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000206353 0247_ $$2arXiv$$aarXiv:1411.7771
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000206353 0881_ $$aBELLE-PREPRINT-2014-18; arXiv:1411.7771
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000206353 088__ $$2arXiv$$aarXiv:1411.7771
000206353 1001_ $$0P:(DE-HGF)0$$aDutta, D.$$b0
000206353 245__ $$aSearch for $B_{s}^{0}\rightarrow\gamma\gamma$ and a measurement of the branching fraction for $B_{s}^{0}\rightarrow\phi\gamma$
000206353 260__ $$a[S.l.]$$bAmerican Physical Society$$c2015
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000206353 520__ $$aWe search for the decay ${B}_{s}^{0}\to \gamma \gamma $ and measure the branching fraction for ${B}_{s}^{0}\to \varphi \gamma $ using $121.4\text{}\text{}{\mathrm{fb}}^{-1}$ of data collected at the $\mathrm{\Upsilon }\left(5S\right)$ resonance with the Belle detector at the KEKB asymmetric-energy ${e}^{+}{e}^{-}$ collider. The ${B}_{s}^{0}\to \varphi \gamma $ branching fraction is measured to be $\left(3.6±0.5\left(\text{stat}\right)±0.3\left(\text{syst}\right)±0.6\left({f}_{s}\right)\right)×1{0}^{-5}$, where ${f}_{s}$ is the fraction of ${B}_{s}^{\left(*\right)}{\overline{B}}_{s}^{\left(*\right)}$ in $b\overline{b}$ events. Our result is in good agreement with the theoretical predictions as well as with a recent measurement from LHCb. We observe no statistically significant signal for the decay ${B}_{s}^{0}\to \gamma \gamma $ and set a 90% confidence-level upper limit on its branching fraction at $3.1×1{0}^{-6}$. This constitutes a significant improvement over the previous result.
000206353 536__ $$0G:(DE-H253)POF2-BELLE-I-II-Exp.-20130405$$aExperiments at KEK (BELLE I/II) (POF2-515)$$cPOF2-515$$fPOF II$$x0
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000206353 650_7 $$2INSPIRE$$aelectron positron: annihilation
000206353 650_7 $$2INSPIRE$$aelectron positron: colliding beams
000206353 650_7 $$2INSPIRE$$aUpsilon(10870): electroproduction
000206353 650_7 $$2INSPIRE$$aUpsilon(10870): hadronic decay
000206353 650_7 $$2INSPIRE$$aB/s0: radiative decay
000206353 650_7 $$2INSPIRE$$aB/s0: branching ratio: measured
000206353 650_7 $$2INSPIRE$$aB/s0: branching ratio: upper limit
000206353 650_7 $$2INSPIRE$$aexperimental results
000206353 650_7 $$2INSPIRE$$aBELLE
000206353 650_7 $$2INSPIRE$$aKEK-B
000206353 650_7 $$2INSPIRE$$aB/s0 --> 2photon
000206353 650_7 $$2INSPIRE$$aB/s0 --> Phi(1020) photon
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000206353 7001_ $$0P:(DE-HGF)0$$aBhuyan, B.$$b1$$eCorresponding author
000206353 7001_ $$0P:(DE-HGF)0$$aAbdesselam, A.$$b2
000206353 7001_ $$0P:(DE-HGF)0$$aAdachi, I.$$b3
000206353 7001_ $$0P:(DE-HGF)0$$aAihara, H.$$b4
000206353 7001_ $$0P:(DE-HGF)0$$aSaid, S. Al$$b5
000206353 7001_ $$0P:(DE-HGF)0$$aArinstein, K.$$b6
000206353 7001_ $$0P:(DE-HGF)0$$aAsner, D. M.$$b7
000206353 7001_ $$0P:(DE-HGF)0$$aAulchenko, V.$$b8
000206353 7001_ $$0P:(DE-HGF)0$$aAushev, T.$$b9
000206353 7001_ $$0P:(DE-HGF)0$$aAyad, R.$$b10
000206353 7001_ $$0P:(DE-HGF)0$$aAziz, T.$$b11
000206353 7001_ $$0P:(DE-HGF)0$$aBahinipati, S.$$b12
000206353 7001_ $$0P:(DE-HGF)0$$aBakich, A. M.$$b13
000206353 7001_ $$0P:(DE-HGF)0$$aBansal, V.$$b14
000206353 7001_ $$0P:(DE-HGF)0$$aBhardwaj, V.$$b15
000206353 7001_ $$0P:(DE-HGF)0$$aBonvicini, G.$$b16
000206353 7001_ $$0P:(DE-HGF)0$$aBracko, M.$$b17
000206353 7001_ $$0P:(DE-HGF)0$$aBrowder, T. E.$$b18
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000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.85.014008$$o10.1103/PhysRevD.85.014008
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000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1093/ptep/pts072$$o10.1093/ptep/pts072
000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/S0168-9002(02)01771-0$$o10.1016/S0168-9002(02)01771-0
000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevD.87.031101$$o10.1103/PhysRevD.87.031101
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000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1103/PhysRevLett.41.1581$$o10.1103/PhysRevLett.41.1581
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000206353 999C5 $$2Crossref$$9-- missing cx lookup --$$a10.1016/0370-2693(90)91293-K$$o10.1016/0370-2693(90)91293-K
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