Implication of MINOS results to neutrino masses
We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles θ 13 and θ 23 in combination. According to the exclusion curve obtained from recent experimental results, the mass spectrum of the normal hierarchy is disfavored. A model is constru...
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| Published in | Journal of the Korean Physical Society Vol. 61; no. 3; pp. 324 - 329 |
|---|---|
| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
Seoul
The Korean Physical Society
01.08.2012
한국물리학회 |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0374-4884 1976-8524 |
| DOI | 10.3938/jkps.61.324 |
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| Abstract | We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles
θ
13
and
θ
23
in combination. According to the exclusion curve obtained from recent experimental results, the mass spectrum of the normal hierarchy is disfavored. A model is constructed and examined to explain the compatibility of the model and the phenomenologically allowed parameter region in sin
θ
23
vs.
sin
θ
13
. The prediction of the model, which contains certain criteria in the ratio of non-Standard Model additional Higgs scales, results in an inverted hierarchy in masses, 1 <
m
2
/
m
3
< 1.7. |
|---|---|
| AbstractList | We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles
θ
13
and
θ
23
in combination. According to the exclusion curve obtained from recent experimental results, the mass spectrum of the normal hierarchy is disfavored. A model is constructed and examined to explain the compatibility of the model and the phenomenologically allowed parameter region in sin
θ
23
vs.
sin
θ
13
. The prediction of the model, which contains certain criteria in the ratio of non-Standard Model additional Higgs scales, results in an inverted hierarchy in masses, 1 <
m
2
/
m
3
< 1.7. We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles θ13 and θ23 in combination. According to the exclusion curve obtained from recent experimental results, the mass spectrum of the normal hierarchy is disfavored. A model is constructed and examined to explain the compatibility of the model and the phenomenologically allowed parameter region in sin θ23 vs. sin θ13. The prediction of the model, which contains certain criteria in the ratio of non-Standard Model additional Higgs scales, results in an inverted hierarchy in masses, 1 < m2/m3 < 1.7. KCI Citation Count: 0 |
| Author | Kim, Siyeon |
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| Cites_doi | 10.1103/PhysRevLett.107.041801 10.1103/PhysRevLett.107.181802 10.1007/JHEP11(2011)106 10.1088/0954-3899/37/7A/075021 10.1103/PhysRevD.70.073008 10.1103/PhysRevD.84.053002 10.1103/PhysRevLett.108.191802 10.1103/PhysRevD.83.056013 10.1103/PhysRevD.78.093008 10.1016/j.physrep.2007.12.004 10.1088/0954-3899/38/1/015003 10.1103/PhysRevLett.108.131801 10.1103/PhysRevLett.108.171803 |
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| Keywords | Neutrino oscillation Flavor symmetry Mixing angles |
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| References_xml | – reference: MeloniD.MorisiS.PeinadoE.J. Phys. G2011380150032011JPhG...38a5003M10.1088/0954-3899/38/1/015003 – reference: AhnJ. K.Phys. Rev. Lett.20121081918022012PhRvL.108s1802A10.1103/PhysRevLett.108.191802 – reference: ParkN. W.NamK. H.SiyeonK.Phys. Rev. D2011830560132011PhRvD..83e6013P10.1103/PhysRevD.83.056013 – reference: ChenS. L.FrigerioM.MaE.Phys. Rev. D2004700730082004PhRvD..70g3008C10.1103/PhysRevD.70.073008 – reference: E. Ma, arXiv:hep-ph/0409075. – reference: AbeK.Phys. Rev. Lett.20111070418012011PhRvL.107d1801A10.1103/PhysRevLett.107.041801 – reference: Gonzalez-GarciaM. C.MaltoniM.Phys. Rep.200846012008PhR...460....1G10.1016/j.physrep.2007.12.004 – reference: MorisiS.PatelK. M.PeinadoE.Phys. Rev. D2011840530022011PhRvD..84e3002M10.1103/PhysRevD.84.053002 – reference: AnF. P.Phys. Rev. Lett.20121081718032012PhRvL.108q1803A10.1103/PhysRevLett.108.171803 – reference: HwangG. -R.SiyeonK.Phys. Rev. D2008780930082008PhRvD..78i3008H10.1103/PhysRevD.78.093008 – reference: AbeY.Phys. Rev. Lett.20121081318012012PhRvL.108m1801A10.1103/PhysRevLett.108.131801 – reference: NakamuraK.J. Phys. G2010370750212010JPhG...37g5021N10.1088/0954-3899/37/7A/075021 – reference: ChuX.DhenM.HambyeT.J. High Energy Phys.201111111062011JHEP...11..106C10.1007/JHEP11(2011)106 – reference: AdamsonP.Phys. Rev. Lett.20111071818022011PhRvL.107r1802A10.1103/PhysRevLett.107.181802 – reference: P. V. Dong, H. N. Long, C. H. Nam and V. V. Vien, arXiv:1111.6360 [hep-ph]. – volume: 107 start-page: 041801 year: 2011 ident: 457_CR1 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.107.041801 – volume: 107 start-page: 181802 year: 2011 ident: 457_CR2 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.107.181802 – ident: 457_CR14 – volume: 1111 start-page: 106 year: 2011 ident: 457_CR13 publication-title: J. High Energy Phys. doi: 10.1007/JHEP11(2011)106 – volume: 37 start-page: 075021 year: 2010 ident: 457_CR6 publication-title: J. Phys. G doi: 10.1088/0954-3899/37/7A/075021 – volume: 70 start-page: 073008 year: 2004 ident: 457_CR15 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.70.073008 – volume: 84 start-page: 053002 year: 2011 ident: 457_CR10 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.84.053002 – volume: 108 start-page: 191802 year: 2012 ident: 457_CR5 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.108.191802 – volume: 83 start-page: 056013 year: 2011 ident: 457_CR9 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.83.056013 – volume: 78 start-page: 093008 year: 2008 ident: 457_CR8 publication-title: Phys. Rev. D doi: 10.1103/PhysRevD.78.093008 – volume: 460 start-page: 1 year: 2008 ident: 457_CR7 publication-title: Phys. Rep. doi: 10.1016/j.physrep.2007.12.004 – volume: 38 start-page: 015003 year: 2011 ident: 457_CR11 publication-title: J. Phys. G doi: 10.1088/0954-3899/38/1/015003 – ident: 457_CR12 – volume: 108 start-page: 131801 year: 2012 ident: 457_CR3 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.108.131801 – volume: 108 start-page: 171803 year: 2012 ident: 457_CR4 publication-title: Phys. Rev. Lett. doi: 10.1103/PhysRevLett.108.171803 |
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| Snippet | We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles
θ
13
and
θ
23
in combination. According... We analyzed the results of Main Injector Neutrino Oscillation Search (MINOS) that constrain the neutrino mixing angles θ13 and θ23 in combination. According to... |
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| Title | Implication of MINOS results to neutrino masses |
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