The singular seesaw mechanism with hierarchical Dirac neutrino mass
Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Chikira, Y. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2000 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer-Verlag Berlin Heidelberg 2000 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal / C - Springer-Verlag, 1998, 16(2000), 4 vom: Sept., Seite 701-705 |
|---|---|
| Übergeordnetes Werk: |
volume:16 ; year:2000 ; number:4 ; month:09 ; pages:701-705 |
| Links: |
|---|
| DOI / URN: |
10.1007/s100520000397 |
|---|
| Katalog-ID: |
OLC2069066991 |
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| 520 | |a Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. | ||
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10.1007/s100520000397 doi (DE-627)OLC2069066991 (DE-He213)s100520000397-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Chikira, Y. verfasserin aut The singular seesaw mechanism with hierarchical Dirac neutrino mass 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 2000 Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. Independent Experiment Mass Matrix Neutrino Mass Neutrino Oscillation Solar Neutrino Haba, N. aut Mimura, Y. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 16(2000), 4 vom: Sept., Seite 701-705 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:16 year:2000 number:4 month:09 pages:701-705 https://doi.org/10.1007/s100520000397 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 AR 16 2000 4 09 701-705 |
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10.1007/s100520000397 doi (DE-627)OLC2069066991 (DE-He213)s100520000397-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Chikira, Y. verfasserin aut The singular seesaw mechanism with hierarchical Dirac neutrino mass 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 2000 Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. Independent Experiment Mass Matrix Neutrino Mass Neutrino Oscillation Solar Neutrino Haba, N. aut Mimura, Y. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 16(2000), 4 vom: Sept., Seite 701-705 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:16 year:2000 number:4 month:09 pages:701-705 https://doi.org/10.1007/s100520000397 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 AR 16 2000 4 09 701-705 |
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10.1007/s100520000397 doi (DE-627)OLC2069066991 (DE-He213)s100520000397-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Chikira, Y. verfasserin aut The singular seesaw mechanism with hierarchical Dirac neutrino mass 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 2000 Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. Independent Experiment Mass Matrix Neutrino Mass Neutrino Oscillation Solar Neutrino Haba, N. aut Mimura, Y. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 16(2000), 4 vom: Sept., Seite 701-705 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:16 year:2000 number:4 month:09 pages:701-705 https://doi.org/10.1007/s100520000397 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 AR 16 2000 4 09 701-705 |
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10.1007/s100520000397 doi (DE-627)OLC2069066991 (DE-He213)s100520000397-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Chikira, Y. verfasserin aut The singular seesaw mechanism with hierarchical Dirac neutrino mass 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 2000 Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. Independent Experiment Mass Matrix Neutrino Mass Neutrino Oscillation Solar Neutrino Haba, N. aut Mimura, Y. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 16(2000), 4 vom: Sept., Seite 701-705 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:16 year:2000 number:4 month:09 pages:701-705 https://doi.org/10.1007/s100520000397 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 AR 16 2000 4 09 701-705 |
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10.1007/s100520000397 doi (DE-627)OLC2069066991 (DE-He213)s100520000397-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Chikira, Y. verfasserin aut The singular seesaw mechanism with hierarchical Dirac neutrino mass 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin Heidelberg 2000 Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. Independent Experiment Mass Matrix Neutrino Mass Neutrino Oscillation Solar Neutrino Haba, N. aut Mimura, Y. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 16(2000), 4 vom: Sept., Seite 701-705 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:16 year:2000 number:4 month:09 pages:701-705 https://doi.org/10.1007/s100520000397 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_32 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4277 GBV_ILN_4306 GBV_ILN_4310 AR 16 2000 4 09 701-705 |
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The singular seesaw mechanism with hierarchical Dirac neutrino mass |
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Chikira, Y. |
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The European physical journal / C |
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Chikira, Y. Haba, N. Mimura, Y. |
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10.1007/s100520000397 |
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the singular seesaw mechanism with hierarchical dirac neutrino mass |
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The singular seesaw mechanism with hierarchical Dirac neutrino mass |
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Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. © Springer-Verlag Berlin Heidelberg 2000 |
| abstractGer |
Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. © Springer-Verlag Berlin Heidelberg 2000 |
| abstract_unstemmed |
Abstract. The singular seesaw mechanism can naturally explain the atmospheric neutrino deficit by maximal oscillations between $\nu_{\mu_{\mathrm{L}}}$ and $\nu_{\mu_{\mathrm{R}}}$. This mechanism can also induce three different scales of the neutrino mass squared differences, which can explain the neutrino deficits of three independent experiments (solar, atmospheric, and LSND) by neutrino oscillations. In this paper we show that realistic mixing angles among the neutrinos can be obtained by introducing a hierarchy in the Dirac neutrino mass. In the case where the Majorana neutrino mass matrix has rank 2, the solar neutrino deficit is explained by vacuum oscillations between $\nu_e$ and $\nu_\tau$. We also consider the case where the Majorana neutrino mass matrix has rank 1. In this case, the matter enhanced Mikheyev–Smirnov–Wolfenstein solar neutrino solution is preferred as the solution of the solar neutrino deficit. © Springer-Verlag Berlin Heidelberg 2000 |
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The singular seesaw mechanism with hierarchical Dirac neutrino mass |
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