QCD factorization of the four-lepton decay $$B^-\rightarrow \ell \bar{\nu }_\ell \ell ^{(\prime )} \bar{\ell }^{(\prime )}$$ B - ν ¯ ( ) ¯ ( )

Martin Beneke (Physik Department T31, Technische Universität München, James-Franck-Straße 1, Garching, 85748, Germany) ; Philipp Böer (Physik Department T31, Technische Universität München, James-Franck-Straße 1, Garching, 85748, Germany) ; Panagiotis Rigatos (Physik Department T31, Technische Universität München, James-Franck-Straße 1, Garching, 85748, Germany) ; K. Vos (Gravitational Waves and Fundamental Physics (GWFP), Maastricht University, Duboisdomein 30, Maastricht, 6229 GT, The Netherlands; Nikhef, Science Park 105, Amsterdam, 1098 XG, The Netherlands)

Motivated by the first search for the rare charged-current B decay to four leptons, $$\ell \bar{\nu }_\ell \ell ^{(\prime )} \bar{\ell }^{(\prime )}$$ ν ¯ ( ) ¯ ( ) , we calculate the decay amplitude with factorization methods. We obtain the $$B\rightarrow \gamma ^*$$ B γ form factors, which depend on the invariant masses of the two lepton pairs, at leading power in an expansion in $$\Lambda _\mathrm{QCD}/m_b$$ Λ QCD / m b to next-to-leading order in $$\alpha _s$$ α s , and at $$\mathcal {O}(\alpha _s^0)$$ O ( α s 0 ) at next-to-leading power. Our calculations predict branching fractions of a few times $$10^{-8}$$ 10 - 8 in the $$\ell ^{(\prime )} \bar{\ell }^{(\prime )}$$ ( ) ¯ ( ) mass-squared bin up to $$q^2=1~$$ q 2 = 1 GeV $$^2$$ 2 with $$n_+q>3~$$ n + q > 3 GeV. The branching fraction rapidly drops with increasing $$q^2$$ q 2 . An important further motivation for this investigation has been to explore the sensitivity of the decay rate to the inverse moment $$\lambda _B$$ λ B of the leading-twist B meson light-cone distribution amplitude. We find that in the small- $$q^2$$ q 2 bin, the sensitivity to $$\lambda _B$$ λ B is almost comparable to $$B^- \rightarrow \mathrm {\ell }^- \bar{\nu }_{\mathrm {\ell }}\gamma $$ B - - ν ¯ γ when $$\lambda _B$$ λ B is small, but with an added uncertainty from the light-meson intermediate resonance contribution. The sensitivity degrades with larger $$q^2$$ q 2 .

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          "country": "Germany", 
          "value": "Physik Department T31, Technische Universit\u00e4t M\u00fcnchen, James-Franck-Stra\u00dfe 1, Garching, 85748, Germany", 
          "organization": "Technische Universit\u00e4t M\u00fcnchen"
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      "surname": "Beneke", 
      "given_names": "Martin", 
      "full_name": "Beneke, Martin"
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      "affiliations": [
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          "country": "Germany", 
          "value": "Physik Department T31, Technische Universit\u00e4t M\u00fcnchen, James-Franck-Stra\u00dfe 1, Garching, 85748, Germany", 
          "organization": "Technische Universit\u00e4t M\u00fcnchen"
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      "surname": "B\u00f6er", 
      "email": "philipp.boeer@tum.de", 
      "full_name": "B\u00f6er, Philipp", 
      "given_names": "Philipp"
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    {
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      "surname": "Rigatos", 
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      "surname": "Vos", 
      "given_names": "K.", 
      "full_name": "Vos, K."
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      "title": "QCD factorization of the four-lepton decay  $$B^-\\rightarrow \\ell \\bar{\\nu }_\\ell \\ell ^{(\\prime )} \\bar{\\ell }^{(\\prime )}$$  <math> <mrow> <msup> <mi>B</mi> <mo>-</mo> </msup> <mo>\u2192</mo> <mi>\u2113</mi> <msub> <mover> <mrow> <mi>\u03bd</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mi>\u2113</mi> </msub> <msup> <mi>\u2113</mi> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> <msup> <mover> <mrow> <mi>\u2113</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> </mrow> </math>"
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      "source": "Springer", 
      "value": "Motivated by the first search for the rare charged-current B decay to four leptons,  $$\\ell \\bar{\\nu }_\\ell \\ell ^{(\\prime )} \\bar{\\ell }^{(\\prime )}$$  <math> <mrow> <mi>\u2113</mi> <msub> <mover> <mrow> <mi>\u03bd</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mi>\u2113</mi> </msub> <msup> <mi>\u2113</mi> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> <msup> <mover> <mrow> <mi>\u2113</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> </mrow> </math>  , we calculate the decay amplitude with factorization methods. We obtain the  $$B\\rightarrow \\gamma ^*$$  <math> <mrow> <mi>B</mi> <mo>\u2192</mo> <msup> <mi>\u03b3</mi> <mo>\u2217</mo> </msup> </mrow> </math>   form factors, which depend on the invariant masses of the two lepton pairs, at leading power in an expansion in  $$\\Lambda _\\mathrm{QCD}/m_b$$  <math> <mrow> <msub> <mi>\u039b</mi> <mi>QCD</mi> </msub> <mo>/</mo> <msub> <mi>m</mi> <mi>b</mi> </msub> </mrow> </math>   to next-to-leading order in  $$\\alpha _s$$  <math> <msub> <mi>\u03b1</mi> <mi>s</mi> </msub> </math>  , and at  $$\\mathcal {O}(\\alpha _s^0)$$  <math> <mrow> <mi>O</mi> <mo>(</mo> <msubsup> <mi>\u03b1</mi> <mi>s</mi> <mn>0</mn> </msubsup> <mo>)</mo> </mrow> </math>   at next-to-leading power. Our calculations predict branching fractions of a few times  $$10^{-8}$$  <math> <msup> <mn>10</mn> <mrow> <mo>-</mo> <mn>8</mn> </mrow> </msup> </math>   in the  $$\\ell ^{(\\prime )} \\bar{\\ell }^{(\\prime )}$$  <math> <mrow> <msup> <mi>\u2113</mi> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> <msup> <mover> <mrow> <mi>\u2113</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mrow> <mo>(</mo> <mo>\u2032</mo> <mo>)</mo> </mrow> </msup> </mrow> </math>   mass-squared bin up to  $$q^2=1~$$  <math> <mrow> <msup> <mi>q</mi> <mn>2</mn> </msup> <mo>=</mo> <mn>1</mn> <mspace width=\"3.33333pt\"></mspace> </mrow> </math>  GeV $$^2$$  <math> <msup> <mrow></mrow> <mn>2</mn> </msup> </math>   with  $$n_+q&gt;3~$$  <math> <mrow> <msub> <mi>n</mi> <mo>+</mo> </msub> <mi>q</mi> <mo>&gt;</mo> <mn>3</mn> <mspace width=\"3.33333pt\"></mspace> </mrow> </math>  GeV. The branching fraction rapidly drops with increasing  $$q^2$$  <math> <msup> <mi>q</mi> <mn>2</mn> </msup> </math>  . An important further motivation for this investigation has been to explore the sensitivity of the decay rate to the inverse moment  $$\\lambda _B$$  <math> <msub> <mi>\u03bb</mi> <mi>B</mi> </msub> </math>   of the leading-twist B meson light-cone distribution amplitude. We find that in the small- $$q^2$$  <math> <msup> <mi>q</mi> <mn>2</mn> </msup> </math>   bin, the sensitivity to  $$\\lambda _B$$  <math> <msub> <mi>\u03bb</mi> <mi>B</mi> </msub> </math>   is almost comparable to  $$B^- \\rightarrow \\mathrm {\\ell }^- \\bar{\\nu }_{\\mathrm {\\ell }}\\gamma $$  <math> <mrow> <msup> <mi>B</mi> <mo>-</mo> </msup> <mo>\u2192</mo> <msup> <mrow> <mi>\u2113</mi> </mrow> <mo>-</mo> </msup> <msub> <mover> <mrow> <mi>\u03bd</mi> </mrow> <mrow> <mo>\u00af</mo> </mrow> </mover> <mi>\u2113</mi> </msub> <mi>\u03b3</mi> </mrow> </math>   when  $$\\lambda _B$$  <math> <msub> <mi>\u03bb</mi> <mi>B</mi> </msub> </math>   is small, but with an added uncertainty from the light-meson intermediate resonance contribution. The sensitivity degrades with larger  $$q^2$$  <math> <msup> <mi>q</mi> <mn>2</mn> </msup> </math>  ."
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Published on:
21 July 2021
Publisher:
Springer
Published in:
European Physical Journal C , Volume 81 (2021)
Issue 7
Pages 1-15
DOI:
https://doi.org/10.1140/epjc/s10052-021-09388-y
Copyrights:
The Author(s)
Licence:
CC-BY-4.0

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