Leptogenesis in SO(10)

We consider SO(10) Grand Unified Theories (GUTs) with vacuum expectation values (vevs) for fermion masses in the 10+126¯\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathbf{10}+\overline{\mathbf{126}} $$\end{document} representation. We show that the baryon asymmetry generated via leptogenesis is completely determined in terms of measured low energy observables and of one single high energy parameter related to the ratio of the 10 and 126¯\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \overline{\mathbf{126}} $$\end{document} SU(2) doublet vevs. We identify new decay channels for the heavy Majorana neutrinos into SU(2) singlet leptons ec which can sizeably affect the size of the resulting baryon asymmetry. We describe how to equip SO(10) fits to low energy data with the additional constraint of successful leptogenesis, and we apply this procedure to the fits carried out in ref. [1]. We show that a baryon asymmetry in perfect agreement with observations is obtained.


Introduction
Dark matter, neutrino masses, and the observed Baryon Asymmetry of the Universe (BAU) are all evidences that a theory more fundamental than the Standard Model (SM) must exist. However, so far no other observation has been found to disagree with the SM predictions. In particular, precision electroweak tests, searches for rare flavour changing processes and electric dipole moments, and the results of the first LHC run, have all failed to find new physics, and have not provided hints on how the present theory could be extended. Rather, Nature seems to suggest us that the naturalness paradigm, which has guided the construction of quite appealing extensions of the SM, might need revision: maybe the realm of new physics is way above the electroweak scale, and not around the corner. If this is the case, any information we are able to infer about the structure of the theory at very large energy scales acquires pivotal importance. In this respect, it is unequivocal that the three SM gauge couplings tend to converge while flowing towards high energies, and this strongly suggests that grand unification might be a fundamental feature of the underlying theory, an idea which is also corroborated by the possibility of explaining, within GUT frameworks, electric charge quantization, the absence of SM gauge anomalies, etc. The fact that in the SM gauge coupling unification at a single point does not occur, should not be considered as a problem, but rather as an expected feature, since the three evidences for new physics mentioned above in general require new matter fields below the GUT scale which can affect the running of the couplings and can give rise, for the low energy observer, to a certain amount of aberration rather than to a sharp focus point.
Among the possible GUT groups, SO(10) [2][3][4][5][6] is particularly interesting for several reasons: it is the smallest group for which the fifteen fermions of one SM generation can JHEP01(2015)111 fit within a single irreducible representation (the spinorial 16), it predicts the existence of one right-handed (RH) neutrino per family which in turn, via the seesaw mechanism, can account for massive light neutrinos, it can allow for non-supersymmetric gauge coupling unification and for a sufficiently long nucleon lifetime [7][8][9][10][11][12] and, being the group rank five, it can allow for an intermediate scale a few order of magnitude below the GUT scale where the gauge group reduces to rank 4. Neutrino masses, the mechanism generating the BAU, and possibly also dark matter, might all be related with this scale.
Several connections between SO(10) high energy parameters and observables can be pinned down by studying the Yukawa sector. Vacuum expectation values (vevs) giving rise to fermion masses must belong to conjugate representations of 16⊗16 = 10⊕120⊕126. In a renormalizable model, the 126 is in any case unavoidable since it is the only representation containing a SM singlet, which is needed to implement the seesaw mechanism (otherwise neutrino would have Dirac masses of the order of the charged fermion masses). However, the minimal choice of just one Yukawa coupling is not viable, because it is always possible to rotate the fermionic 16 to a basis in which the Yukawa matrix is diagonal, with the result that the up-and down-quark masses would be diagonal in the same basis and all the Cabibbo-Kobayashi-Maskawa (CKM) mixings would thus vanish. The possibility of 120 ⊕ 126 was suggested in [13] but later found, by dedicated numerical analyzes, to be not viable [1,14]. The option 10 ⊕ 126 has been instead found to allow fitting consistently all the low energy data [1,12,14]. This can be achieved under the assumption that the neutrino masses are dominated by type I seesaw contributions, and after promoting the fields in the 10 to complex fields [8]. 1 Moreover, as it was recently found in [15], in this model both the requirements of gauge coupling unification and of a proton lifetime above the experimental limits can be satisfied.
In conclusion, the results of various studies agree on the fact that the SO(10) model with scalars in the 10 ⊕ 126 (a 45 is also needed for the correct breaking of the GUT gauge symmetry, however it does not contribute to the SM fermion masses) has so far succeeded in passing a large set of phenomenological tests. In this work we will confront the model with one more test, namely we will study if the 10 ⊕ 126 SO(10) model is able to account for the observed amount of the BAU via the standard mechanism of CP violating decays of the heavy Majorana neutrinos N and leptogenesis [16][17][18]. Our main results are that the model is indeed compatible with BAU observations. As a byproduct, we perform a complete disentanglement between the Yukawa coupling matrices and the values of the vevs related to fermion masses (something that cannot be achieved with low energy fits alone) and we also obtain some information about the structure of the intermediate scale particle spectrum. Various studies related to leptogenesis in SO(10) that rely on different sets of assumptions and/or on variations of the minimal model have appeared in the literature [12,[19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34]. Here we stick to the minimal SO(10) model constrained only by the condition that the numerical values of the model parameters are such that all the low energy observables are fitted correctly.

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We start in section 2 by deriving from the SO(10) Yukawa Lagrangian the couplings of the Majorana neutrinos N to the SM fields, as well as to other SO(10) fields with intermediate scale masses, which could provide new decay channels for the N 's. In section 3 we compute the leptogenesis CP asymmetries and we write down the relevant Boltzmann equations. In section 4 we derive the connections between the relevant leptogenesis parameters and quantities that can be fitted from low energy data. In section 5 we apply our results to sets of data points resulting from the fits carried out in ref. [1], and we show that the correct amount of BAU is indeed produced. Finally in section 6 we recap and draw our conclusions.

Yukawa couplings
Fermions are assigned to three 16 a spinorial representations where a = 1, 2, 3 is a generation index. Scalars are assigned to the (fundamental) vector representation 10 µ , where µ, ν, . . . are SO (10) indices, and to the fifth rank antisymmetric tensor 126 µνλρσ (satisfying the constraint 126 µνλρσ = i µνλρσαβγδ 126 αβγδ ). Following refs. [35,36] we write the SO(10) Yukawa Lagrangian as where Γ µ are the matrices of the ten-dimensional Clifford algebra, B is the charge conjugation matrix for the SO(10) spinor representation, and C is the charge conjugation matrix for space-time spinors. The Yukawa matricesh ab andf ab are 3 × 3 complex symmetric, however by a unitary rotation of the fermion multiplets it is always possible to define a basis in which one of the two matrices is diagonal, with real and positive eigenvalues (and we will later assume the basis in whichh is diagonal). Note that such a transformations exhausts the freedom for field redefinition, so that the 3(h) + (6 + 6)(f ) = 15 remaining Yukawas correspond to physical parameters. Our goal is to project eq. (2.1) onto multiplets of the SM gauge group G SM = SU(2) L × U(1)×SU(3) keeping trace of Clebsch-Gordan coefficients between the various terms. These coefficients can be derived by analyzing the symmetry reduction chain SO(10) ⊃ G I ⊃ G SM where the intermediate G I is any (maximal) subgroup of SO(10) like G P S = SU(2)×SU(2)× SU(4) or G 5 = SU(5)×U(1). Clearly, the result does not depend on the particular G I chosen and therefore, even if we have in mind G I = G P S as the intermediate scale symmetry group, here we will follow the chain SO(10) ⊃ G 5 ⊃ G SM since the Majorana neutrinos, which are of utmost relevance for our study, are immediately singled out as the SU(5) singlets 1 = N . We need the following SO(10) → SU(5) branching rules:

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Projecting eq. (2.2) onto the SU(5) multiplets we obtain [36]: where Latin indices i, j, · · · = 1, 2, . . . 5 are SU (5) indices. Since the terms in square brackets are not a ↔ b symmetric, it is left understood thath ab (as well asf ab in the equation below) stands for the symmetrized coupling 1 2 (h ab +h ba ). In eq. (2.5) we have introduced labels for the scalar representations 5 Hu and 5 H d , in order to recall that the terms in square brackets correspond (in this order) to the neutrino Dirac coupling to the multiplet containing the SU(2) doublet H u , to the usual charged lepton and d-quark couplings to the scalar multiplet containing the down type Higgs H d , and to the u-quark Yukawa coupling. The projection of eq. (2.3) onto SU(5) representations yields [36]: The first three terms in square brackets involve the SU(5) singlet 1 = N , and correspond respectively to the Majorana coupling to the SU(5) singlet scalar 1 S that provides the N masses, to a Dirac coupling to a second u-type scalar doublet Σ u , and to an interaction term (the 10 ∆ contains only charged scalars). The terms in the second line couple quarks and leptons to the additional SU(2) scalar doublets Σ u,d . The two terms in the third line do not involve N and do not give corrections to the charged fermion masses. However, 15 contains an SU(2) triplet, and a small vev for its neutral component is often used to implement in SO(10) the type II seesaw. We have assumed from the start that neutrino masses are dominated by the type I seesaw, and thus these last two terms are not relevant for us and will be omitted in the following equations. Then, the relevant SU(5) → SU(2) L × SU(3) branching rules for projecting eqs. (2.5)-(2.6) onto G SM multiplets are: where the 45 contains additional coloured multiplets that play no role in our analysis. Written explicitly, the embedding of the SM fermions into the 5 ⊕ 10 of SU(5) is:

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which also fixes the assignments for the scalars in the 5, 5 and 10 of SU (5). As regards the 45, it is contained in the reducible three index representation antisymmetric in the upper indices 50 ij k = 5 i × 5 j a × 5 k , and it can be singled out by subtracting the i 50 ij i trace part (that transforms as an irreducible 5), that is by imposing the five constraints . The projection of eqs. (2.5)-(2.6) onto G SM multiplets is now straightforward, and yields: where we have omitted several couplings to heavy (GUT scale) coloured scalars. Let us draw the attention to the last term involving the scalar field ∆ with charge −1, since it is going to be relevant in what follows. By redefining: we can finally rewrite eq. (2.9) as:

Leptogenesis Lagrangian and CP asymmetries
The relevant couplings to compute the leptogenesis CP asymmetries and washout scatterings can be read off eq. (2.11) after spelling out a few points characterizing the scenario.
• The scalar field ∆ is the charge −1 component of the same multiplet, and is expected to acquire an intermediate scale mass as well. We thus need to allow for the possibility M N > M ∆ , i.e. that the decay channel N → e c ∆ is open. The possibility of N decays into SU(2) L singlet leptons and scalars was already studied in [37] (although not in relation with SO(10)) and it was found to be potentially interesting for leptogenesis. One of the reasons is that the specific decays into e c 1 , defined as the SU(2) singlet lepton most weakly coupled to the N 's, would generate an asymmetry that remains completely decoupled from the thermal bath, and in particular unaffected, even indirectly, by potentially large 1 H ↔ N washouts, since the Yukawa coupling relating e c 1 and 1 remains out of equilibrium down to temperatures T M N .

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• The scalar fields Σ u,d belong to (2, 2, 15) of G P S and have a mass unrelated to the vev σ. Naturalness considerations then suggest that M Σ M N in which case the decays N → Σ u are kinematically forbidden. Note however, that the neutral components of these bi-doublets will acquire induced vevs proportional to the EW vevs residing in the 10, via the coupling (126 126) (126 10) [8]. These induced vevs are of fundamental importance to achieve the correct fermion mass relations.
As we have already mentioned, at the unbroken SO(10) level one can always choose a basis in which one of the two matrices of Yukawa coupling is diagonal with real nonnegative entries, and we choose h ab =ĥ a δ ab , while f remains a generic complex symmetric matrix. After intermediate SO(10) → G P S breaking, the appropriate basis for leptogenesis is the basis of the N 's mass eigenstates, defined via a rotation of the Majorana fields with a unitary matrix W that brings the matrix f in the first term in eq. (2.11) into diagonal form:f = W f W T . In this basis, the Lagrangian terms relevant for leptogenesis can be written as: Since at the leptogenesis temperatures T ∼ M N M Σ scatterings between leptons and Σ d do not occur, the flavour basis { α , e c α } remains fixed by the leptons Yukawa interactions with the light d-type Higgs:ĥ α e c α α H d . Here and below we denote with Latin subscripts j, k, . . . the heavy neutrinos mass eigenstates ordered from light (j = 1) to heavy (j = 3), and with Greek subscripts α, β, . . . the lepton flavours, ordered according to the strength of their Yukawa couplingsĥ 1 <ĥ 2 <ĥ 3 . It is worth noticing at this point, that due to the contribution of the f couplings to the lepton masses after EW symmetry breaking, the SM mass eigenstates e , µ , τ will not in general coincide with the leptogenesis flavour eigenstates 1 , e c 1 ; 2 , e c 2 ; 3 , e c 3 .

CP violating asymmetries
The CP violating asymmetries for N j decays into leptons of flavour α are defined in terms of decay widths in the usual way:

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where superscripts (subscripts) denote initial (final) decay states, and where the factor of two takes into account gauge multiplicities of the SU(2) doublets, while 6 2 = 36 originates from the prefactor in eq. (3.2) for the SU(2) singlets term. Note that the asymmetry in eq. (3.5) is defined with an overall minus sign, that compensates the fact that in the production of e c lepton number is decreased by one unit. In defining the total width Γ N j tot eq. (3.6) we have neglected W R mediated three body decays N → e cūc d c . Given that all the N 's are strongly coupled to at least one lepton flavour (one Yukawa coupling is in fact related to the top Yukawa coupling) this is justified as long as M W R > ∼ M N . Computation of the CP asymmetries can be carried out in the usual way [42]. In particular, in spite of the presence of the new decay channel N → e c ∆, there are no new loop contributions. This is because f -related couplings appear in the loops in the combination For the same reason, the total CP asymmetries in N j → e c α ∆ decays summed over flavours also vanish α ∆ jα = 0. Thus, the contribution of this channel is of the "purely flavoured leptogenesis" (PFL) type [43]. For the CP asymmetries we obtain: The function g SV = g S + g V is the sum of the self energy and vertex loop functions: where the limiting expressions hold for x → ∞. Let us note that for the ∆ jα asymmetries there is no vertex contribution g V . The second term in eq. (3.8) (which is sometimes denoted as the 'lepton number conserving term') involves the self energy function and it does not contribute to the total asymmetry H j = α H jα . In fact by summing over flavour one obtains |(Wĥ 2 W † ) jk | 2 which is real. We can conclude that the g S contribution is also of the PFL type [41,42]. It is interesting to note that while in H 1α this term is in any JHEP01(2015)111 case subdominant, given that (in the hierarchical limit) g S (x k1 )/g S (x k1 ) ∼ M 1 /M k 1, it represents instead the dominant contribution to the N 1 CP asymmetry ∆ 1α . This is because at the leading order in M 1 /M k =f 1 /f k , which comes from the g S expansion, ∆ 1α vanishes, so that g S contributes only at order (f 1 /f k ) 3 . Thus the first order contribution from g S ∼ (f 1 /f k ) 2 is the dominant one. The fact that ∆ 1α vanishes at first order in the expansion can be seen by extending the sum over k in the first term of eq. (3.9) to include also k = 1 (the added term is real and does not contribute). At leading order we obtain Thus the first term in eq. (3.9) is, at leading order, real ∝ |W jα | 2 and gives no contribution to ∆ 1α (for ∆ 2,3 there is no analogous result because the expansions eqs. (3.10)-(3.12) do not hold). This is yet another example of the various cancellations that follow as a consequence of the SO(10) Yukawa structure.

Boltzmann Equations
We are now ready to write the network of Boltzmann Equations (BE) for SO(10) leptogenesis. In full generality, we need three BE for the evolution of the N 1,2,3 number densities and three for the usual anomaly free lepton charges ∆ α = ∆B/3 − ∆L α [38,39]. There is, however, another quantity that in the limit of vanishing N couplings is conserved: it corresponds to the U(1) e 1 generator of phase transformations for the SU(2) singlet lepton field e 1 defined as the one with the smallest coupling to the Higgs. Since e 1 is an SU (2)  → 0 [44]. This results in the U(1) e 1 invariance and in a fourth conserved charge ∆ 4 = ∆e 1 . Let us thus define the following charge densities (normalized to the entropy density) that are violated just by N 's interactions while are conserved by all the reactions which are in thermal equilibrium (including non-perturbative sphaleron processes): 14) To write down the network of flavoured BE as a closed system, one needs to express the density asymmetries of the five leptons Y ∆l ≡ {Y ∆ 1 , Y ∆ 2 , Y ∆ 3 , Y ∆e 2 , Y ∆e 3 } and of the up-type Higgs Y ∆Hu , which weight the washout terms, as linear combinations of the four

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(Y ∆ ) q , that is: Note in passing that while H u develops an asymmetry, there is no asymmetry for the scalar ∆. This is because the ∆ are produced in decays for which the total asymmetry vanishes, and in addition there are no other scatterings in the plasma involving the ∆ and SM or other particles with intermediate scale masses. Therefore the ∆ are not subject to any chemical potential equilibrium condition that could result in Y ∆ ∆ = 0. The 5×4 A matrix and the C-vector in eq. (3.18) can be obtained by solving the system of linear constraints corresponding to in-equilibrium spectator reactions (Yukawa related scatterings, EW and QCD sphalerons [45]) and exactly conserved quantities (hypercharge). This yields: The final B − L asymmetry resulting from leptogenesis is given by the sum are obtained by integrating the BE. Finally, with two Higgs doublets, the relation between the baryon asymmetry and Y ∆ B−L is: The BE for the evolution of the N j densities and of the (Y ∆ ) q charge asymmetries, considering only decays and inverse decays read: = 2Y eq f = 15/(4π 2 g * ) are the boson and fermion relativistic equilibrium number densities normalized to the entropy density, Y eq N j = n eq N j /s = 45z 2 j K 2 (z j )/(2π 4 g * ) is the equilibrium density for the non-relativistic N 's with z j = √ x j1 z, K n is the modified Bessel function of type n, is the thermal average of the total decay rate Γ N j tot eq. (3.6), and the γ N j ... are similarly thermal averages of the N j partial decay rates.

Relating leptogenesis parameters to observables
To estimate the baryon asymmetry yield of the minimal SO(10) model we need the numerical values of the partial decay widths and CP asymmetries, and to compute these quantities we need to know the values of the Yukawa coupling matrices and of the vev σ that fixes the scale of the N 's masses. As we will now argue, the values of these parameters can be fixed almost univocally in terms of measured low energy observables, with only one single high energy parameter left free. Let us define for the up-and down-type Higgs doublets (denoted with subscripts q = u, d) the following vev-related quantities: and G F the Fermi constant. After EW symmetry breaking, the fermion mass parameters can be read off from eq. (2.11) by projecting the scalar bi-doublets fields H u,d and Σ u,d on their vevs. This yields:

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with M ,d,u the charged leptons, d-and u-type quarks mass matrices, and M D the Dirac mass matrix for the neutrinos. On the right-hand side (r.h.s. ) of the first equalities we have written the mass matrices keeping distinguished the vevs and the Yukawa couplings; this is needed to write down leptogenesis related quantities. The r.h.s. of the second equalities is instead written following a commonly adopted parameterization [1,12,14,[46][47][48], which is best suited for SO(10) fits to low energy data. In these notations the relation with the non-diagonal (M N ) and diagonal (M N ) Majorana neutrino mass matrix can be written as: Thus, once F is given, the unitary matrix W can be determined from the requirement that it brings F into its diagonal form with real non-negative entries. Here we follow in particular the conventions used in ref. [1] withĤ diagonal with 3 real non-negative entries, F complex symmetric with 6 + 6 (real + imaginary) parameters, r and r R real quantities and s ≡ |s|e iδs complex, for a total of 19 parameters (12 real and 7 imaginary). The low energy data set consists of 9 charged fermion masses, 2 neutrinos mass squared differences, 3 + 3 quark and lepton mixing angles and 1 CKM phase, for a total of 18 parameters (17 real and 1 imaginary). Although the number of parameters exceeds by one the number of constraints from the data, SO(10) numerical fits are able to determine all 19 parameters (and thus to yield also predictions for yet unmeasured quantities like the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) Dirac phase and the 0ν2β effective neutrino mass [1,14]). This is due in part to the nonlinearity of the relations that connect {Ĥ, F, r, r R , s} to the data, and also to the fact that the number of real observables (moduli) is sizeably larger than that of real free parameters. All in all, fits to low energy data are able to fix the numerical values of the whole set {Ĥ, F, r, r R , s}. We want to relate these numerical quantities to our Yukawa parametersĥ,f , W (two diagonal real matrices and one unitary, for a total of 3 + 3 + (3 + 6) = 9 real + 6 imaginary parameters) and to the 4+1 vevs-related quantities σ, t β , s d , s u e iδu , defined in the following way: the vevs H u,d ∝ c u,d have one common phase [8] that can be reabsorbed redefining the remaining ones, and the phase of s d can be absorbed into W * by redefining δ u and σ. As regards σ, it is in general complex, but its overall phase does not affect low energy data or leptogenesis, and therefore for simplicity we take σ to be real. With respect to the parameterization in the r.h.s. of eqs. (4.8)-(4.12) we have one additional real parameter, that can be identified via the relation F ↔ f · s d . While low energy data are only sensitive to the product of the coupling matrices times the vev Σ d , leptogenesis is directly sensitive to the values of f alone, and then it can allow to disentangle the Yukawa couplings from the vevs. More precisely, it is the value of t d (defined in eq. (4.5)) that can tell us which part of the corrections to quark/lepton universality is due to the f Yukawas (whose size is relevant for leptogenesis) and which part is due to the vevs of the 126 bi-doublets. We will then take t d as the new independent variable. All the other vev related quantities can then be written as: 14) JHEP01(2015)111 Finally, for the two matricesĥ and f we obtain: where the approximations hold for r 2 1, |s| 2 1 (which result from numerical fits) and t d < ∼ 1 (which is favoured theoretically since t d is the ratio between an induced vev Σ d and the EW vev H d ). From eq. (4.14) we can see that in this approximation t β ≈ r, from eq. (4.16) we learn that the matrixĥ is not very sensitive with respect to changes in t d while, in contrast, from eq. (4. 17) we see that f is inversely proportional to t d . This means that at fixed values of F , small vevs Σ d imply large f -Yukawa couplings and this would render, among other things, more important the 'exotic' decay channel N → e c ∆.

Results
From the equations above it should be clear that once the values of {Ĥ, F, r, r R , s} are determined by fits to the low energy observables, the CP asymmetries eqs. (3.8)-(3.9) and the partial decay rates entering the BE eqs. (3.22)-(3.26) remain determined solely in terms of t d . Note, however, that the heavy Majorana masses M N do not depend on this parameter (given that they do not depend on the doublets vevs) and thus the RH neutrino spectrum is univocally fixed solely by the low energy data. As we have already mentioned, the RH neutrino masses obtained from the numerical fits generally fall in the range 10 9 − 10 12 GeV, which is a favourable one for leptogenesis, but it should be remarked that this type of results always implies a certain degree of tuning. The mass of the lightest Majorana neutrino N 1 would in fact more naturally lie in a mass range well below 10 9 GeV. To show this, let us start by writing the seesaw formula in a generic basis: where we have defined W = V † U . Let us now write:

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Taking the trace of this equation yields: where in the left-hand side the sum of the squares of the inverse RH neutrino masses has been expressed as i with M 1 the mass of the lightest RH neutrino and ranging between 1 (strong hierarchy: M 1 M 2,3 ) and 3 (degeneracy: . The RH side of eq. (5.4) is a sum of positive definite terms, and is thus larger than each single term. Let us take as dominant the one involving (M d D 1 ) 4 at the denominator. We obtain: 2 Approximate quark-lepton Yukawa universality suggests M d D 1 ∼ m up . On the other hand W is the product of the PMNS matrix U and of the matrix V that, in the basis in which the down-type Yukawa couplings are diagonal, should be approximately given by the CKM matrix. This implies that W should depart sizeably from a pure diagonal form, and thus the denominator in eq. (5.5) is bounded from below. For example, for GeV is obtained. Departures from quark-lepton Yukawa universality can at most yield a factor of a few enhancement of M d D 1 with respect to m up , and therefore eq. (5.5) can give an estimate of the amount of tuning required to enforce cancellations in i W 2 1i m d i such that M 1 can be lifted into the 10 9 -10 12 GeV range. If from one hand it is somewhat unpleasant that the numerical values that we will use result from a certain amount of tuning in fitting SO (10) parameters, on the other hand we find intriguing that, without any knowledge of what is required for leptogenesis to be successful, low energy data alone force all the M j 's in the correct ballpark.
By means of numerical integration of the BE (3.22)- (3.26) it is now possible to verify if a set of fitted data points {Ĥ, F, r, r R , s} can yield an amount of baryon asymmetry in agreement with observations. We use the most recent combined Planck and WMAP CMB measurements [50,51], which yield at 95% c.l.
We take the {Ĥ, F, r, r R , s} data points from the fits of Dueck and Rodejohann (DR) [1] to non-supersymmetric SO(10) with scalars in 10 + 126, that are labeled as MN (minimal non-supersymmetric). Starting from the low energy data set (SM fermion masses and mixings) at the scale µ = M Z , DR perform two different types of fits to the MN model. In the first approach, which they denote as MN-RGE, the observable are evolved from the high energy scale down to M Z , integrating out the heavy neutrinos N j one by one at the appropriate scale. The outcome of the running is then compared with the experimental data. This is the most JHEP01(2015)111 sophisticated approach, and in particular is expected to yield a more reliable fit to the heavy neutrino masses. This, besides having sizeable effects on the neutrino parameters [52], is a quite crucial ingredient in leptogenesis. The N spectrum obtained with this procedure is: As regards the numerical values of the set {Ĥ, F, r, r R , s}, they can be found in appendix A of [1] labeled as MN-RGE and are not recopied here. The main approximation in the DR analysis is that of neglecting effects of the intermediate scale states on gauge coupling unification and on the running of the Yukawa matrices, and it is quite hard to estimate the related uncertainty on the fitted parameters. 3 Since, as said above, the details of the N 's mass spectrum is one of the most influential ingredient for the outcome of leptogenesis, we will present our results allowing for a 3% fluctuation around the central values in eq. (5.7). While we make no claim that this fluctuation is accounting for the aforementioned theoretical uncertainty, it can still be illustrative of the sensitivity of the results on changes in the details of the N 's spectrum.
The second approach followed by DR, that they denote as MN-noRGE, is based on a direct fit to the low energy neutrino parameters, and to the GUT scale values of the charged fermion observables, evolved to the high scale ignoring the effects of non-degenerate RH neutrinos. As it is clearly explained in the DR paper, this second approach cannot be considered fully consistent, however it provides a second reference point for our study which allows for an important comparison for the outcome of leptogenesis. The N 's mass spectrum for the MN-noRGE case is: with the experimental value which is derived from eq. (5.6) via eq. (3.21), and that is represented by the horizontal grey band. The thick purple line depicts the results for the combined contributions of the N j → α H and N j → e c α ∆ channels and the purple band corresponds to a 3% variation in the values of the N j masses in eq. (5.7). We see that Y ∆ B−L keeps growing with increasing values of t d , that is with decreasing values of the f -couplings. The reason is that there is an overall contribution of the wrong sign from the N j → e c α ∆ channels which is sizeable for small t d , while with decreasing values of the f couplings it becomes less important. All in all, we see that in the theoretically favoured region t d < 1 ( i.e. Σ † d Σ d < H † d H d ) the purple band fails to intersect the experimentally allowed grey region. Only in the shaded region, corresponding to values t d > 1, which are however theoretically questionable, the upper border of the purple band touches the grey band. The results for the contributions of the N j → α H JHEP01(2015)111 Figure 1. The B-L asymmetry produced with the MN-RGE data set of ref. [1] plotted as a function of t d . The horizontal grey band represents the experimental limit, the orange curve depicts the asymmetry generated via N j → H α decays alone, while the purple band includes also the N j → ∆e c α decays. The width of the orange and purple bands correspond to a 3% variations in the N j masses. channel alone are represented by the thick orange line. This corresponds to the situation in which the ∆ scalar is heavier than N 1,2 (N 3 contributions to leptogenesis remain quite marginal), that is M ∆ > ∼ 2.0 × 10 11 GeV, so that N 1,2 decays into e c α ∆ are kinematically forbidden. In this case the predicted central value touches the experimental band well within the region t d < 1, while the orange band nicely overlaps with the experimental band in the full interval 0.3 < ∼ t d < ∼ 1. It is also worth noticing that the maximum value of the Y ∆ B−L asymmetry obtained in this model coincides rather precisely with the value obtained from observations. This is a bit intriguing, given that a priori this value could have been anything.
In summary, we find that the DR RGE fit to the minimal non-supersymmetric SO(10) model is fully consistent with the requirement that the observed value of the BAU is produced via leptogenesis, if the two conditions (i) M ∆ > ∼ M N 2 2.0 × 10 11 GeV and (ii) We present for comparison in figure 2 the results for the MN-noRGE data set. In this case the spectrum is sufficiently hierarchical (see eq. (5.8)) that leptogenesis is largely dominated by N 1 dynamics. The contribution of the N j → α H channels alone, represented by the thick orange line, remains well below the Y ∆ B−L experimental band even in the t d > 1 region. In this case the effect of the 3% variations in the N 's mass values is much milder than in the previous case, and this can be traced to the larger mass hierarchy and to N 1 dominance. Adding the contributions of the N j → e c α ∆ channels (the purple band and thick central line) has the striking effect of yielding a sizeably larger asymmetry, which is JHEP01(2015)111 however of the wrong sign (this is depicted in the figure by means of a dashed, rather than continuous, line). The fact that the N j → e c α ∆ contributions become particularly large with increasing t d is due to the fact that in this regime all the N 1 → e c α ∆ decay channels enter the weak washout regime, and washout effects keep decreasing as t d increases. N 1 → 1,2 H decays also remain in the weak washout regime as long as t d < ∼ 3, while 3 is sufficiently strongly coupled to N 1 to ensure a thermal abundance for the RH neutrino independently of initial conditions. We also see how the purple bands widens at small values of t d (i.e. large values of the f -couplings). This is due to the vanishing of the first order O(M 1 /M k ) contribution to ∆ 1α that we have discussed at the end of section 3.1, which results in an enhanced sensitivity to the M 1 /M k ratio. Let us also remark at this point that the sign of Y ∆ B−L can be reverted (and the correct sign and size can thus be obtained) by simply reverting the signs of all the imaginary parts of the F and s parameters. While this will leave untouched the predictions for the fermion masses and mixings, it will result in the wrong sign for the CKM matrix δ CKM . Thus, it is just the interplay between Y ∆ B−L and δ CKM which allows to rule out the MN-noRGE data set with the contributions of the N j → e c α ∆ decays included. In summary, while the results of the DR analysis [1] indicate that the MN-noRGE data set gives a better fit to the low energy data than the (more reliable) MN-RGE data set, we can conclude that MN-noRGE fails to produce a sufficiently large baryon asymmetry, and thus it does not pass the leptogenesis test.

Concluding remarks
In this work we have considered leptogenesis in a non-supersymmetric SO(10) GUT with fermion masses from the 10 ⊕ 126 Higgs representations, which can (i) fit well all the JHEP01(2015)111 low energy data, (ii) successfully account for unification of the gauge couplings, and (iii) allow for a sufficiently long lifetime of the proton. We have shown that, once the model parameters are fixed in terms of measured low energy observables, the requirement of successful leptogenesis can fix the only one remaining high energy parameter. We have highlighted that a new decay channel for the heavy Majorana neutrinos into the SU(2) singlet leptons e c is possible, and we have found that these decays can sizeably affect the size of the resulting baryon asymmetry. We have shown that the values of the model parameters obtained from the fits to low energy observables given in ref. [1] yield a baryon asymmetry in agreement with observations.