NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING

Size: px
Start display at page:

Download "NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING"

Transcription

1 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING ALAIN CONNES Abstract. We show that allowing the metric dimension of a space to be independent of its KO-dimension and turning the finite noncommutative geometry F whose product with classical 4-dimensional space-time gives the standard model coupled with gravity into a space of KO-dimension 6 by changing the grading on the antiparticle sector into its opposite, allows to solve three problems of the previous noncommutative geometry interpretation of the standard model of particle physics: The finite geometry F is no longer put in by hand but a conceptual understanding of its structure and a classification of its metrics is given. The fermion doubling problem in the fermionic part of the action is resolved. The spectral action of our joint work with Chamseddine now automatically generates the full standard model coupled with gravity with neutrino mixing and see-saw mechanism for neutrino masses. The predictions of the Weinberg angle and the Higgs scattering parameter at unification scale are the same as in our joint work but we also find a mass relation (to be imposed at unification scale).. Introduction We showed some time ago (cf. [6]) how to interpret the Lagrangian of the standard model in terms of noncommutative geometry. This interpretation was based on the extension of the Yang-Mills functional to the algebraic framework of NCG. In [6] the color degrees of freedom were still added in an artificial manner and the action functional was obtained by analogy with the classical gauge theories. In our joint work with A. Chamseddine [], [2] and in [8] we showed how to incorporate the color naturally and more importantly how to obtain the bosonic part of the standard model action coupled to gravity from a very general spectral action principle. We call it a principle since it is based on the very general idea that a refined notion of geometry (suitable in particular to deal with spaces whose coordinates do not commute) is obtained by focussing not on the traditional g µν but on the Dirac operator D. As it turns out this way of defining a geometry by specifying the Dirac operator is meaningful both in mathematical terms (where the Dirac operator specifies the fundamental class in KO-homology) and in physics terms (where, modulo a chiral gauge transformation, the Dirac operator is the inverse of the Euclidean propagator of fermions). The spectral action principle then asserts that D is all that is needed to define the bosonic part of the action. Moreover since disjoint union of spaces correspond to direct sums of the Dirac operators, a simple additivity requirement of the action functional shows that it has to be of the form () S = Tr(f(D/Λ))

2 2 ALAIN CONNES where f is an even function of the real variable and Λ a parameter fixing the mass scale. In fact the choice of the test function f only plays a small role since when expanded in inverse powers of Λ the action S only depends on the first moments f(u) u k du and the Taylor expansion of f at 0. Not surprisingly the gravitational Einstein action appears naturally in the expansion of S, a point which is reminiscent of the idea of induced gravity. Moreover in the presence of gauge fields A the operator D gets modified (replacing derivatives by covariant derivatives) to D A and the Yang-Mills action functional YM(A) appears, in its Euclidean form and with the correct sign if f 0, in the coefficient of Λ 0 in the spectral action () for the operator D A. The simple idea developed in [], then, is that one should understand the modification D D A coming from the presence of gauge fields as a slight change in the metric, while the action principle () which is in essence purely gravitational delivers when applied to D A the combined Einstein-Yang-Mills action. To keep track of the change of metric coming from the gauge fields one needs to enhance the algebra of coordinates on the manifold M to the algebra of matrix valued functions on M which encodes the gauge group as its group of inner automorphisms. We refer to section 2 of [2] for the case of an SU(n) theory. The advantage in passing to noncommutative algebras of coordinates A is that their automorphism group Aut(A) admits a decomposition Inn(A) Aut(A) Out(A) into inner and outer parts, which fits very well with the physics distinction between the internal symmetries g G and the others, i.e. the exact sequence governing the structure of the symmetry group U of the combined Lagrangian of gravity and matter, G U Diff(M) Moreover a similar decomposition into an inner piece and an outer one holds at the level of the noncommutative metric i.e. of the Dirac operator. Thus in the noncommutative world, the metrics (encoded by D) admit natural inner fluctuations which come directly from the self Morita equivalence A A and are encoded by gauge potentials i.e. operators of the form A = a j [D, b j ], a j, b j A, A = A The main result of our joint work [], [2] is that, when applied to the inner fluctuations of the product geometry M F the spectral action gives the standard model coupled with gravity. Here M is a Riemannian compact spin 4-manifold, the standard model coupled with gravity is in the Euclidean form, and the geometry of the finite space F is encoded (as in the general framework of NCG) by a spectral triple (A F, H F, D F ) i.e. by a Hilbert space H F, a representation of the algebra of coordinates A F, and the inverse line element D F. Besides a Z/2 grading γ this spectral triple has a crucial piece of structure: a real structure (cf. [7]) i.e. an antilinear isometry of H of square ± with simple algebraic rules and whose dimension, called the KO-dimension is well defined modulo 8 from the signs involved in the algebraic rules (cf. section 7). For the noncommutative geometry F used in [2] to obtain the standard model coupled to gravity, all the ingredients are finite dimensional. The algebra A F = C H M 3 (C) (i.e. the direct sum of the algebras C of complex numbers, H of quaternions, and M 3 (C) of 3 3 matrices) encodes the gauge group. The Hilbert space H F is of dimension 90 and encodes It is 96 in the model described below

3 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING 3 the elementary quarks and leptons. The operator D F encodes those free parameters of the standard model related to the Yukawa couplings. For M the spectral triple is given by the representation of the algebra of smooth functions acting by multiplication in the Hilbert space L 2 (M, S) of square integrable spinors, the grading is given by γ 5 and the real structure J M is given by charge conjugation. While it is certainly remarkable to obtain the standard model action from simple geometric principles the above work has several shortcomings: () The finite geometry F is put in by hand with no conceptual understanding of the representation of A F in H F. (2) There is a fermion doubling problem (cf. [5]) in the fermionic part of the action. (3) It does not incorporate the neutrino mixing and see-saw mechanism for neutrino masses. We shall show in this note how to solve these three problems (the first only partly since the number of generations is put by hand) simply by keeping the distinction between the following two notions of dimension of a noncommutative space, The metric dimension The KO-dimension The metric dimension manifests itself by the growth of the spectrum of the Dirac operator. As far as space-time goes it appears that the situation of interest will be the 4-dimensional one. In particular the metric dimension of the finite geometry F will be zero. The KO-dimension is only well defined modulo 8 and it takes into account both the Z/2- grading γ of H as well as the real structure J (cf. Appendix 7). The real surprise is that in order for things to work the only needed change (besides the easy addition of a right handed neutrino) is to change the Z/2 grading of the finite geometry F to its opposite in the antiparticle sector. It is only thanks to this that the Fermion doubling problem pointed out in [5] can be successfully handled. Moreover it will automatically generate the full standard model i.e. the model with neutrino mixing and the see-saw mechanism as follows from the full classification of Dirac operators: Theorem 2.7. When one looks at the table (7.) giving the KO-dimension of the finite space F one then finds that its KO-dimension is now equal to 6 modulo 8 (!). As a result we see that the KO-dimension of the product space M F is in fact equal to 0 2 modulo 8. Of course the above 0 is very reminiscent of string theory, in which the finite space F might be a good candidate for an effective compactification at least for low energies 2. But 0 is also 2 modulo 8 which might be related to the observations of [4] about gravity. It is also remarkable that the noncommutative spheres arising from quantum groups, such as the Podleś spheres already exhibit the situation where the metric dimension (0 in that case) is distinct from the KO-dimension (2 in that case) as pointed out in [0]. 2. The finite non commutative geometry F In this section we shall first describe in a conceptual manner the representation of A F in H F and classify the Dirac operators D F. The only small nuance with [8] is that we incorporate a right handed neutrino ν R and change the Z/2 grading in the antiparticle sector to its opposite. 2 Note however that we are dealing with the standard model, not its supersymmetrized version.

4 4 ALAIN CONNES This, innocent as it looks, allows for a better conceptual understanding of the representation of A F in H F and also will completely alter the classification of Dirac operators (Theorem 2.7). 2.. The representation of A F in H F. We start from the involutive algebra (with H the quaternions with involution q q) (2) A LR = C H L H R M 3 (C) We are looking for a natural representation (A LR, H F, J F, γ F ) fulfilling definition 7. in dimension 6 modulo 8. The commutation relation (43) shows that there is an underlying structure of A LR -bimodule on H F and we shall use that structure as a guide. Definition 2.. Let M be an A LR -bimodule. s = (,,, ) fulfills Ad(s) =. Then M is odd iff the adjoint action 3 of Such a bimodule is a representation of the reduction of A LR R A 0 LR by the projection 2 (+s s0 ). This subalgebra is an algebra over C and we restrict to complex representations. One defines the contragredient bimodule of a bimodule M as the complex conjugate space (3) M 0 = { ξ ; ξ M}, a ξ b = b ξ a, a, b A LR We can now give the following characterization of the A LR -bimodule M F and the real structure J F for one generation. Proposition 2.2. The A LR -bimodule M F is the direct sum of all inequivalent irreducible odd A LR -bimodules. The real structure J F is given by the isomorphism with the contragredient bimodule. We define the Z/2-grading γ F by (4) γ F = c J F c J F, c = (0,,, 0) A LR One then checks that the following holds (5) J 2 F =, J F γ F = γ F J F which together with the commutation of J F with the Dirac operators, is characteristic of KO-dimension equal to 6 modulo 8 (cf. definition 7.). The equality ι(λ, q, m) = (λ, q, λ, m) defines a homomorphism ι of involutive algebras from A F to A LR so that we view A F as a subalgebra of A LR. Definition 2.3. The real representation (A F, H F, J F, γ F ) is the restriction to A F A LR of the direct sum M F C 3 of three copies of M F. It has dimension 32 3 = 96, needless to say this 3 is the number of generations and it is put in by hand here. 3 For u A unitary, one defines Ad(u) by Ad(u)ξ = uξu

5 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING The unimodular unitary group SU(A F ). Using the action of A F in H F one defines the unimodular subgroup SU(A F ) of the unitary group U(A F ) = {u A F, uu = u u = } as follows, Definition 2.4. We let SU(A F ) be the subgroup of U(A F ) defined by SU(A F ) = {u U(A F ) : Det(u) = } where Det(u) is the determinant of the action of u in H F. One obtains both the standard model gauge group and its action on fermions from the adjoint action of SU(A F ) in the following way: Proposition 2.5. () The group SU(A F ) is, up to an abelian finite group, SU(A F ) U() SU(2) SU(3) (2) The adjoint action u Ad(u) (cf. (47)) of SU(A F ) in H F coincides with the standard model action on elementary quarks and leptons. To see what happens we first have to label the basis of the bimodule M F. following idempotents in A LR, (6) e l = (, 0, 0, 0), e L = (0,, 0, 0), e R = (0, 0,, 0), e q = (0, 0, 0, ). We use the The reduced algebras are respectively C, H L, H R, M 3 (C). One has e j = and similarly in the algebra A LR A 0 LR one has ej e 0 k = Using the action of A LR A 0 LR associated to the bimodule structure of M thus gives a decomposition of the form M = e j M e k Since M is odd this decomposition can be written as M = e j M e K + e J M e k Let us consider the term e L M e l. It is a H L -left, C-right module. Thus it is a multiple of the only irreducible representation π L of H L which is two dimensional. The action of C is given by the scalar action. Let us consider the term e L M e q. It is a H L -left, M 3 (C)-right module. Since the algebra H L R M 3 (C) is M 6 (C) we see that all such bimodules are multiples of the bimodule π 3 L given for the left action of H L as the direct sum of three copies of π L and with the obvious right action of M 3 (C) permuting the three copies. Exactly the same holds for the bimodules e R M e l and e R M e q, which are respectively multiples of π R and of π 3 R. Similar results hold switching the left and right actions i.e. by passing to the contragredient bimodule of M. We thus see that the sum of the irreducible odd bimodules is given by (7) M F = (π L π R π 3 R π 3 L) (π L π R π 3 R π 3 L) 0 This A LR -bimodule M F is of dimension 2 ( ) = 32 and the adjoint action gives the gauge action of the standard model for one generation, with the following labels for the basis elements of M F, ( νl ν R e L e R )

6 6 ALAIN CONNES for the term π L π R, ( u j L d j L for the term πr 3 π3 L ( with color indices j) and the transformation q q to pass to the contragredient bimodules. With these labels one checks that the adjoint action of the U() factor is given by multiplication of the basis vectors f by the following powers of λ U(): uj R dj R ) e ν u d f L 3 3 f R The classification of Dirac operators. To be precise we adopt the following, Definition 2.6. A Dirac operator is a self-adjoint operator D in H F commuting with J F, C F = {(λ, λ, 0)} A F, anticommuting with γ F and fulfilling the order one condition [[D, a], b 0 ] = 0 for any a, b A F. In order to state the classification of Dirac operators we introduce the following notation, let M e, M ν, M d, M u and M R be three by three matrices, we then let D(M) be the operator in H F given by [ ] S T (8) D(M) = T S where (9) S = S l (S q 3 ) and in the basis (ν R, e R, ν L, e L ) and (u R, d R, u L, d L ), 0 0 M ν M (0) S l = Me u 0 M ν S q = Md M u M e M d 0 0 while the operator T is 0 except on the subspace H νr H F with basis the ν R which it maps, using the matrix M R, to the subspace H νr H F with basis the ν R. Theorem 2.7. () Let D be a Dirac operator. There exists three by three matrices M e, M ν, M d, M u and M R, with M R symmetric, such that D = D(M). (2) All operators D(M) (with M R symmetric) are Dirac operators. (3) The operators D(M) and D(M ) are conjugate by a unitary operator commuting with A F, γ F and J F iff there exists unitary matrices V j and W j such that M e = V M e V3, M ν = V 2 M ν V3, M d = W M d W3, M u = W 2 M u W3, M R = V 2 M R V 2 In particular Theorem 2.7 shows that the Dirac operators give all the required features, such as Mixing matrices for quarks and leptons Unbroken color

7 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING 7 See-saw mechanism for right handed neutrinos Let us briefly explain the last item, i.e. the analogue of the seesaw mechanism in our context. The restriction of D(M) to the subspace of H F with basis the (ν R, ν L, ν R, ν L ) is given by the matrix, () 0 M ν M R 0 M ν M R 0 0 M ν 0 0 Mν 0 Let us simplify to one generation and let M R M be a very large mass term- the largest eigenvalue of M R will be set to the order of the unification scale by the equations of motion (40) of the spectral action below- while M ν m is much smaller 4. The eigenvalues of the matrix () are then given by 2 (±M ± M 2 + 4m 2 ) which gives two eigenvalues very close to ±M and two others very close to ± m2 M as can be checked directly from the determinant of the matrix (), which is equal to M ν 4 m 4 (for one generation). 3. The spectral action for M F and the Standard Model We now consider a 4-dimensional smooth compact Riemannian manifold M with a fixed spin structure and consider its product with the above finite geometry. With (A j, H j, γ j ) of KO-dimensions 4 for j = and 6 for j = 2, the product geometry is given by the rules, A = A A 2, H = H H 2, D = D + γ D 2, γ = γ γ 2, J = J J 2 Note that it matters that J commutes with γ to check that J commutes with D. The KO-dimension of the finite space F is 6 Z/8 and thus the KO-dimension of the product geometry M F is now 2 Z/8. In other words according to definition 7. the commutation rules are (2) J 2 =, JD = DJ, and Jγ = γj. Let us now explain how these rules allow to define a natural antisymmetric bilinear form on the even part H + = {ξ H, γ ξ = ξ} of H. Proposition 3.. On a real spectral triple of KO-dimension 2 Z/8, the following equality defines an antisymmetric bilinear form on H + = {ξ H, γ ξ = ξ}, (3) A D (ξ, ξ) = J ξ, D ξ, ξ, ξ H + The above trilinear pairing between D, ξ and ξ is gauge invariant under the adjoint action (cf. (47)) of the unitary group of A, (4) A D (ξ, ξ) = A Du (Ad(u)ξ, Ad(u)ξ), D u = Ad(u) D Ad(u ) 4 it is a Dirac mass term, fixed by the Higgs vev

8 8 ALAIN CONNES Now the Pfaffian of an antisymmetric bilinear form is best expressed in terms of the functional integral involving anticommuting classical fermions which at the formal level means that Pf(A) = e 2 A(ξ) D[ξ] It is the use of the Pfaffian as a square root of the determinant that allows to solve the Fermion doubling puzzle which was pointed out in [5]. The solution obtained by a better choice of the KO-dimension of the space F and hence of M F is not unrelated to the point made in []. Theorem 3.2. Let M be a Riemannian spin 4-manifold and F the finite noncommutative geometry of KO-dimension 6 described above. Let M F be endowed with the product metric. () The unimodular subgroup of the unitary group acting by the adjoint representation Ad(u) in H is the group of gauge transformations of SM. (2) The unimodular inner fluctuations A of the metric (cf. (49)) are parameterized exactly by the gauge bosons of SM (including the Higgs doublet). (3) The full standard model (see the explicit formula in 5) minimally coupled with Einstein gravity is given in Euclidean form by the action functional 56 S = Tr(f(D A /Λ)) + 2 J ξ, D A ξ, ξ H + applied to unimodular inner fluctuations D A = D + A + JAJ of the metric. The proof is an excruciating computation, which is a variant of [2] (cf. [2] for a detailed version). After turning of gravity to simplify and working in flat space (after Wick rotation back to Lorentzian signature) one gets exactly the Lagrangian of 5 which can hardly be fortuitous. The fermion doubling problem is resolved by the use of the Pfaffian, we checked that part for the Dirac mass terms, and trust that the same holds for the Majorana mass terms. There is one subtle point which is the use of the following chiral transformation: U = e i π 4 γ 5 to transform the fermionic part of the action to the traditional one i.e. the Euclidean action for Fermi fields (cf. [5]). While this transformation is innocent at the classical level, it is non-trivial at the quantum level and introduces some kind of Maslov index in the transition from our form of the Euclidean action to the more traditional one. We shall now give more details on the bosonic part of the action. 4. Detailed form of the Bosonic action We shall now give the precise form of the bosonic action, the calculation is entirely similar to [2] with new terms appearing from the presence of M R. 5 We take f 0 and f (n) (0) = 0 for n for definiteness 6 the components of ξ anticommute so the antisymmetric form does not vanish

9 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING 9 One lets f k = f(u) u k du for k > 0 and = f(0). Also (5) a = Tr(Mν M ν + Me M e + 3(MuM u + Md M d)) b = Tr((Mν M ν ) 2 + (Me M e ) 2 + 3(MuM u ) 2 + 3(Md M d) 2 ) c = Tr(MRM R ) d = Tr((MRM R ) 2 ) e = Tr(MRM R Mν M ν ) The spectral action is given by a computation entirely similar to [2] which yields: (6) S = π 2 (48 f 4 Λ 4 f 2 Λ 2 c + f 0 g 4 d) d 4 x + 96 f 2 Λ 2 c 24π 2 R g d 4 x + 0 π 2 ( 6 R R 3 C µνρσ C µνρσ ) g d 4 x + ( 2 a f 2 Λ 2 + e ) π 2 ϕ 2 g d 4 x + 2 π 2 a D µ ϕ 2 g d 4 x 2 π 2 a R ϕ 2 g d 4 x + 2 π 2 (g3 2 G i µν G µνi + g2 2 Fµν α F µνα g2 B µν B µν ) g d 4 x + 2 π 2 b ϕ 4 g d 4 x where (a, b, c, d, e) are defined above and D µ ϕ is the minimal coupling. A simple change of variables as in [2], namely (7) H = a f0 ϕ, π so that the kinetic term becomes 7 and 2 D µh 2 g d 4 x (8) g 2 3 2π 2 = 4, g2 3 = g 2 2 = 5 3 g2. 7 here we differ slightly from [2] by a factor of 2 to match the conventions of Veltman [7]

10 0 ALAIN CONNES transforms the bosonic action into the form: S = d 4 x [ (9) g R + α 0 C µνρσ C µνρσ where (20) (2) (22) (23) (24) (25) (26) 2κ γ 0 + τ 0 R R + δ 0 R; µ µ + 4 Gi µν G µνi + 4 F µν α F µνα + 4 B µν B µν + 2 D µ H 2 µ 2 0 H 2 ] 2 R H 2 + λ 0 H 4 κ 2 0 = 96 f 2 Λ 2 c 2 π 2 µ 2 0 = 2 f 2 Λ 2 e a α 0 = 3 0 π 2 τ 0 = 60 π 2 δ 0 = 2 3 α 0 γ 0 = π 2 (48 f 4 Λ 4 f 2 Λ 2 c + 4 d) λ 0 = π2 b 2 a 2 = b g2 a 2 5. Detailed form of the spectral action without gravity To make the comparison easier we Wick rotate back to Minkowski space and after turning off gravity by working in flat space (and addition of gauge fixing terms 8 ) the spectral action, after the change of variables summarized in table, is given by the following formula: L SM = 2 νgµ a ν gµ a g s f abc µ gνg a µg b ν c 4 g2 sf abc f ade gµg b νg c µg d ν e ν W µ + ν Wµ M 2 W µ + Wµ 2 νzµ 0 ν Zµ 0 M 2 Z 2c µz 0 2 µ 0 w 2 µa ν µ A ν igc w ( ν Zµ(W 0 µ + Wν W ν + Wµ ) Zν(W 0 µ + ν Wµ Wµ ν W µ + ) + Zµ(W 0 ν + ν Wµ Wν ν W µ + )) igs w ( ν A µ (W µ + Wν W ν + Wµ ) A ν (W µ + ν Wµ Wµ ν W µ + ) + A µ (W ν + ν Wµ Wν ν W µ + )) 2 g2 W µ + Wµ W ν + Wν + 2 g2 W µ + Wν W µ + Wν + g 2 c 2 w(zµw 0 µ + ZνW 0 ν ZµZ 0 µw 0 ν + Wν ) + g 2 s 2 w(a µ W µ + A ν Wν A µ A µ W ν + Wν ) + g 2 s w c w (A µ Zν(W 0 µ + Wν W ν + Wµ ) 2A µ ZµW 0 ν + Wν ) 2 µh µ H 2M 2 α h H 2 µ φ + µ φ 2 µφ 0 µ φ 0 ( ) β 2M 2 h + 2M g 2 g H + 2 (H2 + φ 0 φ 0 + 2φ + φ ) + 2M 4 α g 2 h gα h M ( H 3 + Hφ 0 φ 0 + 2Hφ + φ ) ( 8 g2 α h H 4 + (φ 0 ) 4 + 4(φ + φ ) 2 + 4(φ 0 ) 2 φ + φ + 4H 2 φ + φ + 2(φ 0 ) 2 H 2) gmw µ + Wµ H 2 g M Z c µz 0 µh 0 2 w 2 ig ( W µ + (φ 0 µ φ φ µ φ 0 ) Wµ (φ 0 µ φ + φ + µ φ 0 ) ) + 2 g ( W µ + (H µ φ φ µ H) + Wµ (H µ φ + φ + µ H) ) + 2 g c w (Zµ(H 0 µ φ 0 φ 0 µ H) + M ( c w Zµ 0 µ φ 0 + W µ + µ φ + Wµ µ φ + ) ig s2 w cw MZµ(W 0 µ + φ Wµ φ + ) + igs w MA µ (W µ + φ 8 We add the Feynman gauge fixing terms just to simplify the form of the gauge kinetic terms

11 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING Wµ φ + ) ig 2c2 w 2c w Zµ(φ 0 + µ φ φ µ φ + ) + igs w A µ (φ + µ φ φ µ φ + ) 4 g2 W µ + Wµ ( H 2 + (φ 0 ) 2 + 2φ + φ ) 8 g2 Z c µz 0 0 ( 2 µ H 2 + (φ 0 ) 2 + 2(2s 2 w ) 2 φ + φ ) w 2 g2 s 2 w cw Zµφ 0 0 (W µ + φ + Wµ φ + ) 2 ig2 s 2 w cw ZµH(W 0 µ + φ Wµ φ + ) + 2 g2 s w A µ φ 0 (W µ + φ + Wµ φ + ) + 2 ig2 s w A µ H(W µ + φ Wµ φ + ) g 2 s w cw (2c 2 w )ZµA 0 µ φ + φ g 2 s 2 wa µ A µ φ + φ + 2 ig s λ a ij ( qσ i γµ qj σ)ga µ ē λ (γ + m λ e )e λ ν λ (γ + m λ ν)ν λ ū ( λ j (γ + mλ u)u λ j d λ j (γ + mλ d )dλ j + igs w A µ (ē λ γ µ e λ ) (ūλ j γµ u λ j ) 3 ( d ) λ j γµ d λ j ) + ig 4c w Zµ{( ν 0 λ γ µ ( + γ 5 )ν λ ) + (ē λ γ µ (4s 2 w γ 5 )e λ ) + ( d λ j γµ ( 4 3 s2 w γ 5 )d λ j ) + (ūλ j γµ ( 8 3 s2 w + γ 5 )u ) λ j )} + ig 2 W + 2 µ (( ν λ γ µ ( + γ 5 )U lep λκe κ ) + (ū λ j γµ ( + γ 5 )C λκ d κ j ) + ig ((ē κ U lep κλγ µ ( + γ 5 )ν λ ) + ( d ) κ j C κλ γµ ( + γ 5 )u λ j ) + ( ig 2M 2 φ 2 W 2 µ ig ( 2M 2 φ+ m κ e ( ν λ U lep λκ( γ 5 )e κ ) + m λ ν( ν λ U lep λκ( + γ 5 )e κ) + ) m λ e (ē λ U lep λκ( + γ 5 )ν κ ) m κ ν(ē λ U lep λκ( γ 5 )ν κ g 2 g m λ e 2 M H(ēλ e λ ) + ig m λ ν 2 M φ0 ( ν λ γ 5 ν λ ) ig m λ e 2 4 ν λ Mλκ R ( γ 5)ˆν κ + ig m λ ν M H( νλ ν λ ) M φ0 (ē λ γ 5 e λ ) 4 ν λ M R λκ ( γ 5)ˆν κ ( m 2M 2 φ+ κ d (ūλ j C λκ( γ 5 )d κ j ) + mλ u(ū λ j C λκ( + γ 5 )d κ j ig (m 2M 2 φ λ d ( d λ j C λκ ( + γ5 )u κ j ) mκ u( d ) λ j C λκ ( γ5 )u κ j g m λ u 2 M H(ūλ j uλ j ) g 2 ig m λ u 2 M φ0 (ū λ j γ5 u λ j ) ig 2 m λ d M φ0 ( d λ j γ5 d λ j ) ) + m λ d M H( d λ j dλ j ) + This formula compares nicely with [7]. Besides the addition of the neutrino mass terms, and absence of the ghost terms there is only one difference: in the spectral action Lagrangian one gets the term: (27) M ( c w Z 0 µ µ φ 0 + W + µ µ φ + W µ µ φ + ) while in the Veltman s formula [7] one gets instead the following: (28) M 2 φ + φ 2c 2 M 2 φ 0 φ 0 w This difference comes from the gauge fixing term (29) L fix = 2 C2, C a = µ W µ a + M a φ a given by the Feynman-t Hooft gauge in Veltman s formula [7], indeed one has (30) L fix = 2 ( µw a µ ) 2 2c 2 M 2 φ 0 φ 0 M 2 φ + φ +M ( φ 0 µ Zµ 0 +φ µ W µ + +φ + µ Wµ ) w c w The numerical values are similar to those of [2] and in particular one gets the same value of gauge couplings as in grand unified SU(5)-theory. This means that in the above formula the values of g, g s and s w, c w are fixed exactly as in [2] at (3) g s = g, tg(w) 2 = 3 5 One also gets a specific value of the Higgs scattering parameter α h, as in [2] (which agrees with [3]), (32) α h = 8 b a 2

12 2 ALAIN CONNES (with the notations (5)) which is of the order of 8 3 if there is a dominating top mass. The change of notations for the Higgs fields is (33) H = 2 a g ( + ψ) = (2M g + H iφ0, i 2φ + ), while the huge term in Λ 2 in the spectral action can be absorbed by a suitable choice of the tadpole constant β h (34) β h = 2α h M 2 4 f 2Λ e a Note that the matrices M u, M d, M ν and M e are only relevant up to an overall scale. Indeed they only enter in the coupling of the Higgs with fermions and because of the rescaling (7) only by the terms (35) k x = π M x, x {u, d, ν, e} a f0 which are dimensionless matrices by construction. The conversion for the mass matrices is (36) (k u ) λκ = g 2M mλ u δλ κ (k d ) λκ = g 2M mµ d C λµδµc ρ ρκ (k ν ) λκ = g 2M mλ ν δλ κ (k e ) λκ = g 2M mµ e U lep λµδµu ρ lep ρκ It might seem at first sight that one can simply use (36) to define the matrices k x but this overlooks the fact that (35) implies one constraint: (37) Tr(k νk ν + k ek e + 3(k uk u + k d k d)) = 2 g 2, using (8) to replace π2 by 2 g 2. When expressed in the right hand side i.e. the standard model parameters this gives (38) (m λ ν) 2 + (m λ e ) (m λ u) (m λ d )2 = 8 M 2 λ where M is the mass of the W boson. Thus with the standard notation ([3]) for the Yukawa couplings, so that the fermion masses are m f = 2 y f v, v = 2M g the relation reads (39) (yν λ ) 2 + (ye λ ) (yu) λ (yd λ )2 = 4 g 2 λ Neglecting the other Yukawa coupling except for the top quark, and imposing the relation (39) at unification scale, then running it downwards using the renormalization group one gets the boundary value 2 3 g for y t at unification scale which gives a Fermi scale value of the order of z =.4 and a top quark mass of the order of 2 z v z GeV. This is fine since large neglected tau neutrino Yukawa couplings (corresponding to the see-saw 3 mechanism) would tend to lower this value by a factor of 4 z. The conversion table shows that all the mass parameters of the standard model now acquire geometric meaning as components of the noncommutative metric as displayed in the right column.

13 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING 3 Standard Model notation notation Spectral Action Higgs Boson ϕ = ( 2M g + H iφ 0, i 2φ + ) H = a 2 g ( + ψ) Inner metric(0,) Gauge bosons A µ, Z 0 µ, W ± µ, g a µ (B, W, V ) Inner metric (,0) Fermion masses m u, m ν M u = δ u, M ν = δ ν Dirac (0,) in u, ν u, ν CKM matrix C κ λ, m d M d = C δ d C Dirac (0,) in d Masses down Lepton mixing U lep λκ, m e M e = U lep δ e U lep Dirac (0,) in e Masses leptons e Majorana M R M R Dirac (0,) in ν R, ν R mass matrix Gauge couplings g = g tg(w), g 2 = g, g 3 = g s g 2 3 = g2 2 = 5 3 g2 Fixed at unification Higgs scattering 8 g2 α h, α h = m2 h λ 4M 2 0 = g 2 b parameter a 2 Fixed at unification Tadpole constant β h, ( α h M 2 + β h 2 ) ϕ 2 µ 2 0 = 2 f 2Λ 2 e a µ 2 0 H 2 Graviton g µν / M Dirac (,0) Table. Conversion from Spectral Action to Standard Model 6. Interpretation It is not clear what the physics meaning is since unlike in grand unified theories one is still lacking a renormalizable theory that would take over above the unification energy. But one can nevertheless hope that such a theory will be discovered along the lines of QFT on noncommutative spaces, or even that the fundamental theory has selected a preferred scale and is a fully unified theory at the operator theoretic level (i.e. a kind of spectral random matrix theory where the operator D varies in the symplectic ensemble corresponding to the commutation with i = and J that generate the quaternions) of which the standard model coupled with gravity is just a manifestation when one integrates the high energy modes á la

14 4 ALAIN CONNES Wilson. Then following [2] one can take the value of the Higgs quartic self-coupling (32) as an indication at that same energy and ([3]) get a rough estimate (in the range GeV) for the Higgs mass under the big desert hypothesis. It is satisfactory that the prediction for the Weinberg angle (the same as SU(5) GUT) is not too far off and that the mass relation gives a sensible answer. But it is of course very likely that instead of the big desert one will meet gradual refinements of the noncommutative geometry M F when climbing in energy to the unification scale. The naturalness problem is of course still there, but interestingly the new terms involving M R provide room for obtaining in the spectral action a term that mimics the nasty quadratic divergence, whose coefficient changes sign under the running of the remormalization group. This freedom holds provided that the number of generations is >. The quadratic coupling is µ 2 0 = 2 f 2 Λ 2 e a. The presence of the new term e a (which was absent in [2]) allows for the possibility that the sign of this mass term is arbitrary provided there are at least two generations. We shall assume to discuss this point that the matrix M R is a multiple of a fixed matrix k R i.e. is of the form M R = x k R. The value of x is fixed by the equations of motion of the spectral action i.e. by minimizing the cosmological term. It gives (40) x 2 = 2 f 2 Λ 2 Tr(kR k R) Tr((kR k R) 2 ), M RM R = 2 f 2 Λ 2 kr k R Tr(kR k R) Tr((kR k R) 2 ) Using (40) and (35) one gets (4) µ 2 0 = 2 Λ 2 f 2 ( X), X = Tr(k R k R k νk ν ) Tr(k R k R) Tr(k νk ν + k ek e + 3(k uk u + k d k d))tr((k R k R) 2 ) In order to compare X with we need to determine the range of variation of the largest eigenvalue of ρ(k R ) = k R k R Tr(kR k R) Tr((kR k as a function of the number N of generations. One finds R) 2 ) that this range of variation, for k R M N (C), is the interval [, 2 ( + N)] This suffices to show that provided the number N of generations is >, there is room to get a small value of µ 2 0. Note that a similar discussion applies to the cosmological term γ 0 which inherits a negative contribution from the presence of the M R term. 7. Appendix: Real Structure We just briefly recall here the definition of a real structure (cf. [7]) on a spectral triple (A, H, D), Definition 7.. A real structure of KO-dimension n Z/8 on a spectral triple (A, H, D) is an antilinear isometry J : H H, with the property that (42) J 2 = ε, JD = ε DJ, and Jγ = ε γj (even case). The numbers ε, ε, ε {, } are a function of n mod 8 given by n ε ε - - ε - -

15 NONCOMMUTATIVE GEOMETRY AND THE STANDARD MODEL WITH NEUTRINO MIXING 5 Moreover, the action of A satisfies the commutation rule (43) [a, b 0 ] = 0 a, b A, where (44) b 0 = Jb J b A, and the operator D satisfies (45) [[D, a], b 0 ] = 0 a, b A. The key role of the real structure J is to yield the following adjoint action of the unitary group U of the algebra A on the hilbert space H (of spinors). One defines a right A-module structure on H by (46) ξ b = b 0 ξ, ξ H, b A The unitary group of the algebra A then acts by the adjoint representation in H in the form (47) ξ H Ad(u) ξ = u ξ u, ξ H, u A, u u = u u =, and the inner fluctuation of the metric is given by (48) D D A = D + A + ε J A J where A is a self-adjoint operator of the form (49) A = a j [D, b j ], a j, b j A. The unimodular inner fluctuations are obtained by restricting to those A which are traceless i.e. fulfill the condition Tr(A) = Aknowledgements The detailed computations and extension of this work to the left-right model will appear in a joint work with Ali Chamseddine and Matilde Marcolli. The need to have independence between the KO-dimension and the metric dimension already emerged implicitly in the work of L. D abrowski and A. Sitarz on Podleś quantum spheres [0]. The results of this work were announced in a talk at the Newton Institute in July 2006, and the fear of a numerical error in the above computations delayed the present publication. It is a pleasure to acknowledge the independent preprint by John Barrett (A Lorentzian version of the non-commutative geometry of the standard model of particle physics) with a similar solution of the fermion doubling problem which accelerated the present publication. References [] A. Chamseddine, A. Connes, Universal Formula for Noncommutative Geometry Actions: Unification of Gravity and the Standard Model, Phys. Rev. Lett. 77, (996). [2] A. Chamseddine, A. Connes, The Spectral Action Principle, Comm. Math. Phys. 86, (997). [3] A. Chamseddine, A. Connes, Scale Invariance in the Spectral Action, hep-th/05269 to appear in Jour. Math. Phys [4] A. Chamseddine, A. Connes, Inner fluctuations of the spectral action, hep-th/ [5] S. Coleman, Aspects of symmetry, Selected Erice Lectures, Cambridge University Press, 985. [6] A. Connes, Noncommutative geometry, Academic Press (994). [7] A. Connes, Non commutative geometry and reality, Journal of Math. Physics 36 no. (995). [8] A. Connes, Gravity coupled with matter and the foundation of noncommutative geometry, Comm. Math. Phys. (995) [9] A. Connes, M. Marcolli Quantum fileds, noncommutative spaces and motives, Book in preparation.

16 6 ALAIN CONNES [0] L. D abrowski, A. Sitarz, Dirac operator on the standard Podleś quantum sphere, Noncommutative Geometry and Quantum Groups, Banach Centre Publications 6, Hajac, P. M. and Pusz, W. (eds.), Warszawa: IMPAN, 2003, pp [] J. Gracia-Bonda, B. Iochum, T. Schucker, The standard model in noncommutative geometry and fermion doubling. Phys. Lett. B 46 no. -2 (998), [2] D. Kastler, Noncommutative geometry and fundamental physical interactions: The Lagrangian level, Journal. Math. Phys. 4 (2000), [3] M. Knecht, T. Schucker Spectral action and big desert hep-ph/06566 [4] O. Lauscher, M. Reuter, Asymptotic Safety in Quantum Einstein Gravity: nonperturbative renormalizability and fractal spacetime structure, hep-th/05260 [5] F. Lizzi, G. Mangano, G. Miele, G. Sparano, Fermion Hilbert space and Fermion Doubling in the Noncommutative Geometry Approach to Gauge Theories hep-th/ [6] R.N. Mohapatra, P.B. Pal, Massive neutrinos in physics and astrophysics, World Scientific, [7] M. Veltman, Diagrammatica: the path to Feynman diagrams, Cambridge Univ. Press, 994.

Noncommutative geometry and the spectral model of space-time

Noncommutative geometry and the spectral model of space-time Séminaire Poincaré X (2007) 79 202 Séminaire Poincaré Noncommutative geometry and the spectral model of space-time Alain Connes IHÉS 35, route de Chartres 9440 Bures-sur-Yvette - France Abstract. This

More information

Duality between shapes and spectra The music of shapes

Duality between shapes and spectra The music of shapes Duality between shapes and spectra The music of shapes A. Connes How to specify our location in space. Vibrations of shapes. Hearing simple shapes. Isospectral shapes and CKM invariant. Towards a musical

More information

The Spectral Geometry of the Standard Model

The Spectral Geometry of the Standard Model Ma148b Spring 2016 Topics in Mathematical Physics References A.H. Chamseddine, A. Connes, M. Marcolli, Gravity and the Standard Model with Neutrino Mixing, Adv. Theor. Math. Phys., Vol.11 (2007) 991 1090

More information

The Spectral Model. A. Connes Leiden, October 2013

The Spectral Model. A. Connes Leiden, October 2013 The Spectral Model Joint work with Ali Chamseddine A. Connes Leiden, October 2013 1 Space-Time Our knowledge of spacetime is described by two existing theories : General Relativity The Standard Model of

More information

The Music of Shapes. Alain Connes. and Viatcheslav Mukhanov. Pisa, September 2014

The Music of Shapes. Alain Connes. and Viatcheslav Mukhanov. Pisa, September 2014 The Music of Shapes Alain Connes Joint work with Ali Chamseddine and Viatcheslav Mukhanov Pisa, September 2014 1 Our goal is to understand the very elaborate Lagrangian given by gravity coupled with the

More information

The Standard Model in Noncommutative Geometry and Morita equivalence

The Standard Model in Noncommutative Geometry and Morita equivalence The Standard Model in Noncommutative Geometry and Morita equivalence Francesco D Andrea e + u u W + ν g d Geometry, Symmetry and Quantum Field Theory Vietri, 30-31 March 2015 The spectral action approach

More information

The Spectral Action and the Standard Model

The Spectral Action and the Standard Model Ma148b Spring 2016 Topics in Mathematical Physics References A.H. Chamseddine, A. Connes, M. Marcolli, Gravity and the Standard Model with Neutrino Mixing, Adv. Theor. Math. Phys., Vol.11 (2007) 991 1090

More information

Summary. Talk based on: Keywords Standard Model, Morita equivalence, spectral triples. Summary of the talk: 1 Spectral action / Spectral triples.

Summary. Talk based on: Keywords Standard Model, Morita equivalence, spectral triples. Summary of the talk: 1 Spectral action / Spectral triples. Summary The Standard Model in Noncommutative Geometry and Morita equivalence Francesco D Andrea 27/02/2017 Talk based on: FD & L. Dabrowski, J. Noncommut. Geom. 10 (2016) 551 578. L. Dabrowski, FD & A.

More information

Spectral Triples and Pati Salam GUT

Spectral Triples and Pati Salam GUT Ma148b Spring 2016 Topics in Mathematical Physics References A.H. Chamseddine, A. Connes, W. van Suijlekom, Beyond the Spectral Standard Model: Emergence of Pati-Salam Unification, JHEP 1311 (2013) 132

More information

The Standard Model in Noncommutative Geometry: fermions as internal Dirac spinors

The Standard Model in Noncommutative Geometry: fermions as internal Dirac spinors 1/21 The Standard Model in Noncommutative Geometry: fermions as internal Dirac spinors Ludwik Dabrowski SISSA, Trieste (I) (based on JNCG in print with F. D Andrea) Corfu, 22 September 2015 Goal Establish

More information

EARLY UNIVERSE MODELS FROM NONCOMMUTATIVE GEOMETRY

EARLY UNIVERSE MODELS FROM NONCOMMUTATIVE GEOMETRY EARLY UNIVERSE MODELS FROM NONCOMMUTATIVE GEOMETRY MATILDE MARCOLLI AND ELENA PIERPAOLI Abstract. We investigate cosmological predictions on the early universe based on the noncommutative geometry models

More information

and the seeds of quantisation

and the seeds of quantisation noncommutative spectral geometry algebra doubling and the seeds of quantisation m.s.,.,, stabile, vitiello, PRD 84 (2011) 045026 mairi sakellariadou king s college london noncommutative spectral geometry

More information

arxiv: v1 [hep-ph] 7 May 2009

arxiv: v1 [hep-ph] 7 May 2009 arxiv:0905.0997v1 [hep-ph] 7 May 9 BEYOND THE STANDARD MODEL: A NONCOMMUTATIVE APPROACH C.A. STEPHAN Institut für Mathematik, Universität Potsdam 14469 Potsdam, Germany During the last two decades Alain

More information

Noncommutative geometry, Grand Symmetry and twisted spectral triple

Noncommutative geometry, Grand Symmetry and twisted spectral triple Journal of Physics: Conference Series PAPER OPEN ACCESS Noncommutative geometry, Grand Symmetry and twisted spectral triple To cite this article: Agostino Devastato 2015 J. Phys.: Conf. Ser. 634 012008

More information

NONCOMMUTATIVE GEOMETRY IN THE LHC-ERA

NONCOMMUTATIVE GEOMETRY IN THE LHC-ERA NONCOMMUTATIVE GEOMETRY IN THE LHC-ERA C.A. STEPHAN Institut für Mathematik, Universität Potsdam, Am Neuen Palais 0, 4469 Potsdam, Germany Noncommutative geometry allows to unify the basic building blocks

More information

BOUNDARY CONDITIONS OF THE RGE FLOW IN THE NONCOMMUTATIVE GEOMETRY APPROACH TO PARTICLE PHYSICS AND COSMOLOGY

BOUNDARY CONDITIONS OF THE RGE FLOW IN THE NONCOMMUTATIVE GEOMETRY APPROACH TO PARTICLE PHYSICS AND COSMOLOGY BOUNDARY CONDITIONS OF THE RGE FLOW IN THE NONCOMMUTATIVE GEOMETRY APPROACH TO PARTICLE PHYSICS AND COSMOLOGY DANIEL KOLODRUBETZ AND MATILDE MARCOLLI Abstract. We investigate the effect of varying boundary

More information

The Standard Model in Noncommutative Geometry: fermions as internal forms

The Standard Model in Noncommutative Geometry: fermions as internal forms 1/35 The Standard Model in Noncommutative Geometry: fermions as internal forms Ludwik Dabrowski (based on JNCG 10 (2016) with F. D Andrea and arxiv:1703.05279 with F. D Andrea and A. Sitarz) Warsaw, 2

More information

!"" #$%&"'()&*+,"-./%*+0/%1"23456""

! #$%&'()&*+,-./%*+0/%123456 BUILDING COSMOLOGICAL MODELS VIA NONCOMMUTATIVE GEOMETRY MATILDE MARCOLLI!"",, " (from Changsha, 1925) #$%&"'()&*+,"-./%*+/%1"23456"" Abstract. This is an overview of new and ongoing research developments

More information

Grand Unification in the Spectral Pati Salam Model

Grand Unification in the Spectral Pati Salam Model Grand Unification in the Spectral Pati Salam Model Ali H Chamseddine 1,3, Alain Connes 2,3,4 and Walter D van Suijlekom 5 1 Physics Department, American University of Beirut, Lebanon 2 College de France,

More information

Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books

Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books Week 3: Renormalizable lagrangians and the Standard model lagrangian 1 Reading material from the books Burgess-Moore, Chapter Weiberg, Chapter 5 Donoghue, Golowich, Holstein Chapter 1, 1 Free field Lagrangians

More information

Pati-Salam unification from noncommutative geometry and the TeV-scale WR boson

Pati-Salam unification from noncommutative geometry and the TeV-scale WR boson Pati-Salam unification from noncommutative geometry and the TeV-scale WR boson Ufuk Aydemir Department of Physics and Astronomy, Uppsala University Collaborators: Djordje Minic, Tatsu Takeuchi, Chen Sun

More information

Spectral action, scale anomaly. and the Higgs-Dilaton potential

Spectral action, scale anomaly. and the Higgs-Dilaton potential Spectral action, scale anomaly and the Higgs-Dilaton potential Fedele Lizzi Università di Napoli Federico II Work in collaboration with A.A. Andrianov (St. Petersburg) and M.A. Kurkov (Napoli) JHEP 1005:057,2010

More information

Reconstruction theorems in noncommutative Riemannian geometry

Reconstruction theorems in noncommutative Riemannian geometry Reconstruction theorems in noncommutative Riemannian geometry Department of Mathematics California Institute of Technology West Coast Operator Algebra Seminar 2012 October 21, 2012 References Published

More information

ASYMPTOTIC SAFETY, HYPERGEOMETRIC FUNCTIONS, AND THE HIGGS MASS IN SPECTRAL ACTION MODELS

ASYMPTOTIC SAFETY, HYPERGEOMETRIC FUNCTIONS, AND THE HIGGS MASS IN SPECTRAL ACTION MODELS ASYMPTOTIC SAFETY, HYPERGEOMETRIC FUNCTIONS, AND THE HIGGS MASS IN SPECTRAL ACTION MODELS CHRISTOPHER ESTRADA AND MATILDE MARCOLLI Abstract. We study the renormalization group flow for the Higgs self coupling

More information

Models of Neutrino Masses

Models of Neutrino Masses Models of Neutrino Masses Fernando Romero López 13.05.2016 1 Introduction and Motivation 3 2 Dirac and Majorana Spinors 4 3 SU(2) L U(1) Y Extensions 11 4 Neutrino masses in R-Parity Violating Supersymmetry

More information

Symmetries, Groups Theory and Lie Algebras in Physics

Symmetries, Groups Theory and Lie Algebras in Physics Symmetries, Groups Theory and Lie Algebras in Physics M.M. Sheikh-Jabbari Symmetries have been the cornerstone of modern physics in the last century. Symmetries are used to classify solutions to physical

More information

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model

November 24, Scalar Dark Matter from Grand Unified Theories. T. Daniel Brennan. Standard Model. Dark Matter. GUTs. Babu- Mohapatra Model Scalar from November 24, 2014 1 2 3 4 5 What is the? Gauge theory that explains strong weak, and electromagnetic forces SU(3) C SU(2) W U(1) Y Each generation (3) has 2 quark flavors (each comes in one

More information

Spectral Triples and Supersymmetry

Spectral Triples and Supersymmetry Ma148b Spring 2016 Topics in Mathematical Physics Reference: Wim Beenakker, Thijs van den Broek, Walter van Suijlekom, Supersymmetry and Noncommutative Geometry, Springer, 2015 (also all images in this

More information

Lecture 7: N = 2 supersymmetric gauge theory

Lecture 7: N = 2 supersymmetric gauge theory Lecture 7: N = 2 supersymmetric gauge theory José D. Edelstein University of Santiago de Compostela SUPERSYMMETRY Santiago de Compostela, November 22, 2012 José D. Edelstein (USC) Lecture 7: N = 2 supersymmetric

More information

Spectral Action from Anomalies

Spectral Action from Anomalies Spectral Action from Anomalies Fedele Lizzi Università di Napoli Federico II and Insitut de Ciencies del Cosmo, Universitat de Barcelona Work in collaboration with A.A. Andrianov & M. Kurkov (St. Petersburg)

More information

arxiv:hep-th/ v1 8 Mar 1996

arxiv:hep-th/ v1 8 Mar 1996 hep-th/9603053 Gravity coupled with matter and the foundation of non commutative geometry Alain CONNES I.H.E.S., 91440 Bures-sur-Yvette, France arxiv:hep-th/9603053 v1 8 Mar 1996 Abstract. We first exhibit

More information

SM predicts massless neutrinos

SM predicts massless neutrinos MASSIVE NEUTRINOS SM predicts massless neutrinos What is the motivation for considering neutrino masses? Is the question of the existence of neutrino masses an isolated one, or is connected to other outstanding

More information

Elementary particles and typical scales in high energy physics

Elementary particles and typical scales in high energy physics Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents

More information

Early Universe Models

Early Universe Models Ma148b Spring 2016 Topics in Mathematical Physics This lecture based on, Elena Pierpaoli, Early universe models from Noncommutative Geometry, Advances in Theoretical and Mathematical Physics, Vol.14 (2010)

More information

THE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE

THE STANDARD MODEL AND THE GENERALIZED COVARIANT DERIVATIVE THE STANDAD MODEL AND THE GENEALIZED COVAIANT DEIVATIVE arxiv:hep-ph/9907480v Jul 999 M. Chaves and H. Morales Escuela de Física, Universidad de Costa ica San José, Costa ica E-mails: mchaves@cariari.ucr.ac.cr,

More information

Introduction to Noncommutative geometry

Introduction to Noncommutative geometry Introduction to Noncommutative geometry Apimook Watcharangool March 19, 2014 1 Abstract The objective of non-commutative geometry(ncg) is to find the link between the spectrum of operator algebra and the

More information

SM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises

SM, EWSB & Higgs. MITP Summer School 2017 Joint Challenges for Cosmology and Colliders. Homework & Exercises SM, EWSB & Higgs MITP Summer School 017 Joint Challenges for Cosmology and Colliders Homework & Exercises Ch!"ophe Grojean Ch!"ophe Grojean DESY (Hamburg) Humboldt University (Berlin) ( christophe.grojean@desy.de

More information

Gauge coupling unification without leptoquarks Mikhail Shaposhnikov

Gauge coupling unification without leptoquarks Mikhail Shaposhnikov Gauge coupling unification without leptoquarks Mikhail Shaposhnikov March 9, 2017 Work with Georgios Karananas, 1703.02964 Heidelberg, March 9, 2017 p. 1 Outline Motivation Gauge coupling unification without

More information

The Standard Model and beyond

The Standard Model and beyond The Standard Model and beyond In this chapter we overview the structure of the Standard Model (SM) of particle physics, its shortcomings, and different ideas for physics beyond the Standard Model (BSM)

More information

Fuzzy extra dimensions and particle physics models

Fuzzy extra dimensions and particle physics models Fuzzy extra dimensions and particle physics models Athanasios Chatzistavrakidis Joint work with H.Steinacker and G.Zoupanos arxiv:1002.2606 [hep-th] Corfu, September 2010 Overview Motivation N = 4 SYM

More information

Clifford Algebras and Spin Groups

Clifford Algebras and Spin Groups Clifford Algebras and Spin Groups Math G4344, Spring 2012 We ll now turn from the general theory to examine a specific class class of groups: the orthogonal groups. Recall that O(n, R) is the group of

More information

arxiv: v1 [hep-th] 3 Jun 2016

arxiv: v1 [hep-th] 3 Jun 2016 Quanta of Geometry and Unification Ali H. Chamseddine 1,2 arxiv:1606.01189v1 [hep-th] 3 Jun 2016 1 Physics Department, American University of Beirut, Lebanon 2 I.H.E.S. F-91440 Bures-sur-Yvette, France

More information

arxiv:hep-th/ v3 20 Jun 2006

arxiv:hep-th/ v3 20 Jun 2006 INNER FLUCTUTIONS OF THE SPECTRL CTION LIN CONNES ND LI H. CHMSEDDINE arxiv:hep-th/65 v3 2 Jun 26 bstract. We prove in the general framework of noncommutative geometry that the inner fluctuations of the

More information

Lie n-algebras and supersymmetry

Lie n-algebras and supersymmetry Lie n-algebras and supersymmetry Jos! Miguel Figueroa"O#Farrill Maxwell Institute and School of Mathematics University of Edinburgh and Departament de Física Teòrica Universitat de València Hamburg, 15th

More information

2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC)

2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC) 2T-physics and the Standard Model of Particles and Forces Itzhak Bars (USC) hep-th/0606045 Success of 2T-physics for particles on worldlines. Field theory version of 2T-physics. Standard Model in 4+2 dimensions.

More information

A model of the basic interactions between elementary particles is defined by the following three ingredients:

A model of the basic interactions between elementary particles is defined by the following three ingredients: I. THE STANDARD MODEL A model of the basic interactions between elementary particles is defined by the following three ingredients:. The symmetries of the Lagrangian; 2. The representations of fermions

More information

The Dirac operator on quantum SU(2)

The Dirac operator on quantum SU(2) Rencontres mathématiques de Glanon 27 June - 2 July 2005 The Dirac operator on quantum SU(2) Walter van Suijlekom (SISSA) Ref: L. D abrowski, G. Landi, A. Sitarz, WvS and J. Várilly The Dirac operator

More information

The Fundamental Interactions in Noncommutative Geometry

The Fundamental Interactions in Noncommutative Geometry The Fundamental Interactions in Noncommutative Geometry Michael Agathos July 18, 2010 1 Contents 1 Introduction 3 2 The Standard Model 3 3 Noncommutative Geometry 6 3.1 Spectral Triples............................

More information

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten

The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local Gauge Transformations Dynamics of Field Ten Lecture 4 QCD as a Gauge Theory Adnan Bashir, IFM, UMSNH, Mexico August 2013 Hermosillo Sonora The Gauge Principle Contents Quantum Electrodynamics SU(N) Gauge Theory Global Gauge Transformations Local

More information

3 Quantization of the Dirac equation

3 Quantization of the Dirac equation 3 Quantization of the Dirac equation 3.1 Identical particles As is well known, quantum mechanics implies that no measurement can be performed to distinguish particles in the same quantum state. Elementary

More information

arxiv: v1 [hep-th] 1 Oct 2018

arxiv: v1 [hep-th] 1 Oct 2018 arxiv:1810.00844v1 [hep-th] 1 Oct 2018 A New SU(2) Anomaly Juven Wang, 1 Xiao-Gang Wen, 2 and Edward Witten 1 1 School of Natural Sciences, Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540

More information

Solutions to gauge hierarchy problem. SS 10, Uli Haisch

Solutions to gauge hierarchy problem. SS 10, Uli Haisch Solutions to gauge hierarchy problem SS 10, Uli Haisch 1 Quantum instability of Higgs mass So far we considered only at RGE of Higgs quartic coupling (dimensionless parameter). Higgs mass has a totally

More information

Problems for SM/Higgs (I)

Problems for SM/Higgs (I) Problems for SM/Higgs (I) 1 Draw all possible Feynman diagrams (at the lowest level in perturbation theory) for the processes e + e µ + µ, ν e ν e, γγ, ZZ, W + W. Likewise, draw all possible Feynman diagrams

More information

Le Modèle Standard et ses extensions

Le Modèle Standard et ses extensions Particules Élémentaires, Gravitation et Cosmologie Année 2007-08 08 Le Modèle Standard et ses extensions Cours I: 8 février f 2008 Théories de jauge : un rappel Programme du cours 2008 Théories de jauge:

More information

HIGHER SPIN PROBLEM IN FIELD THEORY

HIGHER SPIN PROBLEM IN FIELD THEORY HIGHER SPIN PROBLEM IN FIELD THEORY I.L. Buchbinder Tomsk I.L. Buchbinder (Tomsk) HIGHER SPIN PROBLEM IN FIELD THEORY Wroclaw, April, 2011 1 / 27 Aims Brief non-expert non-technical review of some old

More information

arxiv:hep-th/ v1 3 Jun 1996

arxiv:hep-th/ v1 3 Jun 1996 The Spectral Action Principle arxiv:hep-th/9606001v1 3 Jun 1996 Ali H. Chamseddine 1,2 and Alain Connes 2 1. Theoretische Physik, ETH-Hönggerberg, CH-8093 Zürich, Switzerland 2. I.H.E.S., F-91440 Bures-sur-Yvette,

More information

An extended standard model and its Higgs geometry from the matrix model

An extended standard model and its Higgs geometry from the matrix model An extended standard model and its Higgs geometry from the matrix model Jochen Zahn Universität Wien based on arxiv:1401.2020 joint work with Harold Steinacker Bayrischzell, May 2014 Motivation The IKKT

More information

Intrinsic Time Quantum Geometrodynamics (ITQG)

Intrinsic Time Quantum Geometrodynamics (ITQG) Intrinsic Time Quantum Geometrodynamics (ITQG) Assistant Professor Eyo Ita Eyo Eyo Ita Physics Department LQG International Seminar United States Naval Academy Annapolis, MD 27 October, 2015 Outline of

More information

Connes NCG Physics and E8

Connes NCG Physics and E8 Connes NCG Physics and E8 Frank Dodd (Tony) Smith, Jr. - vixra 1511.0098 Connes has constructed a realistic physics model in 4-dim spacetime based on NonCommutative Geometry (NCG) of M x F where M = 4-dim

More information

Generalized Global Symmetries

Generalized Global Symmetries Generalized Global Symmetries Anton Kapustin Simons Center for Geometry and Physics, Stony Brook April 9, 2015 Anton Kapustin (Simons Center for Geometry and Physics, Generalized StonyGlobal Brook) Symmetries

More information

Muon as a Composition of Massless Preons: A Confinement Mechanism beyond the Standard Model

Muon as a Composition of Massless Preons: A Confinement Mechanism beyond the Standard Model International Journal of Advanced Research in Physical Science (IJARPS) Volume 4, Issue 10, 2017, PP 7-11 ISSN No. (Online) 2349-7882 www.arcjournals.org Muon as a Composition of Massless Preons: A Confinement

More information

Rethinking Gauge Theory through Connes Noncommutative Geometry

Rethinking Gauge Theory through Connes Noncommutative Geometry Rethinking Gauge Theory through Connes Noncommutative Geometry Chen Sun Virginia Tech October 24, 2015 Chen Sun @ Duke Gauge Theory through NCG October 24, 2015 1 / 44 Work with Ufuk Aydemir, Djordje Minic,

More information

BRST and Dirac Cohomology

BRST and Dirac Cohomology BRST and Dirac Cohomology Peter Woit Columbia University Dartmouth Math Dept., October 23, 2008 Peter Woit (Columbia University) BRST and Dirac Cohomology October 2008 1 / 23 Outline 1 Introduction 2 Representation

More information

The Strong Interaction and LHC phenomenology

The Strong Interaction and LHC phenomenology The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Lecture 2: The QCD Lagrangian, Symmetries and Feynman Rules

More information

Manifestly diffeomorphism invariant classical Exact Renormalization Group

Manifestly diffeomorphism invariant classical Exact Renormalization Group Manifestly diffeomorphism invariant classical Exact Renormalization Group Anthony W. H. Preston University of Southampton Supervised by Prof. Tim R. Morris Talk prepared for Asymptotic Safety seminar,

More information

Theory of Elementary Particles homework VIII (June 04)

Theory of Elementary Particles homework VIII (June 04) Theory of Elementary Particles homework VIII June 4) At the head of your report, please write your name, student ID number and a list of problems that you worked on in a report like II-1, II-3, IV- ).

More information

The spectral action for Dirac operators with torsion

The spectral action for Dirac operators with torsion The spectral action for Dirac operators with torsion Christoph A. Stephan joint work with Florian Hanisch & Frank Pfäffle Institut für athematik Universität Potsdam Tours, ai 2011 1 Torsion Geometry, Einstein-Cartan-Theory

More information

Towards particle physics models from fuzzy extra dimensions

Towards particle physics models from fuzzy extra dimensions Towards particle physics models from fuzzy extra dimensions Athanasios Chatzistavrakidis National Technical University and NCSR Demokritos, Athens Joint work with H.Steinacker and G.Zoupanos Particles

More information

Lecture 6 The Super-Higgs Mechanism

Lecture 6 The Super-Higgs Mechanism Lecture 6 The Super-Higgs Mechanism Introduction: moduli space. Outline Explicit computation of moduli space for SUSY QCD with F < N and F N. The Higgs mechanism. The super-higgs mechanism. Reading: Terning

More information

The Strong Interaction and LHC phenomenology

The Strong Interaction and LHC phenomenology The Strong Interaction and LHC phenomenology Juan Rojo STFC Rutherford Fellow University of Oxford Theoretical Physics Graduate School course Introduction and motivation: QCD and modern high-energy physics

More information

Geometry and Physics. Amer Iqbal. March 4, 2010

Geometry and Physics. Amer Iqbal. March 4, 2010 March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries

More information

Twisted reality condition for spectral triple on two points

Twisted reality condition for spectral triple on two points for spectral triple on two points Ludwik Dabrowski SISSA (Scuola Internazionale Superiore di Studi Avanzati), Via Bonomea 265, 3436 Trieste, Italy E-mail: dabrow@sissa.it Andrzej Sitarz Institute of Physics,

More information

New Model of massive spin-2 particle

New Model of massive spin-2 particle New Model of massive spin-2 particle Based on Phys.Rev. D90 (2014) 043006, Y.O, S. Akagi, S. Nojiri Phys.Rev. D90 (2014) 123013, S. Akagi, Y.O, S. Nojiri Yuichi Ohara QG lab. Nagoya univ. Introduction

More information

Physics 557 Lecture 5

Physics 557 Lecture 5 Physics 557 Lecture 5 Group heory: Since symmetries and the use of group theory is so much a part of recent progress in particle physics we will take a small detour to introduce the basic structure (as

More information

One Loop Tests of Higher Spin AdS/CFT

One Loop Tests of Higher Spin AdS/CFT One Loop Tests of Higher Spin AdS/CFT Simone Giombi UNC-Chapel Hill, Jan. 30 2014 Based on 1308.2337 with I. Klebanov and 1401.0825 with I. Klebanov and B. Safdi Massless higher spins Consistent interactions

More information

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama Lorentz-covariant spectrum of single-particle states and their field theory Physics 30A, Spring 007, Hitoshi Murayama 1 Poincaré Symmetry In order to understand the number of degrees of freedom we need

More information

Physics 129 LECTURE 6 January 23, Particle Physics Symmetries (Perkins Chapter 3)

Physics 129 LECTURE 6 January 23, Particle Physics Symmetries (Perkins Chapter 3) Physics 129 LECTURE 6 January 23, 2014 Particle Physics Symmetries (Perkins Chapter 3) n Lagrangian Deductions n Rotations n Parity n Charge Conjugation Gauge Invariance and Charge Conservation The Higgs

More information

Diffeomorphism Invariant Gauge Theories

Diffeomorphism Invariant Gauge Theories Diffeomorphism Invariant Gauge Theories Kirill Krasnov (University of Nottingham) Oxford Geometry and Analysis Seminar 25 Nov 2013 Main message: There exists a large new class of gauge theories in 4 dimensions

More information

Gravity vs Yang-Mills theory. Kirill Krasnov (Nottingham)

Gravity vs Yang-Mills theory. Kirill Krasnov (Nottingham) Gravity vs Yang-Mills theory Kirill Krasnov (Nottingham) This is a meeting about Planck scale The problem of quantum gravity Many models for physics at Planck scale This talk: attempt at re-evaluation

More information

Regularization Physics 230A, Spring 2007, Hitoshi Murayama

Regularization Physics 230A, Spring 2007, Hitoshi Murayama Regularization Physics 3A, Spring 7, Hitoshi Murayama Introduction In quantum field theories, we encounter many apparent divergences. Of course all physical quantities are finite, and therefore divergences

More information

Fermion Mixing Angles and the Connection to Non-Trivially Broken Flavor Symmetries

Fermion Mixing Angles and the Connection to Non-Trivially Broken Flavor Symmetries Fermion Mixing ngles and the Connection to Non-Trivially Broken Flavor Symmetries C. Hagedorn hagedorn@mpi-hd.mpg.de Max-Planck-Institut für Kernphysik, Heidelberg, Germany. Blum, CH, M. Lindner numerics:.

More information

Quantum Fields in Curved Spacetime

Quantum Fields in Curved Spacetime Quantum Fields in Curved Spacetime Lecture 3 Finn Larsen Michigan Center for Theoretical Physics Yerevan, August 22, 2016. Recap AdS 3 is an instructive application of quantum fields in curved space. The

More information

A Brief Introduction to AdS/CFT Correspondence

A Brief Introduction to AdS/CFT Correspondence Department of Physics Universidad de los Andes Bogota, Colombia 2011 Outline of the Talk Outline of the Talk Introduction Outline of the Talk Introduction Motivation Outline of the Talk Introduction Motivation

More information

Lectures on Standard Model Effective Field Theory

Lectures on Standard Model Effective Field Theory Lectures on Standard Model Effective Field Theory Yi Liao Nankai Univ SYS Univ, July 24-28, 2017 Page 1 Outline 1 Lecture 4: Standard Model EFT: Dimension-six Operators SYS Univ, July 24-28, 2017 Page

More information

Inner Fluctuations in Noncommutative Geometry without the first order condition. Abstract

Inner Fluctuations in Noncommutative Geometry without the first order condition. Abstract Inner Fluctuations in Noncommutative Geometry without the first order condition Ali H. Chamseddine 1,3, Alain Connes 2,3,4 and Walter D. van Suilekom 5 1 Physics Department, American University of Beirut,

More information

A Classification of 3-Family Grand Unification in String Theory I. The SO(10) and E 6 Models. Abstract

A Classification of 3-Family Grand Unification in String Theory I. The SO(10) and E 6 Models. Abstract CLNS 96/1433, HUTP-96/A048, NUB 3145 A Classification of 3-Family Grand Unification in String Theory I. The SO(10) and E 6 Models Zurab Kakushadze 1 and S.-H. Henry Tye 2 1 Lyman Laboratory of Physics,

More information

Grand Unification. Strong, weak, electromagnetic unified at Q M X M Z Simple group SU(3) SU(2) U(1) Gravity not included

Grand Unification. Strong, weak, electromagnetic unified at Q M X M Z Simple group SU(3) SU(2) U(1) Gravity not included Pati-Salam, 73; Georgi-Glashow, 74 Grand Unification Strong, weak, electromagnetic unified at Q M X M Z Simple group G M X SU(3) SU() U(1) Gravity not included (perhaps not ambitious enough) α(q ) α 3

More information

Noncommutative Geometry in Physics

Noncommutative Geometry in Physics Noncommutative Geometry in Physics Ali H Chamseddine American University of Beirut (AUB) & Instiut des Hautes Etudes Scientifique (IHES) Frontiers of Fundamental Physics FFP14, Math Phys July 16, 2014

More information

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14.

As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14. As usual, these notes are intended for use by class participants only, and are not for circulation. Week 7: Lectures 13, 14 Majorana spinors March 15, 2012 So far, we have only considered massless, two-component

More information

QFT Dimensional Analysis

QFT Dimensional Analysis QFT Dimensional Analysis In the h = c = 1 units, all quantities are measured in units of energy to some power. For example m = p µ = E +1 while x µ = E 1 where m stands for the dimensionality of the mass

More information

The mass of the Higgs boson

The mass of the Higgs boson The mass of the Higgs boson LHC : Higgs particle observation CMS 2011/12 ATLAS 2011/12 a prediction Higgs boson found standard model Higgs boson T.Plehn, M.Rauch Spontaneous symmetry breaking confirmed

More information

Electroweak and Higgs Physics

Electroweak and Higgs Physics Electroweak and Higgs Physics Lecture 2 : Higgs Mechanism in the Standard and Supersymmetric Models Alexei Raspereza DESY Summer Student Program Hamburg August 2017 Standard Model (Summary) Building blocks

More information

Is SUSY still alive? Dmitri Kazakov JINR

Is SUSY still alive? Dmitri Kazakov JINR 2 1 0 2 The l o o h c S n a e p o r Eu y g r e n E h g i of H s c i s y PAnhjou, France 2 1 0 2 e n 6 19 Ju Is SUSY still alive? Dmitri Kazakov JINR 1 1 Why do we love SUSY? Unifying various spins SUSY

More information

Electroweak physics and the LHC an introduction to the Standard Model

Electroweak physics and the LHC an introduction to the Standard Model Electroweak physics and the LHC an introduction to the Standard Model Paolo Gambino INFN Torino LHC School Martignano 12-18 June 2006 Outline Prologue on weak interactions Express review of gauge theories

More information

Triplet Higgs Scenarios

Triplet Higgs Scenarios Triplet Higgs Scenarios Jack Gunion U.C. Davis Grenoble Higgs Workshop, March 2, 203 Higgs-like LHC Signal Fits with MVA CMS suggest we are heading towards the SM, but it could simply be a decoupling limit

More information

Yang-Mills Gravity and Accelerated Cosmic Expansion* (Based on a Model with Generalized Gauge Symmetry)

Yang-Mills Gravity and Accelerated Cosmic Expansion* (Based on a Model with Generalized Gauge Symmetry) review research Yang-Mills Gravity and Accelerated Cosmic Expansion* (Based on a Model with Generalized Gauge Symmetry) Jong-Ping Hsu Physics Department, Univ. of Massachusetts Dartmouth, North Dartmouth,

More information

E 6 Spectra at the TeV Scale

E 6 Spectra at the TeV Scale E 6 Spectra at the TeV Scale Instituts-Seminar Kerne und Teilchen, TU Dresden Alexander Knochel Uni Freiburg 24.06.2010 Based on: F. Braam, AK, J. Reuter, arxiv:1001.4074 [hep-ph], JHEP06(2010)013 Outline

More information

Lecture 8. September 21, General plan for construction of Standard Model theory. Choice of gauge symmetries for the Standard Model

Lecture 8. September 21, General plan for construction of Standard Model theory. Choice of gauge symmetries for the Standard Model Lecture 8 September 21, 2017 Today General plan for construction of Standard Model theory Properties of SU(n) transformations (review) Choice of gauge symmetries for the Standard Model Use of Lagrangian

More information

Quantum Field Theory 2 nd Edition

Quantum Field Theory 2 nd Edition Quantum Field Theory 2 nd Edition FRANZ MANDL and GRAHAM SHAW School of Physics & Astromony, The University of Manchester, Manchester, UK WILEY A John Wiley and Sons, Ltd., Publication Contents Preface

More information

arxiv:hep-ph/ v1 10 Oct 1995

arxiv:hep-ph/ v1 10 Oct 1995 UCL-IPT-95-16 Symmetry breaking induced by top quark loops from a model without scalar mass. arxiv:hep-ph/9510266v1 10 Oct 1995 T. Hambye Institut de Physique Théorique UCL B-1348 Louvain-la-Neuve, Belgium.

More information