![Page 1: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/1.jpg)
NNbar programNNbar program::
• 3:30-5:30• R. N. Mohapatra: 3:30-4:00 (25+5)
What physics from NNbar ?• K. S. Babu: 4:00-4:25 (20+5)
Origin of matter and NNbar• R. Shrock: 4:25-4:50 (20+5)
Extra D and NNbar• Y. Kamyshkov: 4:50-5:10 (15+5)
Experimental issues• Discussion 5:10-5:30
![Page 2: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/2.jpg)
Working group members Working group members
• K. S. Babu• Z. Berezhiani• A. Dolgov• G. Gabadadze• A. Gal • Y. Kamyshkov• B. Kopeliovich• R. N. Mohapatra• R. Shrock
……………..
![Page 3: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/3.jpg)
What can N-N-bar Oscillation What can N-N-bar Oscillation teach us about physics teach us about physics
Beyond the standard model ?Beyond the standard model ?
R. N. MohapatraUniversity of Maryland
DUSEL Theory Workshop, Columbus, Ohio; April 4-6,2008.
![Page 4: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/4.jpg)
Particle oscillationsParticle oscillations
• Oscillations of quantum mechanical states is a familiar phenomenon in Nature.
• In particle physics, electrically neutral particles e.g. Kaons and neutrinos have been observed to oscillate, teaching us a great deal about the fundamental forces and matter.
• Neutron is another neutral particle- it could oscillate to anti-neutrons. What can it tell us about physics beyond the standard model ?
![Page 5: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/5.jpg)
Neutron-anti-neutron OscillationNeutron-anti-neutron Oscillation::
• Violates baryon number by two units:
• Any Indication of B-violation in Nature ?
(i) Standard model has B-violation (but it leaves B-L symmetry exact and B-L is emerging as an important new symmetry of Nature ) !!
(ii) Understanding the origin of matter requires B-Violation and often involves B-L violation !!
(iii) Most physics scenarios of physics BSM have B-violation e.g. Grand unified th.
![Page 6: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/6.jpg)
B-L : new symmetry in B-L : new symmetry in Nature ?Nature ?
• What happens to B-L symmetry beyond standard model ?
• Remain exact or gets broken ?• If broken, what is the scale of its
breaking ?• Physics associated with this
breaking e.g. is B-L part of GUT ?• Two expts that can probe it directly
are and N-N-bar oscillation.0
![Page 7: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/7.jpg)
Neutrino Mass and B-L=2Neutrino Mass and B-L=2• If neutrino is Majorana particle, it
breaks B-L by two units; observation of decay will confirm this but by itself will not tell us much about new physics associated with (B-L).
•N-N-bar observation MAY supply this information !!• (with normal nu-hierarchy, may be very
difficult to observe leaving NNbar as only way)
0
0
![Page 8: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/8.jpg)
Neutrino mass-NNbar connectionNeutrino mass-NNbar connection
• Majorana neutrino -> implies (B-L)=2;• In quark-lepton unified theories B and L get
connected and L=2 implies B =2 via B-L symmetry and hence N-N-bar oscillation.
• There are reasons to think that there may be quark lepton unification at high energies.
• Discovery of neutrino mass therefore provides a very strong motivation to search for N-N-bar oscillation, which can be new window to Q-L unification as well as B-L symmetry.
![Page 9: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/9.jpg)
Questions for N-N-bar oscillationQuestions for N-N-bar oscillation
• Can the possible reach of N-N-bar oscillation time in existing facilities probe interesting range for new physics indicated by neutrino mass ?
- Are there decent theories EMBEDDING small neutrino masses where scale N-N-bar oscillation is observable?
• Is it cosmologically safe to have observable N-N-bar oscillation ?
• The answer to all these questions is YES .
![Page 10: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/10.jpg)
March 2005Theme Group 2
Phenomenology of N-N-bar OscPhenomenology of N-N-bar Osc
n
n
Vm
Vm
n
n
ti
2
1
tVVSinVV
P nn )( 212
2
21
Two :cases:1))(( 21 tVVi
2
nnnn
tP
1))(( 21 VVii
2
21
VVP nn
t
![Page 11: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/11.jpg)
Present expt situation in N-N-bar OscPresent expt situation in N-N-bar Osc..
Range accessible to current reactor fluxes: Present limit:ILL experiment: Baldoceolin et al. (1994)
New proposal (Y. Kamyshkov et al.) for an expt. In DUSEL
GOAL:
Figure of merit ~
.sec108 nn
10 > 10 sec.n n
2
nn
tFlux
8 11~ 10 10 sec.n n
or factor 1,000-10,000in appearance probability
![Page 12: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/12.jpg)
Could proton decay set-up be used to Could proton decay set-up be used to discover N-N-bar ?discover N-N-bar ?
• Nuclei will become unstable with N-N-bar interaction; but rate suppressed due to nuclear potential diff. between N and N-bar. (Gal et al; Alberico et al; Kopeliovich et al.)
• Present limits:• Sudan, IMB, SK-
• Nuclear Uncertainties !• Atmos, Bg makes
discovery reach very limited
freeNuc R 2 123 sec105.0 R
Could Proton decay set-up be used to discover NNbar ?
8~ 3 10 s
![Page 13: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/13.jpg)
Mass scales probed by N-N-barMass scales probed by N-N-bar
To see what is probed by N-N-bar, do operator analysis for processes:
2BO cccccc ddudduM 5
1
62 QCDBnn Om
5~/ Mm nnnn 6/
giving .sec10~ 8nn GeV5.510
2B
M
Note M5 suppression
![Page 14: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/14.jpg)
Scale Reach of N-N-barScale Reach of N-N-bar
• Is the scale reach of N-N-bar limited to only 300 TeV in generic models as suggested ?
• NO- once new physics at TeV scale is entertained e.g. SUSY, new Higgs !
![Page 15: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/15.jpg)
Weaker suppression with SUSYWeaker suppression with SUSY
A. Dominant operator with SUSY:
B. SUSY + diquark Higgs field , at TeV scale
ccuu
Can probe M_B-L upto
109 GeV
Probe M_{B-L} to 1012 GeV.
![Page 16: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/16.jpg)
theory For N-N-bar theory For N-N-bar • Neutrino mass points to New
electroweak symmetry with B-L• Gauge group: Left-right sym th.
• Fermion:
• New approach to observed parity violation i.e. it is only a low energy phenomenon !!
• The true weak interaction theory is parity conserving like strong, EM and gravity !!
LBRL USUSU )1()2()2(
L
L
d
u
R
R
d
u
L
L
e
R
R
e
P P
![Page 17: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/17.jpg)
scale of new B-L physics ?scale of new B-L physics ?
One attractive possibility suggested by coupling constant unification is that it is GeV.
Local B-L is part of a grand unifying symmetry and it breaks at GUT scale. Related physics is GUT physics. Group: SO(10)
1610
![Page 18: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/18.jpg)
Alternative B-L UnificationAlternative B-L Unification• New physics below GUT scale• Only 16 fermions unified but not gauge
couplings:
(Pati, Salam, 73)
Only restriction on B-L scale is nu mass (not coupling unification) and hence
-even 100 TeV
N-N-bar is an effective probe in this case;
cRL SUSUSU )4()2()2(
GeVGeVM 1611224 1010
![Page 19: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/19.jpg)
Non-SUSY G(224) and N-N-barNon-SUSY G(224) and N-N-bar• The Feynman diagram for N-N-bar in Non-
SUSY 224 model (RNM, Marshak, 80)
• vertex needed for baryogenesis .• With M= N-N-bar
observable only if
5~/ Mm nnnn
6/5~/ Mm nnnn
LBMM GeVM LB65.510
4
![Page 20: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/20.jpg)
Origin of matter in N-N-bar Origin of matter in N-N-bar modelsmodels
• Popular scenarios: e.g. leptogenesis have baryon asymmetry generated at very high temperatues;
• Observable N-N-bar -> remains in equilibrium down to TeV Temp: erases this asymmetry;
• Discovery of NNbar osc will point to radically new way to understand the origin of matter
One example of such a scenario: Baryon asymmetry after sphaleron decoupling: In the context of 224 model, it is the late decay of field that can create baryons using the CKM phase.
Post-sphaleron baryogenesis: Babu,RNM, Nasri PRL, (2006,2007);
(BABU’s talk)
0
![Page 21: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/21.jpg)
.sec1010 1211 NNRoughly
Baryogenesis upper limit on Baryogenesis upper limit on NNbar Osc time.NNbar Osc time.
![Page 22: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/22.jpg)
Preliminary conclusion:Preliminary conclusion:
• Non-SUSY G_224 model with ~100 TeV B-L scale is a completely self consistent alternative to usual GUT scenarios !!
• No proton decay problem- NN-bar observable and has an upper limit !
• Could imagine solving gauge hierarchy problem via extra dim scenarios !!
![Page 23: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/23.jpg)
Estimate of N-N-bar in SUSY 224 model:Estimate of N-N-bar in SUSY 224 model:
• New Feynman diagram for N-N-bar osc.
N-N-bar osc can probe MB-L~1011 GeV (Dutta, Mimura, RNM; PRL (2006)
![Page 24: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/24.jpg)
Proton decay vs N-N-bar oscillationProton decay vs N-N-bar oscillation
![Page 25: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/25.jpg)
Other Theories probed by N-N-barOther Theories probed by N-N-bar
• N-N-bar is also observable in generic low gravity scale extra dim. Models:
• (Nussinov, Shrock; Dvali, Gabadadze; Dolgov, Bambi; )
• N-N-bar expt could also probe mirror sector of the Universe by searching for N-N’ oscillation:
- Current limits ~400 sec.• (Bento, Berezhiani, 2005)
![Page 26: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/26.jpg)
• Berezhiani’s Talk: MIRROR WORLD• Lee and Yang, parity paper (1957)
A bit more on N-N’ Oscillation:A bit more on N-N’ Oscillation:
![Page 27: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/27.jpg)
What is a mirror neutron ?What is a mirror neutron ?
• u’d’d’=n’ mirrror neutron
![Page 28: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/28.jpg)
n-n’ oscillation n-n’ oscillation
• Phenomenology: very similar to n-n-bar case:
![Page 29: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/29.jpg)
Present status of searchPresent status of search
![Page 30: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/30.jpg)
So Why do N-N-bar search ?So Why do N-N-bar search ?• If neutrino are Majorana, it implies B-L=2 and it is
important to know the scale of B-L breaking. Neutrino mass by itself does not give us this information.
• If there is quark lepton unif., N-N-bar oscillation exists and can probe the scale and physics associated with B-L.
• Search at 1010 sec level will test for (B-L) (seesaw) scale < 1011 GeV vs GUT seesaw.
• NNbar discovery will fundamentally alter our thinking about:
(i) grand unification; (ii) Origin of matter; (Babu) (iii) constrain CPT violation, extra dim. (iv) N-N’ to throw light on dark matter.
Thank you for your attention.
![Page 31: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/31.jpg)
Discussion points:Discussion points:
• Physics issues- mass scale probed
• Cosmology
• Nuclear physics
• Experiment
nuclnn vs 2
![Page 32: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/32.jpg)
ConclusionConclusion
• With the discovery of neutrino mass the case for N-N-bar oscillation is a lot stronger now than before. Urge new search at the level of >1010 sec to test for (B-L) (seesaw) scale less than 1011 GeV vs GUT scale seesaw.
• N-N-bar discovery will completely change the thinking on grand unification.
• Baryon asymmetry consistent with NN-bar;
Upper limit on NN-bar time in some cases.• Reactor oscillation search much better than
decay searches due to nucl. uncertainties !!
Thank you for your attention.
![Page 33: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/33.jpg)
B-L- Grand unificationB-L- Grand unification• SO(10) : the minimal GUT theory with
B-L motivated by Gauge coupling unification:
• All fermions unified to
one {16} dim rep.• (Georgi; Fritzch, Minkowski)
• B-L violation scale is GUT scale
due to unification. N-N-bar
suppressed and unobservable.
![Page 34: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/34.jpg)
Nucleon Decay in Generic SignatureNucleon Decay in Generic Signature
• Key test of GUTS: Gauge Boson mediated p-decay:
![Page 35: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/35.jpg)
Origin of MatterOrigin of Matter• Possible scenarios:
• Leptogenesis:
• Hard to test at low energies: Strictly No connection to neutrino mass phases;
• Electroweak baryogenesis: • Higgs mass < 120 GeV. Testable.
![Page 36: NNbar program: 3:30-5:30 R. N. Mohapatra: 3:30-4:00 (25+5) What physics from NNbar ? K. S. Babu: 4:00-4:25 (20+5) Origin of matter and NNbar R. Shrock:](https://reader036.vdocument.in/reader036/viewer/2022062714/56649d585503460f94a38661/html5/thumbnails/36.jpg)
Baryogenesis upper limit onBaryogenesis upper limit on
• Scenario for NON-SUSY 224 model ( )
• S has B=2 coupling; • S Decays go out of Eq. around ~ few 100 GEV • The S-particle does not decay until
• After which it decays and produces baryon-anti-baryon asymmetry:
• The S-decay reheats the Universe to TR
giving a dilution of which should not too small.
These put an upper limit on NNbar time (Babu’s talk)
NN
2/11 ][ PS MT
ccS Re
S
R
M
T