html5-img
1 / 24

Status of GMSB studies

Status of GMSB studies. Shilei Zang University of Colorado, Boulder. CU CMS Meeting, 28th Apr. 2008. Outline. Invariant mass of neutralino. De-convolution method. MET. MET distribution is used to get signal yield, but we have two gravitinos. g. jet. q. q. jet. …. p. p. q. ….

Download Presentation

Status of GMSB studies

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Status of GMSB studies ShileiZang University of Colorado, Boulder CU CMS Meeting, 28th Apr. 2008

  2. Outline • Invariant mass of neutralino • De-convolution method

  3. MET • MET distribution is used to get signal yield, but we have two gravitinos. g jet q q jet … p p q … jet q jet g

  4. MET distribution is used to get signal yield. • Simple variable; powerful separation; largely used • 1) It’s crowded at small MET region for both signal and background. • 2) Shapes are different for signal and each bkg. • 3) Vector addition of the two gravitinos. • 4) MET resolution is difficult to estimate. • 5) Can not get mass from MET •  MET is not a much sensitive variable; bkg studies are difficult; not directly relate with mass •  Can we use the invariant mass of photon+gravitino?

  5. MET • MET • Pt2>0GeV • Peak=157 GeV • MET • Pt1>90GeV; Pt2>30GeV • Peak=160.4 GeV;

  6. Invariant mass of neutralino • Pt1>90GeV; Pt2>30GeV; MET>130GeV • Peak=223GeV; sig=61GeV • Pt2>0GeV • Peak=185GeV • Sig=77GeV • Pt1>90GeV; Pt2>30GeV; • Peak=196GeV

  7. two gravitinos. • photon and gravitino. • photon1 and gravitino2 • photon2 and gravitino1 • Cos(theta) from MC Truth

  8. Cos(theta) of and .

  9. -cos(theta) • cos(theta) • Ratio = (-cos(theta))/cos(theta) • -cos(theta) • cos(theta)

  10. mass • mass2 • mass minus • mass2 weighted • mass2 weighted • mass = CB Line; mass2weighted = CB Line + Polynomial • mass = mass2weighted for background

  11. Variables for GMSB analysis MET Rough mass of neutralino Edge of MT2 distribution Edges of some invariant masses Accurate calculation with cross-events for long decay chain Long-lived neutralinos: photon timing, cluster shapes, decay chain, .. (CDF, ATLAS, CMS) Deconvolution method accurate mass of neutralino; accurate ctau of neutralino hep-ph/9906349 CMS Note1997/079 arXiv:0802.4290v1

  12. Rough mass of neutralino • Many questions on mass: Not accurate; Bias? Shape? Backgrounds? • Signal can be fitted with CB Line? • Bkg shapes are expected to be similar (CB Line + Polynomial functions) can study all backgrounds together? • mass2weighted can be used for bkg study or as a cross check.

  13. De-convolution Method • Convolution: linear shift-invariant f(mass) (mass) system: g(mass) • Mass: rough mass Briet-Wigner (Delta) transfer Resolution (Gaussian) noise (Argus)

  14. Rough mass in Data: • Accurate mass in Data : • Rough mass in signal MC: • Accurate mass in signal MC: • Suppose we know h and f for signal MC; • We can determine the transfer function g by deconvolution using signal MC. • In Fourier space: • h, f  H, F  G g (signal MC) • h, g  H, G  F f (Data)

  15. Signal MC: GM1b~1g • h • Peak=196 • RMS=112 Gaussian f (mean=mass0 rough sigma) ? = system: g RooFit

  16. Data : • signal MC: • h0 • Peak=175 • RMS=89 • h • Peak=196 • RMS=112 • Peak=196.8GeV

  17. h • Mean=235 • Peak=196 • RMS=112 • g • Mean=1GeV • RMS=89 Signal MC: GM1e • f • Mean=196GeV • RMS=70 Gold deconvolution algorithm

  18. Convolution is largely used in: Statistics; Astronomy; Meteorology; Geophysics; Optics; Digital image; Spectroscopy; …;but not in Particle physics as I know. • Deconvolution can be used to recover the missing information. MET, resolution, … mass, width, … • A shadow is the convolution of the shape of the light source that is casting the shadow and the object whose shadow is being cast • An out-of-focus photograph is the convolution of the sharp image with the shape of the iris diaphragm. • An echo is the convolution of the original sound with a function representing the various objects that are reflecting it. • …… wikipedia

  19. Summary • We can use mass to get signal yield, CB Linefunctions. Same methods as in MET for bkg studies; or bkg studies are simple. • We can use mass-mass2weighted as a cross check of the result. • De-convolution method is introduced, which is expected to be useful in experimental particle physics. • Test the invariant mass and the de-convolution method with all GMSB points and all backgrounds. • Study the QCD control samples: • Correlation between shower shape/isolation and MET/massneed to be studied. • Can shower shape/isolation get enough control sample? Do we need photon Pt, MET, number of jets, or jets’ pt for control sample? Thank you!

  20. MT2 • hep-ph/9906349 • Left edge is known; use the right edge to get the mass. • Enough signal events close to the right edge? • Edge is not sharp; shape? Background?

  21. Edge of invariant mass Jet+photon  • CMS Note 1997/079 • Kinematics reasons 2 leptons  2 leptons+1photon 

  22. Accurate calculation with cross-events • arXiv:0802.4290v1 • 6 constraints; 8 unknowns for one event. • 6+10 constrains; 16 unknowns for two events. solve the equations • Need long decay chain. • Wrong combinations are large. • Bias? Shape? ill equations? measure uncertainties? ...

  23. Long-lived neutralino • arXiv:0804.1043v1 Search for heavy, long-lived neutralinos that decay to photons at CDF II using photon timing • arXiv:0704.0760v1 Search for heavy, long-lived particles that decay to photons at CDF II • arXiv:0710.2647v1 Search for GMSB NLSPs at LHC • PRD 69, 035003 (2004) Study of the gauge mediation signal with nonpointing photons at the CERN LHC • ……

More Related