resonance-continuum interference in gg h bb
DESCRIPTION
_. Resonance-Continuum Interference in gg H bb. Lance Dixon (CERN & SLAC) and Yorgos Sofianatos (SLAC) 0812.3712. LCWS2010, CERN/Geneva, 19 Octo ber. Motivation. - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/1.jpg)
Resonance-Continuum Interference in gg H bb
Lance Dixon (CERN & SLAC)and Yorgos Sofianatos (SLAC)
0812.3712
LCWS2010, CERN/Geneva, 19 October
_
![Page 2: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/2.jpg)
Motivation• One of the principal motivations for building a gg collider is to produce a light Higgs boson via gg H, and then detect its dominant decay to b quark pairs.
• In order to extract Higgs couplings, would like to interpret the size of the bump as
• But this is not necessarily true if the signal interferes appreciably with the continuum background, in this case
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 2
![Page 3: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/3.jpg)
Motivation in pictures
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 3
![Page 4: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/4.jpg)
Motivation (cont.)• For
the anticipated experimental uncertainty in
assuming 80 fb-1 in the high-energy peak and mH < 140 GeVis 2% Melles, Stirling, Khoze, hep-ph/9970238; Ginsburg, Krawczyk, Osland, hep-ph/0101208, hep-ph/0101229;Soldner-Rembold, Jikia, hep-ex/0101056; Niezurawski, Zarnecki and Krawczyk, hep-ph/0208034, hep-ph/0307183;Nieurawski, hep-ph/0503295, hep-ph/0507004; Bechtel et al., physics/0601204; K. Monig and A. Rosca, 0705.1259.
• So we should check whether the peak height is equal to this quantity to better than 2%.
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 4
![Page 5: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/5.jpg)
Motivation (cont.)• Another place resonance-continuum interference could be
significant is in the SM Higgs gg decay mode at the LHC (gluon fusion production). LD, Siu, hep-ph/0302233
• Here effect is 3-5%, smaller than currently envisaged experimental uncertainties, and smaller than some of the estimated theoretical uncertainties (but not all).
• But not a lot smaller.
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 5
![Page 6: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/6.jpg)
Amplitude interference• Total amplitude:
• Interference term has 2 pieces:
• First term vanishes upon integration over as long as don’t vary too quickly
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 6
Dicus, Stange, Willenbrock, hep-ph/9404359
![Page 7: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/7.jpg)
In search of a phase• Need• All mostly real in SM.
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 7
![Page 8: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/8.jpg)
Computing the phase• A little algebra
• 2nd term dominates• Comes just from this cut graph
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 8
![Page 9: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/9.jpg)
Analytical result
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 9
For all but very forward scattering angles, we can let mb 0in the brackets, obtaining:
![Page 10: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/10.jpg)
Numerical result at 45◦
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 10
![Page 11: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/11.jpg)
Dependence on scattering angle
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 11
![Page 12: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/12.jpg)
Beyond SM?
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference 12
• We did not study this very thoroughly; however, d scaleswithYukawa coupling lb (for a while):
• E.g., MSSM “intense coupling regime” can have large lb Boos, Djouadi, Muhlleitner, Vologdin, hep-ph/0205160; Boos Djouadi, Nikitenko, hep-ph/0307079
• As an example, we took lb = 20 x lb(SM)d = - 4% for mH = 130 GeV, q = 45◦ . (Now is significant too.)
![Page 13: Resonance-Continuum Interference in gg H bb](https://reader036.vdocuments.site/reader036/viewer/2022062314/56812c6c550346895d91036e/html5/thumbnails/13.jpg)
13
Conclusions
• In the SM, resonance-continuum interference in the process
is safely below the anticipated experimental uncertainties for
• However, if there is evidence that the b quark Yukawa coupling is greatly enhanced over that in the SM, then the interference effect could be significant and should be investigated further, as a function of model parameters.
LCWS2010 19 Oct. 2010L. Dixon Resonance-Continuum Interference