The Cabibbo angle as a universal seed for quark and lepton mixings

A model-independent ansatz to describe lepton and quark mixing in a unified way is suggested based upon the Cabibbo angle. In our framework neutrinos mix in a “Bi-Large” fashion, while the charged leptons mix as the “down-type” quarks do. In addition to the standard Wolfenstein parameters (λ, A) two...
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Autor*in:	S. Roy [verfasserIn] S. Morisi [verfasserIn] N.N. Singh [verfasserIn] J.W.F. Valle [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Schlagwörter:	PMNS matrix CKM matrix Cabibbo angle Bi-Large mixing Wolfenstein parameter Neutrino mixing

Übergeordnetes Werk:	In: Physics Letters B - Elsevier, 2015, 748(2015), C, Seite 4
Übergeordnetes Werk:	volume:748 ; year:2015 ; number:C ; pages:4

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.1016/j.physletb.2015.06.052

Katalog-ID:	DOAJ053296974

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topic	misc QC1-999 misc PMNS matrix misc CKM matrix misc Cabibbo angle misc Bi-Large mixing misc Wolfenstein parameter misc Neutrino mixing misc Physics
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title	The Cabibbo angle as a universal seed for quark and lepton mixings
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title_full	The Cabibbo angle as a universal seed for quark and lepton mixings
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title_sort	cabibbo angle as a universal seed for quark and lepton mixings
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title_auth	The Cabibbo angle as a universal seed for quark and lepton mixings
abstract	A model-independent ansatz to describe lepton and quark mixing in a unified way is suggested based upon the Cabibbo angle. In our framework neutrinos mix in a “Bi-Large” fashion, while the charged leptons mix as the “down-type” quarks do. In addition to the standard Wolfenstein parameters (λ, A) two other free parameters (ψ, δ) are needed to specify the physical lepton mixing matrix. Through this simple assumption one makes specific predictions for the atmospheric angle as well as leptonic CP violation in good agreement with current observations.
abstractGer	A model-independent ansatz to describe lepton and quark mixing in a unified way is suggested based upon the Cabibbo angle. In our framework neutrinos mix in a “Bi-Large” fashion, while the charged leptons mix as the “down-type” quarks do. In addition to the standard Wolfenstein parameters (λ, A) two other free parameters (ψ, δ) are needed to specify the physical lepton mixing matrix. Through this simple assumption one makes specific predictions for the atmospheric angle as well as leptonic CP violation in good agreement with current observations.
abstract_unstemmed	A model-independent ansatz to describe lepton and quark mixing in a unified way is suggested based upon the Cabibbo angle. In our framework neutrinos mix in a “Bi-Large” fashion, while the charged leptons mix as the “down-type” quarks do. In addition to the standard Wolfenstein parameters (λ, A) two other free parameters (ψ, δ) are needed to specify the physical lepton mixing matrix. Through this simple assumption one makes specific predictions for the atmospheric angle as well as leptonic CP violation in good agreement with current observations.
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title_short	The Cabibbo angle as a universal seed for quark and lepton mixings
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The Cabibbo angle as a universal seed for quark and lepton mixings

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