, the significances of the ωb(6316)- and ωb(6330)- peaks are reduced to 2.1σ and 2.6σ, respectively, while the two higher mass peaks exceed 5σ. The observed peaks are consistent with expectations for excited ωb- resonances.",

author = "{The LHCb Collaboration} and R. Aaij and {Abell{\'a}n Beteta}, C. and T. Ackernley and B. Adeva and M. Adinolfi and H. Afsharnia and Aidala, {C. A.} and S. Aiola and Z. Ajaltouni and S. Akar and P. Albicocco and J. Albrecht and F. Alessio and M. Alexander and {Alfonso Albero}, A. and G. Alkhazov and {Alvarez Cartelle}, P. and Alves, {A. A.} and S. Amato and Y. Amhis and L. An and L. Anderlini and G. Andreassi and M. Andreotti and F. Archilli and {Arnau Romeu}, J. and A. Artamonov and M. Artuso and K. Arzymatov and E. Aslanides and M. Atzeni and B. Audurier and S. Bachmann and Back, {J. J.} and S. Baker and V. Balagura and W. Baldini and A. Baranov and Barlow, {R. J.} and S. Barsuk and W. Barter and M. Bartolini and F. Baryshnikov and A. Bondar and S. Eidelman and P. Krokovny and V. Kudryavtsev and T. Maltsev and L. Shekhtman and V. Vorobyev",

year = "2020",

month = feb,

day = "25",

doi = "10.1103/PhysRevLett.124.082002",

language = "English",

volume = "124",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "8",

}

RIS

TY - JOUR

T1 - First Observation of Excited ωb- States

AU - The LHCb Collaboration

AU - Aaij, R.

AU - Abellán Beteta, C.

AU - Ackernley, T.

AU - Adeva, B.

AU - Adinolfi, M.

AU - Afsharnia, H.

AU - Aidala, C. A.

AU - Aiola, S.

AU - Ajaltouni, Z.

AU - Akar, S.

AU - Albicocco, P.

AU - Albrecht, J.

AU - Alessio, F.

AU - Alexander, M.

AU - Alfonso Albero, A.

AU - Alkhazov, G.

AU - Alvarez Cartelle, P.

AU - Alves, A. A.

AU - Amato, S.

AU - Amhis, Y.

AU - An, L.

AU - Anderlini, L.

AU - Andreassi, G.

AU - Andreotti, M.

AU - Archilli, F.

AU - Arnau Romeu, J.

AU - Artamonov, A.

AU - Artuso, M.

AU - Arzymatov, K.

AU - Aslanides, E.

AU - Atzeni, M.

AU - Audurier, B.

AU - Bachmann, S.

AU - Back, J. J.

AU - Baker, S.

AU - Balagura, V.

AU - Baldini, W.

AU - Baranov, A.

AU - Barlow, R. J.

AU - Barsuk, S.

AU - Barter, W.

AU - Bartolini, M.

AU - Baryshnikov, F.

AU - Bondar, A.

AU - Eidelman, S.

AU - Krokovny, P.

AU - Kudryavtsev, V.

AU - Maltsev, T.

AU - Shekhtman, L.

AU - Vorobyev, V.

PY - 2020/2/25

Y1 - 2020/2/25

N2 - We report four narrow peaks in the Ξb0K- mass spectrum obtained using pp collisions at center-of-mass energies of 7, 8, and 13 TeV, corresponding to a total integrated luminosity of 9 fb-1 recorded by the LHCb experiment. Referring to these states by their mass, the mass values are m[ωb(6316)-]=6315.64±0.31±0.07±0.50 MeV, m[ωb(6330)-]=6330.30±0.28±0.07±0.50 MeV, m[ωb(6340)-]=6339.71±0.26±0.05±0.50 MeV, m[ωb(6350)-]=6349.88±0.35±0.05±0.50 MeV, where the uncertainties are statistical, systematic, and the last is due to the knowledge of the Ξb0 mass. The natural widths of the three lower mass states are consistent with zero, and the 90% confidence-level upper limits are determined to be Γ[ωb(6316)-]<2.8 MeV, Γ[ωb(6330)-]<3.1 MeV and Γ[ωb(6340)-]<1.5 MeV. The natural width of the ωb(6350)- peak is 1.4-0.8+1.0±0.1 MeV, which is 2.5σ from zero and corresponds to an upper limit of 2.8 MeV. The peaks have local significances ranging from 3.6σ to 7.2σ. After accounting for the look-elsewhere effect, the significances of the ωb(6316)- and ωb(6330)- peaks are reduced to 2.1σ and 2.6σ, respectively, while the two higher mass peaks exceed 5σ. The observed peaks are consistent with expectations for excited ωb- resonances.

AB - We report four narrow peaks in the Ξb0K- mass spectrum obtained using pp collisions at center-of-mass energies of 7, 8, and 13 TeV, corresponding to a total integrated luminosity of 9 fb-1 recorded by the LHCb experiment. Referring to these states by their mass, the mass values are m[ωb(6316)-]=6315.64±0.31±0.07±0.50 MeV, m[ωb(6330)-]=6330.30±0.28±0.07±0.50 MeV, m[ωb(6340)-]=6339.71±0.26±0.05±0.50 MeV, m[ωb(6350)-]=6349.88±0.35±0.05±0.50 MeV, where the uncertainties are statistical, systematic, and the last is due to the knowledge of the Ξb0 mass. The natural widths of the three lower mass states are consistent with zero, and the 90% confidence-level upper limits are determined to be Γ[ωb(6316)-]<2.8 MeV, Γ[ωb(6330)-]<3.1 MeV and Γ[ωb(6340)-]<1.5 MeV. The natural width of the ωb(6350)- peak is 1.4-0.8+1.0±0.1 MeV, which is 2.5σ from zero and corresponds to an upper limit of 2.8 MeV. The peaks have local significances ranging from 3.6σ to 7.2σ. After accounting for the look-elsewhere effect, the significances of the ωb(6316)- and ωb(6330)- peaks are reduced to 2.1σ and 2.6σ, respectively, while the two higher mass peaks exceed 5σ. The observed peaks are consistent with expectations for excited ωb- resonances.

UR - http://www.scopus.com/inward/record.url?scp=85080878467&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.124.082002

DO - 10.1103/PhysRevLett.124.082002

M3 - Article

C2 - 32167334

AN - SCOPUS:85080878467

VL - 124

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 8

M1 - 082002

ER -

ID: 27909476