ebook img

Embedding the neutrino four-group Z_2 x Z_2 into the alternating group of four objects A_4 PDF

0.14 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Embedding the neutrino four-group Z_2 x Z_2 into the alternating group of four objects A_4

IFT-04/32 Z2 Z2 Embedding the neutrino four-group × A4∗ into the alternating group of four obje ts Woj ie h Królikowski 5 0 Institute of Theoreti al Physi s, Warsaw University 0 2 Ho»a 69, PL(cid:21)00(cid:21)681 Warszawa, Poland n a J 3 Abstra t 1 s v If and only if the small neutrino mixing sine 13 is put zero, the e(cid:27)e tive neutrino 8 M s s Z 0 12 23 2 mass matrix with any mixing sines and is invariant under a y li group 0 m m 0 Z Z 1 2 1 2 2 of the order two and (cid:22) in the limit of − → (cid:22) also under the group × 0 5 often alled the four-group. However, the elements of this group do not build up fully the 0 / M m m h term of proportional to 2− 1. When the four-group is embedded into the group of p A M - 4 p even permutations of four obje ts (whi h is of the order twelve), then the term of e m m A 2 1 4 h proportional to − an be fully onstru ted from elements of . In ontrast, when : D v 4 the four-group is embedded into the dihedral group of the order eight, then the term i X M m m D 2 1 4 r of proportional to − annot be fully built up from elements of . a PACS numbers: 12.15.Ff , 14.60.Pq , 12.15.Hh . De ember 2004 ∗ Work supported in partby the PolishState CommitteeforS ienti(cid:28) Resear h(KBN), grant2P03B 129 24 (2003(cid:21)2004). 1. Introdu tion U = (U ) (α = αi As is well known, the generi form of e(cid:27)e tive neutrino mixing matrix e,µ,τ , i = 1,2,3) reads, c s 0 12 12 U = c s c c s , 23 12 23 12 23  −  (1) s s s c c 23 12 23 12 23 −   s 13 if is put zero onsistently with the nonobservation of the neutrino os illations in the ν¯ s2 < 0.04 short-baseline experiments for rea tor e's (the estimated upper bound is 13 ) [1℄. c = cosθ s = sinθ ij ij ij ij Here, and . Two possible CP-violatingMajorana phases irrelevant fortheos illationpro esses areomittedinEq. (1). One CP-violatingDira phase relevant s = 0 13 for these pro esses disappears together with . The formula(1) is onsistent with allwell established neutrino-os illationexperiments θ 32 θ 45 ∆m2 = that provide the globalestimates: 12 ∼ ◦ and 23 ∼ ◦ for mixingangles, and 21 m2 m2 8 10 5 eV2 ∆m2 = m2 m2 2.5 10 3 eV2 2 − 1 ∼ × − and | 32| | 3 − 2| ∼ × − for mass-squared di(cid:27)eren es [2℄. U ν = U ν ν = ν ,ν ,ν The unitary matrix gives the neutrino mixing α i αi i, where α e µ τ νi = ν1,ν2,ν3 P and are the (cid:29)avor and mass a tive neutrinos, respe tively. In the (cid:29)avor U representation, where the harged-lepton mass matrix is diagonal, the matrix gives U M U = m δ also the diagonalization α,β α∗i αβ βj i ij of the e(cid:27)e tive neutrino mass matrix M = (Mαβ) (α,β = e,µ,Pτ). Then, the inverse formula Mαβ = iUαimiUβ∗i enables one Mαβ P mi to al ulate the mass-matrix elements in terms of neutrino masses and mixing- U U αi matrix elements . In this way, using the form (1) of , one obtains the following s = 0 13 generi form of e(cid:27)e tive neutrino mass-matrix valid in the ase of : 1 0 0 0 0 0 m +m M = 1 2 0 c2 c s +m 0 s2 c s 2  23 − 23 23  3 23 23 23  0 c s s2 0 c s c2 − 23 23 23 23 23 23     1 0 0 0 c s +m2 −m1 c −0 c2 c s +s c 203 − 203 , 2  sol 23 − 23 23  sol 23  (2) 0 c s s2 s 0 0 − 23 23 23 − 23      c = c2 s2 = cos2θ s = 2c s = sin2θ where sol 12 − 12 12 and sol 12 12 12. 1 3 3 1(m +m ) m 1(m m ) In the formula(2), allthree × matri es standing at 2 1 2 , 3 and 2 2− 1 3 3 ommute, while two omponents of the third × matrix anti ommute. Diagonalizing both sides of Eq. (2), one gets onsistently m 0 0 1 0 0 0 0 0 1 m +m 1 2 0 m 0 = 0 1 0 + m 0 0 0 2 3   2     0 0 m 0 0 0 0 0 1 3    1 0 0   m2 m1 − + − 0 1 0 , 2   (3) 0 0 0   U MU = (m ,m ,m ) † 1 2 3 where diag . Z Z 2 2 2. The four-group × s = 0 13 The e(cid:27)e tive neutrino mass matrix (2) valid in the ase of an be rewritten as follows: m +m 1 1 1 2 M = (ϕ ϕ )+m (ϕ +ϕ ) 1 4 3 1 4 2 2 − 2 m m 1 2 1 + − [c (ϕ ϕ )+s (c λ s λ )] , sol 2 3 sol 23 1 23 4 2 2 − − (4) 3 3 if the × matri es 1 0 0 1 0 0 − ϕ = 0 1 0 , ϕ = 0 c s , 1 2 atm atm    −  0 0 1 0 s c atm atm − −  1 0 0   1 0 0  − ϕ = 0 1 0 , ϕ = 0 c s 3 4 atm atm  −   −  (5) 0 0 1 0 s c atm atm −     and 0 1 0 0 0 1 λ = 1 0 0 , λ = 0 0 0 1 4     (6) 0 0 0 1 0 0     c = c2 s2 = cos2θ s = 2c s = sin2θ are introdu ed, where atm 23 − 23 23 and atm 23 23 23. Here, the c = 1/√2 = s c = 0 s = 1 23 23 atm atm values (i.e., and ) are onsistent with experimental estimates. 2 c s 3 3 atm atm It is easy to he k for any and that four × matri es (5) are mutually multiplied a ording to the Cayley table of the form ϕ ϕ ϕ ϕ 1 2 3 4 ϕ ϕ ϕ ϕ ϕ 1 1 2 3 4 ϕ ϕ ϕ ϕ ϕ 2 2 1 4 3 ϕ ϕ ϕ ϕ ϕ 3 3 4 1 2 ϕ ϕ ϕ ϕ ϕ 4 4 3 2 1 Z Z 2 2 what hara terizes the Abelian (cid:28)nite group × of the order four, often alled the four-group [3℄. It is isomorphi to the simplest dihedral group of the order four. Thus, c s 3 3 3 atm atm for any and , four × matri es (5) onstitute a redu ible representation of the Abelian four-group [4℄. In fa t, they an be simultaneously diagonalized, leading to a 3 = 1+1+1 = 1,1,1 redu ed representation diag( ). M m m 2 1 One an see from Eq. (4) that the term of proportionalto − is not fullybuilt 3 3 c λ s λ 23 1 23 4 up from elements of four-group: the × matrix − lies outside the four-group. ϕ ϕ ϕ ϕ 1 4 2 3 This matrix ommutes with and , and anti ommutes with and . c s atm atm It is not di(cid:30) ult to verify for any and that the formula (4) implies four M dis rete invarian es of the e(cid:27)e tive neutrino mass matrix , two exa t: ϕ Mϕ = M 1,4 1,4 (7) m m 0 2 1 and two valid in the limit of − → : ϕ2,3Mϕ2,3 = M (m2 m1)ssol(c23λ1 s23λ4) m2−m1→0 M − − − −→ (8) ϕ c s 1 atm atm (of ourse, in the ase of the invarian e is trivial). Thus, for any and , the M m m 0 2 1 four-group is the symmetry group of in the limit of − → . c = 1/√2 = s 23 23 Further on, in onsisten y with experimental estimates, one will put c = 0 s = 1 atm atm (i.e., and ). 3 A 4 3. The alternating group of four obje ts A 4 The group of even permutations of four obje ts was applied to the neutrino mass matrix in Refs. [5℄. This non-Abelian (cid:28)nite group onsists of twelve permutations (1,2,3,4) , (2,1,4,3) , (3,4,1,2) , (4,3,2,1) , (2,3,1,4) , (1,4,2,3) , (4,1,3,2) , (3,2,4,1) , (3,1,2,4) , (4,2,1,3) , (1,3,4,2) , (2,4,3,1) (9) A 4 of whi h the (cid:28)rst four onstitute an Abelian subgroup of , isomorphi to the four- Z Z 2 2 group × . The twelve permutations (9) an be represented, respe tively, by the 4 4 following twelve × matri es onstru ted from the formal Dira matri es in the Dira representation: g = 1(D) , g = σ(D) , g = γ , g = γ σ(D) , 1 2 1 3 5 4 5 1 1(D) β 1(D) +β 1(D) σ(D) 1(D) +σ(D) g = − + σ(D) − 3 +γ 3 , 5 2 2 1 2 5 2 ! (cid:18) (cid:19) (D) g = γ g , g = g γ , g = σ g , 6 5 5 7 5 5 8 1 5 1(D) β 1(D) σ(D) 1(D) +β 1(D) +σ(D) g = − 1(D) +γ σ(D) − 3 + 1(D) +γ σ(D) 3 , 9 2 5 1 2 2 5 1 2 (cid:16) (cid:17) (D) (cid:16) (cid:17) g = g σ , g = g γ , g = γ g , 10 9 1 11 9 5 12 5 9 (10) 1(D) = 1(2),1(2) γ = 1(2),1(2) β = 1(2), 1(2) σ(D) = where diag( ) , 5 antidiag( ) , diag( − ) and 1,3 σ ,σ 1(2) = σ = σ = 1,3 1,3 1 3 diag( ) with diag(1,1) , antidiag(1,1) and diag(1,-1). 4 4 4 Twelve × matri es (10) form a redu ible representation of the non-Abelian group A 4 = 1 + 3 = 1,3 4 . In fa t, it an be redu ed to a representation diag( ) through the unitary transformation realizing the transitions γ diag(1(2), 1(2)) , β antidiag( 1(2), 1(2)) 5 → − → − − (11) and (D) (D) σ diag(σ ,σ ) , σ diag( σ , σ ) 1 → 3 3 3 → − 1 − 1 (12) 4 g g (a = 1,2,...,12) g = 1,ϕ ϕ (a = 1,2,...,12) Then a → a′ with a′ diag( ′a), where ′a are the 3 3 following twelve × matri es: 1 0 0 1 0 0 1 0 0 1 0 0 − − ϕ = 0 1 0 , ϕ = 0 1 0 , ϕ = 0 1 0 , ϕ = 0 1 0 , ′1   ′2   ′3  −  ′4  −  0 0 1 0 0 1 0 0 1 0 0 1 − −         0 1 0 0 1 0 0 1 0 0 1 0 − − ϕ = 0 0 1 , ϕ = 0 0 1 , ϕ = 0 0 1 , ϕ = 0 0 1 , ′5   ′6  −  ′7  −  ′8   1 0 0 1 0 0 1 0 0 1 0 0 − −         0 0 1 0 0 1 0 0 1 0 0 1 − − ϕ = 1 0 0 , ϕ = 1 0 0 , ϕ = 1 0 0 , ϕ = 1 0 0 , ′9   10 −  ′11   ′12 −  0 1 0 0 1 0 0 1 0 0 1 0 − −        (13) 3 A 1 4 forming an irredu ible representation of the group . Its irredu ible representation g (a = 1,2,...,12) a′ involved in onsists of twelve numbers 1,1,...,1. There are also two 1 A g = 1,ϕ 4 a′ ′a other irredu ible representations of , not involved in the diag( ) onsidered here. Note the identities T T T T ϕ = ϕ , ϕ = ϕ , ϕ = ϕ , ϕ = ϕ ′5 ′9 ′6 ′11 ′7 ′12 ′8 ′10 (14) and ϕ +ϕ +ϕ +ϕ = 0 , ′1 ′2 ′3 ′4 ϕ +ϕ +ϕ +ϕ = 0 , ′5 ′6 ′7 ′8 ϕ +ϕ +ϕ +ϕ = 0 , ′9 ′10 ′11 ′12 (15) as well as 0 1 0 1 (ϕ +ϕ +ϕ +ϕ ) = 1 0 0 = λ . 2 ′5 ′6 ′9 ′11   1 (16) 0 0 0   λ ϕ ϕ ϕ ϕ 1 ′1 ′4 ′2 ′3 The matrix ommutes with and , and anti ommutes with and . From Eqs. (15) one gets the "strong" onstraint 5 1 0 0 0 0 0 0 0 ga′ = 12 0 0 0 0  . (17) a X  0 0 0 0      Thus, the "weak" onstraint 1 2 ga′  3  = 0, (18) a X  4      (1,2,3,4)T (1,0,0,0)T if imposed on the state of four obje ts, impliesthat the state of the (0,2,3,4)T obje t 1 vanishes, while the state of the obje ts 2,3,4 isnot onstrained. When ν ν ,ν ,ν s e µ τ interpreting1 asa lightsterileneutrino and 2,3,4asthree a tive neutrinos , the ν ν ,ν ,ν s e µ τ "weak" onstraint (18) may eliminate as an "unphysi al" obje t, leaving only as "physi al". However, in absen e of the "weak" onstraint (18) all four neutrinos may be "physi al" obje ts. 3 A 3 4 Another irredu ible representation of , isomorphi to the previous onsisting of 3 3 twelve × matri es (13), an be de(cid:28)ned through the unitary transformation 1 0 0 1 0 0 ϕ = 0 1 1 ϕ 0 1 1 (a = 1,2,...,12) . a  √2 √2  ′a √2 −√2  (19) 0 1 1 0 1 1 −√2 √2 √2 √2     3 3 3 Then, one obtains twelve new × matri es also forming an irredu ible representation A 4 of : 1 0 0 1 0 0 1 0 0 1 0 0 − − ϕ = 0 1 0 , ϕ = 0 0 1 , ϕ = 0 1 0 , ϕ = 0 0 1 , 1 2 3 4    −   −    0 0 1 0 1 0 0 0 1 0 1 0 − −         0 1 1 0 1 1 1 ± ∓ 1 ± ∓ ϕ = 1 1 1 , ϕ = 1 1 1 , 5,8 √2 ± √2 √2  6,7 √2 ∓ −√2 −√2  1 1 1 1 1 1 ± −√2 −√2 ∓ √2 √2     0 1 1 0 1 1 1 ± ± 1 ∓ ∓ ϕ = 1 1 1 , ϕ = 1 1 1 . 9,10 √2 ± √2 −√2  11,12 √2 ± −√2 √2  (20) 1 1 1 1 1 1 ∓ √2 −√2 ∓ −√2 √2     Noti e the identities 6 ϕT = ϕ , ϕT = ϕ , ϕT = ϕ , ϕT = ϕ 5 9 6 11 7 12 8 10 (21) and ϕ +ϕ +ϕ +ϕ = 0 , 1 2 3 4 ϕ +ϕ +ϕ +ϕ = 0 , 5 6 7 8 ϕ +ϕ +ϕ +ϕ = 0 , 9 10 11 12 (22) as well as 1 0 0 0 0 0 1 1 (ϕ ϕ ) = 0 1 1 , (ϕ +ϕ ) = 0 1 1 , 2 1 − 4  2 −2  2 1 4  2 2  0 1 1 0 1 1 −2 2 2 2     1 0 0 1 − (ϕ ϕ ) = 0 1 1 2 2 − 3  2 −2  (23) 0 1 1 −2 2   and 0 1 1 1 1 − 1 (ϕ +ϕ +ϕ +ϕ ) = 1 0 0 = (λ λ ). 5 6 9 11 1 4 2 √2   √2 − (24) 1 0 0 −   (λ λ )/√2 ϕ ϕ ϕ ϕ 1 4 1 4 2 3 The matrix − ommutes with and , and anti ommutes with and . c = 1/√2 = s c = 0 s = 1 23 23 atm atm In the ase of (i.e., and ), the e(cid:27)e tive neutrino mass matrix (2) takes the form 1 0 0 0 0 0 m +m M = 1 2 0 1 1 + m 0 1 1 2  2 2  3 2 2  0 1 1 0 1 1 −2 2 2 2  1 0 0   0 1 1 + m2 −m1 c −0 1 1 +s 1 1 0 −0 . 2  sol 2 −2  sol√2   (25) 0 1 1 1 0 0 −2 2 −      Thus, making use of Eqs. (23) and (24), one an write m +m 1 1 1 2 M = (ϕ ϕ )+m (ϕ +ϕ ) 1 4 3 1 4 2 2 − 2 m m 1 2 1 + − [c (ϕ ϕ )+s (ϕ +ϕ +ϕ +ϕ )] . sol 2 3 sol 5 6 9 11 2 2 − (26) 7 Here, the identities ϕ +ϕ = (ϕ +ϕ ) , ϕ +ϕ +ϕ +ϕ = (ϕ +ϕ +ϕ +ϕ ) 1 4 2 3 5 6 9 11 7 8 10 12 − − (27) hold due to Eqs. (22). 1(m +m ) m 1(m m ) In the formula (26) there appear at 2 1 2 , 3 and 2 2− 1 three ommuting 3 3 ϕ a ombinations of eight (from twelve) × matri es given in Eqs. (20). In the third ϕ ϕ ϕ +ϕ +ϕ + 2 3 5 6 9 ombination there are two anti ommuting omponents sin e − and ϕ = (λ λ )√2 M 11 1 4 − anti ommute. For the e(cid:27)e tive neutrino mass matrix all these ombinations play the role of dynami al variables. M m m 2 1 In on lusion, one an see from Eq. (26) that the term of proportional to − A 3 3 4 is fully onstru ted from elements of the group embedding the four-group: the × λ λ A 1 4 4 matrix − lies inside the group . As an be inferred from an analogi al dis ussion D 4 for the dihedral group of the order eight, also embedding the four-group, the term of M m m D 3 3 2 1 4 proportional to − is not fully built up from elements of the group : the × λ λ D D 1 4 4 4 matrix − lies outside the group ( f. Appendix in Ref. [4℄). The group was applied to the neutrino mass matrix in Refs. [6℄. Of ourse, in the simple ase of four-group as well as in the more involved ases of A D λ λ M 4 4 1 4 group and group , the matrix − appearing in the term of proportional to m m M ϕ 2 1 2 − violates the invarian e of under the transformations generated by matri es ϕ m m 0 c = 1/√2 = s 3 2 1 23 23 and , unless the limitof − → is onsidered ( f. Eq. (8) with ). As is well known, the neutrino mass matrix, being nonzero, breaks the ele troweak SU(2) U(1) gaugesymmetry × asdothemassmatri esof hargedleptonsaswellasupand down quarks. Thus, it is natural to expe t that, in general, the e(cid:27)e tive family dis rete symmetries of fermion mass matri es (cid:22) appearing after the ele troweak symmetry is broken (cid:22) do not preserve the ele troweak symmetry. In parti ular, the e(cid:27)e tive family Z Z ϕ ϕ 2 2 2 3 symmetry × of neutrino mass matrixworks: under and transformationsinthe m = m ϕ ϕ 2 1 1 4 limit of , and always under and transformations. But, at the same time, in the (cid:29)avor representation, the harged-lepton mass matrix is diagonal with the entries m m m ϕ ϕ e µ τ 2 4 ≪ ≪ ex luding its potential invarian e under and transformations valid m = m c s ϕ τ µ atm atm 1 only at (for any and ), though it is always invariant under diagonal ϕ 3 and transformations. 8 Referen es [1℄ M. Apollonio et al. (Chooz Collaboration), Eur. Phys. J. C 27, 331 (2003). [2℄ For a re ent review f. M. Maltoni et al., hep(cid:21)ph/0405172; M.C. Gonzalez-Gar ia, hep(cid:21)ph/0410030; G. Altarelli, hep(cid:21)ph/0410101. [3℄ E.P. Wigner, Group theory and its appli ation to the quantum me hani s of atomi spe tra, A ademi Press, New York and London, 1959; B. Simon, Representations of (cid:28)nite and ompa t groups, Ameri an Mathemati al So iety,1996. [4℄ W. Królikowski, hep(cid:21)ph/0410257 (to appear in A ta Phys. Pol. B , where Appendix is added); and referen es therein. [5℄ E. Ma, hep(cid:21)ph/0307016; hep(cid:21)ph/0409075; and referen es therein. [6℄ W. Grimus, L. Lavoura, A ta Phys. Pol., B 34, 5393 (2003); W. Grimus, A.S. Yoshi- pura,S.Kaneko,L.Lavoura,M.Tanimoto,hep(cid:21)ph/0407112;W.Grimus,A.S.Yoshipura, S. Kaneko, L. Lavoura, H. Savanaka, M. Tanimoto, hep(cid:21)ph/0408123; and referen es therein. 9

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.