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Yuri Kamyshkov/ University of Tennessee Mini-Workshop, WU St. Louis, February 11, 2011.

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Presentation on theme: "Yuri Kamyshkov/ University of Tennessee Mini-Workshop, WU St. Louis, February 11, 2011."— Presentation transcript:

1 Yuri Kamyshkov/ University of Tennessee email: kamyshkov@utk.edu Mini-Workshop, WU St. Louis, February 11, 2011

2 n  nbar transition probability  -mixing amplitude All beyond SM physics is here 

3 n  nbar transition probability (for given  )

4 Suppression of n  nbar in intranuclear transitions (Friedman and Gal, 2008)

5 General approach: one of the neutrons in the nucleus transforms to anti-neutron and the latter is annihilated with other nucleons to pions

6 Sensitivity for free neutron search (appearance probability) Sensitivity for bound neutron search (in nucleon decay expts) Will use ILL experiment limit as a unit of sensitivity = 1u Corresponds to sensitivity = 16u

7 Important to know theoretical uncertainty Important to know theoretical uncertainty Is nuclear theory reliable? complete? Is nuclear theory reliable? complete? intranuclear search experiments: Super-K, Soudan-2 Frejus Free neutron search limit (ILL)

8 ExperimentYearA n  year (10 32 ) Det. eff.Candid.Bkgr.  nucl, yr (90% CL) Kamiokande1986O3.033%00.9/yr >0.43  10 32 Frejus1990Fe5.030%04 >0.65  10 32 Soudan-22002Fe21.918%54.5 >0.72  10 32 Super-K*2007O245.410.4%2021.3 >1.8  10 32 Super-K *2009O254.512%2324 >1.97  10 32 SNO *2010D0.5441%24.75 >0.301  10 32 * Not yet published Observed improvement weaker than SQRT is due to irreducible background of atmospheric ’s. Still possible to improve a limit (though slowly) but impossible to claim a discovery.

9 ExperimentYearA  nucl, yr (90% CL) R(old), s  1 R(new), s  1  (old), s  (new), s Kamiokande1986O >0.43  10 32 10  10 22 5  10 22 >1.2  10 8 >1.65  10 8 Frejus1990Fe >0.65  10 32 14  10 22 ? >1.2  10 8 ? Soudan-22002Fe >0.72  10 32 14  10 22 ? >1.3  10 8 ? Super-K*2007O >1.77  10 32 10  10 22 5  10 22 >2.36  10 8 >3.34  10 8 Super-K *2009O >1.97  10 32 10  10 22 5  10 22 >2.5  10 8 >3.53  10 8 SNO *2010D >0.301  10 32 2.48  10 22 0.82  10 22 >1.96  10 8 >3.4  10 8 V. Kopeliovich 2010, Deuterium Friedman and Gal 2008, Oxygen Dover, Gal et. al, old

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12 Claudio Ciofi degli Atti (Perugia U.) is going to look at this (January 2011)

13 Proposed by Stuart Raby (2010) overlap of two quarks wavefunctions is more probable than for 3 quarks such 2 quarks might be coming from proton (not only neutron) 4-antiquark final state annihilates faster

14 All these processes governed by the same crossing amplitude can result into the same indistinguishable final state (of ~ 5 pions)  Existing intranuclear NNbar limits will need to be re-evaluated

15 More on n  nbar suppression: sensitivity to CPT violation Following Yu. Abov, F. Djeparov, and L. Okun, Pisma ZhETF 39 (1984) 493 Transitions for free neutrons V=0 are suppressed when Suppression possible if  m >  (due to CPT violation) In the intranuclear transitions where V~10 MeV small provides no Intranuclear transitions additional suppression. Intranuclear transitions are not sensitive to  m ! are not sensitive to  m ! Valid only if  0, i.e. if n  nbar transformation exist

16  m (V=0) vs  in N  Nbar search (if  0) Experimental limits on mass difference Uncertainty of intranuclear suppression If N  Nbar transition will be observed this will be a new limit of CPT  m test


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