Observation of a new χ(b) state in radiative transitions to Υ(1S) and Υ(2S) at ATLAS.
نویسندگان
- G Aad
- B Abbott
- J Abdallah
- A A Abdelalim
- A Abdesselam
- O Abdinov
- B Abi
- M Abolins
- O S AbouZeid
- H Abramowicz
- H Abreu
- E Acerbi
- B S Acharya
- L Adamczyk
- D L Adams
- T N Addy
- J Adelman
- M Aderholz
- S Adomeit
- P Adragna
- T Adye
- S Aefsky
- J A Aguilar-Saavedra
- M Aharrouche
- S P Ahlen
- F Ahles
- A Ahmad
- M Ahsan
- G Aielli
- T Akdogan
- T P A Åkesson
- G Akimoto
- A V Akimov
- A Akiyama
- M S Alam
- M A Alam
- J Albert
- S Albrand
- M Aleksa
- I N Aleksandrov
- F Alessandria
- C Alexa
- G Alexander
- G Alexandre
- T Alexopoulos
- M Alhroob
- M Aliev
- G Alimonti
- J Alison
- M Aliyev
- B M M Allbrooke
- P P Allport
- S E Allwood-Spiers
- J Almond
- A Aloisio
- R Alon
- A Alonso
- B Alvarez Gonzalez
- M G Alviggi
- K Amako
- P Amaral
- C Amelung
- V V Ammosov
- A Amorim
- G Amorós
- N Amram
- C Anastopoulos
- L S Ancu
- N Andari
- T Andeen
- C F Anders
- G Anders
- K J Anderson
- A Andreazza
- V Andrei
- M-L Andrieux
- X S Anduaga
- A Angerami
- F Anghinolfi
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- N Anjos
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- J Antos
- F Anulli
- S Aoun
- L Aperio Bella
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- G Arabidze
- I Aracena
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- E Arik
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- A J Armbruster
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- D Arutinov
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- K Augsten
- M Aurousseau
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- C Ay
- G Azuelos
- Y Azuma
- M A Baak
- G Baccaglioni
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- H Bachacou
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- Y Bai
- D C Bailey
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- S Baker
- E Banas
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- J R Carter
- J Carvalho
- D Casadei
- M P Casado
- M Cascella
- C Caso
- A M Castaneda Hernandez
- E Castaneda-Miranda
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- N F Castro
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- A Chafaq
- D Chakraborty
- K Chan
- B Chapleau
- J D Chapman
- J W Chapman
- E Chareyre
- D G Charlton
- V Chavda
- C A Chavez Barajas
- S Cheatham
- S Chekanov
- S V Chekulaev
- G A Chelkov
- M A Chelstowska
- C Chen
- H Chen
- S Chen
- T Chen
- X Chen
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- A Cheplakov
- V F Chepurnov
- R Cherkaoui El Moursli
- V Chernyatin
- E Cheu
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- A Clark
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- W Cleland
- J C Clemens
- B Clement
- C Clement
- R W Clifft
چکیده
The χ(b)(nP) quarkonium states are produced in proton-proton collisions at the Large Hadron Collider at sqrt[s] = 7 TeV and recorded by the ATLAS detector. Using a data sample corresponding to an integrated luminosity of 4.4 fb(-1), these states are reconstructed through their radiative decays to Υ(1S,2S) with Υ → μ+ μ-. In addition to the mass peaks corresponding to the decay modes χ(b)(1P,2P) → Υ(1S)γ, a new structure centered at a mass of 10.530 ± 0.005(stat) ± 0.009(syst) GeV is also observed, in both the Υ(1S)γ and Υ(2S)γ decay modes. This structure is interpreted as the χ(b)(3P) system.
منابع مشابه
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متن کاملar X iv : h ep - p h / 01 04 25 3 v 5 2 3 O ct 2 00 1 Production of the η b ( nS ) states
The rates for magnetic dipole (M1) transitions Υ(nS) → ηb(n S) + γ, n ≤ n, are compared. The photon energies for allowed (n = n) M1 transitions are very small, so hindered (n < n) transitions could be more favorable for discovering the ηb(1S, 2S). The question then arises whether Υ(2S) or Υ(3S) is a better source of ηb(1S). Whereas one nonrelativistic model favors ηb(1S) production from Υ(2S), ...
متن کاملar X iv : h ep - p h / 01 04 25 3 v 2 2 6 A pr 2 00 1 Production of the η b ( nS ) states 1
The rates for magnetic dipole (M1) transitions Υ(nS) → ηb(n S) + γ, n ≤ n, are compared. The photon energies for allowed (n = n) M1 transitions are very small, so hindered (n < n) transitions could be more favorable for discovering the ηb(1S, 2S). The question then arises whether Υ(2S) or Υ(3S) is a better source of ηb(1S). Whereas one nonrelativistic model favors ηb(1S) production from Υ(2S), ...
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ورودعنوان ژورنال:
- Physical review letters
دوره 108 15 شماره
صفحات -
تاریخ انتشار 2012