Electroweak monopoles and the electroweak phase transition

The European Physical Journal C, Jul 2017

We consider an isolated electroweak monopole solution within the Standard Model with a nonlinear Born–Infeld extension of the hypercharge gauge field. Monopole (and dyon) solutions in such an extension are regular and their masses are predicted to be proportional to the Born–Infeld mass parameter. We argue that cosmological production of electroweak monopoles may delay the electroweak phase transition and make it more strongly first order for monopole masses \(M\gtrsim 9.3 \,{\cdot }\, 10^3\) TeV, while the nucleosynthesis constraints on the abundance of relic monopoles impose the bound \(M\lesssim 2.3\cdot 10^4\) TeV. The monopoles with a mass in this shallow range may be responsible for the dynamical generation of the matter–antimatter asymmetry during the electroweak phase transition.

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Electroweak monopoles and the electroweak phase transition

Eur. Phys. J. C Electroweak monopoles and the electroweak phase transition Suntharan Arunasalam 0 Archil Kobakhidze 0 0 ARC Centre of Excellence for Particle Physics at the Terascale, School of Physics, The University of Sydney , Sydney, NSW 2006 , Australia We consider an isolated electroweak monopole solution within the Standard Model with a nonlinear BornInfeld extension of the hypercharge gauge field. Monopole (and dyon) solutions in such an extension are regular and their masses are predicted to be proportional to the Born-Infeld mass parameter. We argue that cosmological production of electroweak monopoles may delay the electroweak phase transition and make it more strongly first order for monopole masses M 9.3 · 103 TeV, while the nucleosynthesis constraints on the abundance of relic monopoles impose the bound M 2.3 · 104 TeV. The monopoles with a mass in this shallow range may be responsible for the dynamical generation of the matter-antimatter asymmetry during the electroweak phase transition. 1 Introduction For a long time, there was a prevailing view that topologically stable monopole solutions do not exist in the Standard Model because the vacuum manifold SU ( 2 ) × U ( 1 )Y /U ( 1 )E M allows no non-trivial second homotopy group. This has been questioned in [1], where topological stable monopole (and dyon) solutions, representing a non-trivial hybrid between the U ( 1 )E M Dirac monopole [2] and the non-Abelian ’t Hooft–Polyakov monopole [3–5], have been found in [1]. While the SU ( 2 ) non-Abelian configuration is regular, the U ( 1 )E M configuration exhibits a point singularity at the origin. As a result, the monopole mass is divergent. There is no obvious problem with the energy of a classical configuration being divergent as it may be regularized in a more complete quantum theory. In fact, also some regularized monopole solutions have been proposed [6–9] which indicate that electroweak monopoles as light as ∼5–10 TeV may actually exist. In this paper, we consider the Standard Model where the standard kinetic term for the UY ( 1 ) hypercharge gauge boson is a part of a nonlinear Born–Infeld Lagrangian. In this theory we account for an extra mass parameter, √β, which controls the nonlinearity of the hypercharge field. Similar to the regularization of the divergent energy of a point-like charge in the original Born–Infeld electrodynamics [10], we find that the electroweak monopole gets also regularized and it mass predicted to be ∝ √β. Interestingly enough, the Born–Infeld extension considered here emerges as an effective low energy theory of open strings attached to the 3branes [11]. In this picture, the parameter √β defines the distance between 3-branes in the extra-dimensional bulk spacetime. The electroweak monopoles must be copiously produced during the electroweak phase transition via the Kibble mechanism [12,13].1 Furthermore, as we will argue in this paper, cosmological production of electroweak monopoles may delay the electroweak phase transition and make it stronger first order. The physics behind this can be heuristically explained as follows. Magnetic monopoles (and antimonopoles) with symmetric vacuum configuration within the monopole core are trapped in the region surrounded by the domains with symmetry-breaking vacua with different orientation of the Higgs field in the SU ( 2 ) × U ( 1 )Y /U ( 1 )E M vacuum manifold. This costs in energy, leading to a higher free energy in the broken phase relative to the case without monopole production. In particular, we find that φc/ Tc 1 can be achieved without violating nucleosynthesis constraints on relic monopole abundance. This may have important implications for electroweak baryogenesis. Namely, sphaleron mediated B + L-violating processes become ineffective below the critical temperature, Tc, preventing the washout of previously generated baryon asymmetry. 1 Strictly speaking the Kibble mechanism is applicable to global monopole production. The refined mechanism in the case of gauge theories is discussed in [14]. The rest of the paper is organized as follows. In Sect. 2, we discuss the electroweak monopole solution within the Born–Infeld hypercharge extension of the Standard Model. Section 3 is devoted to a discussion of monopole production and its impact on the electroweak phase transition. In Sect. 4, we conclude. 2 Electroweak monopoles in the Born–Infeld hypercharge model Let us consider Standard Model extended by the nonlinear Born–Infeld type hypercharge gauge field. The relevant bosonic Lagrangian reads 1 − 4 Fμν F μν 1 1 1 + 2β2 Bμν Bμν − 16β4 (Bμν B˜ μν )2 where Dμ = ∂μ − i g2 τ a Aaμ − i g2 Bμ is the SU ( 2 )L × U ( 1 )Y gauge covariant derivative with Aaμ and Bμ being SU ( 2 )L and U ( 1 )Y gauge vector fields, respectively and H is the electroweak doublet Higgs field. Fμaν (a = 1, 2, 3) denote the SU ( 2 )L gauge field strength tensors, and B˜ μν = 21 μναβ Bαβ is the Hodge dual to the U ( 1 )Y field strength tensor Bμν . Parameter β is a new Born–Infeld parameter of dimension mass2. It controls the nonlinearity of the hypercharge field and, as we will see shortly, provides ultraviolet regularization of the electroweak monopole mass. In the limit β → ∞, we recover the Standard Model theory. The above Lagrangian leads to the following set of field equations of motion: Dμ(Dμ H ) = λ ∂μ − i g τ a Aa 2 μ μ2 H † H − λ F μiν = i g2 H, H †τ i (Dν H )−(Dν H )†τ i H , ∂μ ⎣ ⎡ g = i 2 1 − 4β2 Bαβ B˜ αβ B˜ μν ⎤ 1 + 2β12 Bαβ Bαβ − 161β4 (Bαβ B˜ αβ )2 ⎦ H †(Dν H ) − (Dν H )† H . ( 2 ) ( 3 ) ( 4 ) Here, (r, θ , ϕ) are the usual spherical polar co-ordinates and rˆ is the unit vector in the radial direction. Now, as done in [1], consider the following ansatz: 1 H = √ ρξ, ρ = ρ(r ), ξ = i 2 sin(θ /2)e−iϕ − cos(θ /2) 1 1 Aμ = g A(r )∂μtrˆ + g ( f (r ) − 1)rˆ × ∂μrˆ, 1 1 Bμ = − g B(r )∂μt − g (1 − cos θ )∂μϕ. In particular, the functions, A(r ) and B(r ) represent dyon solutions of this model. For A(r ) = B(r ) = 0, one obtains pure magnetic monopole, which is also the lightest object and thus we concentrate on this solution. For A(r ) = B(r ) = 0, Eq. ( 4 ) is trivially satisfied and Eqs. ( 2 ) and ( 3 ) yield 2 f 2 ρ¨ + r ρ˙ − 2r 2 ρ = λ ρ2 μ2 2 − λ ρ f¨ − f 2 − 1 r 2 f = g42 ρ2 f. The following boundary conditions can be chosen for these equations: ( 1 ) f (0) = 1, ρ(0) = 0, f (∞) = 0, ρ(∞) = ρ0 = 2μ2 λ ( 5 ) ( 6 ) ( 7 ) . ( 8 ) ( 9 ) ( 10 ) ( 11 ) Under these boundary conditions, it can be seen that near the origin f ≈ 1 + α1r 2, ρ ≈ β1r δ with δ = (−1 + √3)/2 and asymptotically, −gρ0 2 f ≈ f1 exp r , ρ ≈ ρ0 + ρ1 exp(−√2μr ) r . The energy of this monopole is given by E = E0 + E1, 0 ∞ E0 = E1 = 4π ⎡ drβ2 ⎣ 0 ∞ dr h2Y ⎤ (4πr 2)2 + β2 − 4πr 2⎦ , 1 ( f 2 − 1)2 g2 2r 2 1 + 2 (r ρ˙)2 1 2 + g2 f˙ + λr 2 8 ρ2 − ρ02 2 + 41 f 2ρ2 , where hY = 4gπ is the hypermagnetic charge of the monopole, g being the hypercharge gauge coupling. Here, E0 is the term corresponding to Born–Infeld hypercharge term and E1 is due to the remainder of the Lagrangian. In the usual standard model, E1 is finite due to the above boundary conditions and asymptotics and E0 is infinite. However, due to the Born–Infeld modification, E0 is also made finite. E1 has been calculated by [7] to be roughly 4 TeV. As discussed below, the mass of the monopoles that provide a significant impact on the electroweak phase transition must be at least of order 104 TeV. Hence, E0 must dominate this mass and hence, it is assumed that E ≈ E0. This term can be calculated exactly using elliptic integrals as [15]: π 3/2 E ≈ 3 ( 3 )2 4 βh3Y where we have used g = 0.357. Thus the monopole mass is proportional to the Born–Infeld mass parameter, √β. One can verify that the magnetic charge of this monopole solution 4π . is h = e In the perturbative expansion of the Born–Infeld Lagrangian, which is valid for low hypercharge field strength, |Bμν | < β, the lowest order Born–Infeld correction appears as operators of mass dimension 8. They involve only hypercharge field and are suppressed by a factor ∝ β−2. The best bound on the Born–Infeld mass parameter can be inferred from the PVLAS measurements of nonlinearity in light propagation [16] (see also [17]): β 5.0 · 10−4 GeV. This is clearly a very weak constraint compared to constraints from direct searches of massive monopoles [18], which in our case implies √β 15.1 GeV. In contrast, the monopole mass is regularized in [7,8] by non-renormalizable operators with mass dimension n > 8 + 2√3 operator which also involve the Higgs field. These operators are significantly constrained by LHC data on the Higgs-to-2γ decay [9]. 3 Monopole production and electroweak phase transition Consider the one loop high temperature effective potential: V (φ, T ) = D(T 2 − T02)φ2 − E T φ3 − 41 λT φ4 where the parameters are defined by 1 D = 8v2 (2m2W + m2Z + 2mt2), 1 E = 4π v3 (2m3W + m3Z ), ( 13 ) (14) 1 T0 = 2D (μ2 − 4Bv2) with ln a f = 1.14, ln ab = 3.91, m H = 125 GeV, mW = 80.2 GeV, m Z = 91.2 GeV, mt = 173 GeV and v = 246 GeV. Let φc(T ) be the value of the Higgs field at the second minimum. If monopoles are not produced, the Gibbs free energy of the unbroken and broken phases are simply the value of the potential at φ = 0 and φ = φc(T ) and the critical temperature, Tc is defined as the temperature at which these are equal. In order to avoid the sphaleron washout constraint, one requires that (e.g. see [19] and the references therein). (16) φc(Tc) Tc 1. With the standard model parameters, this ratio is roughly 0.17, implying that sphaleron mediated processes will washout any pre-existing matter–antimatter asymmetry in the universe. This conclusion is altered significantly once the electroweak phase transition is supplemented by the production of the electroweak monopoles. The details of the production of monopoles have been discussed in [13], which we closely follow. Although the electroweak monopoles are typically heavier that the critical temperature, M >> Tc, they are produced out of equilibrium during the phase transition when the Higgs field becomes frozen in the broken phase [13]. During the electroweak phase transition, there is a finite distance over which, the field is correlated with itself. At distances larger than the correlation length, the Higgs field may point in different directions in the manifold of degenerate vacua. Following Kibble [12] and Preskill [13], one can argue that a certain density of monopoles is to be expected on this account alone. Monopoles (like vortices in a superconductor) can be thought of as a measure of the disorder remaining in the system, where symmetric (normal) regions trapped by flux quantization in the broken (superconducting) ground state. Hence, production of monopoles will drive the surrounding plasma out of equilibrium. The equilibrium will be eventually restored once the monopole/antimonopole density will drop due to the monopole–antimonopole annihilation. The production of monopoles during the electroweak phase transition offers a qualitatively new picture of baryogenesis at the electroweak scale. In addition to sphalerons, there is additional source of anomalous B + L violation through matter-monopole scattering. These scatterings are known to be unsuppressed [20], and thus are potentially rapid to contribute to the generation of baryon asymmetry at around Tc. Once the equilibrium is achieved, however, below Tc, sphaleron and monopole mediated processes must become irrelevant in the broken phase. The sphalerons are ineffective if condition (16) is satisfied, while matter-monopole scatterings must decouple once the monopole density becomes low enough due to monopole– antimonopole annihilation. The latter process is also important to not upset the standard Big Bang nucleosynthesis. In what follows we will concern ourselves with washout issues, postponing the full discussion of baryogenesis to future work. 3.1 Circumventing the sphaleron induced washout of baryon asymmetry Since monopoles are assumed to be heavier than the critical temperature Tc, they can be treated as nonrelativistic point-like particles. Monopole–antimonopole interactions, as well as interactions of monopoles with charged particles of plasma, are due to the long-range electromagnetic forces. The monopole–antimonopole annihilation cross section can be approximated by σM M¯ = dc2, where dc = h2/4π T is the Coulomb capture distance and h = 4π/e is the monopole charge. Similarly, a relativistic charged particle with a charge q will scatter off the monopole (antimonopole) with the cross section σq M = (qh/4π )2T −2. The initial density of isolated monopoles (and antimonopoles) can be estimated as n0 = dc−3 [13]. Below the capture distance monopole– antimonopole pair would form a unstable bound state and decay subsequently through annihilation. The production of monopoles cost in energy, so the free energy in the broken phase becomes Gb = V (φc(T )) + n0 M. (17) Equating, now, the free energies in the symmetric and broken phases, it becomes clear that the electroweak phase transition happens at lower critical temperatures Tc, and, therefore, sphalerons may start to satisfy the non-washout condition (16). As seen from Fig. 1, this indeed takes place when monopoles are sufficiently heavy, M > 9.3 · 103 TeV. Unfortunately, such heavy monopoles are not able to be produced at the LHC or at other future planned colliders. 3.2 Monopole–antimonopole annihilation and monopole washout constraints The monopoles (antimonopoles) can drift towards antimonopoles (monopoles) through the scatterings on charged particles of plasma. Each of such scattering rate can be estimated as qi σqi M nqi = i (hqi /4π )2T −2nqi = (3/4π 2)ζ ( 3 )T i (hqi /4π )2, where ζ ( 3 ) ≈ 1.20 and the sum goes over relativistic charged particles (we included only fermions) which are at thermal equilibrium at temperature T . After ∼ M/ T such occurrences, a monopole will scatter at large angle and drift towards the antimonopole. Hence, the monopole/antimonopole mean free path is given by [13] λ ≈ M qi σqi M nqi T T M 1/2 1 = B M T 3 1/2 where B = (3/4π 2)ζ ( 3 ) i (hqi /4π )2. As long as the mean free path (18) is smaller than the Coulomb capture distance dc, monopole–antimonopole pairs can annihilate as described. However, as the universe expands and cools down, λ grows faster than dc, and below the temperature T f = 4π h2 where λ ≈ dc, the monopole–antimonopole annihilation rate becomes negligible. Solving the Boltzmann equation for monopole/antimonopole number density and evaluating it at T f one obtains2 [13]: where C = 0.6N −1/2, N is the number of relativistic degrees of freedom and MP is the Planck mass. Below T f this number density simply dilutes as T −3 due to the expansion of the universe. The monopole/antimonopole number density is constrained by the standard Big Bang nucleosynthesis. Namely, at T = 1 MeV the monopole/antimonopole density should be such that n/ T 3 = n f / T f3 (1MeV) M . Plugging in the numbers B ≈ 3 and C ≈ 0.06 and imposing the obvious requirement T f < Tc, we obtain from (21) the following upper bound on the monopole mass: M < 2.28 · 104 TeV. Hence, it is seen that the monopoles required to suppress sphalerons in the broken phase can still satisfy the nucleosynthesis constraints. As has been mentioned above, quark/lepton scatterings off monopoles and antimonopoles also lead to unsuppressed anomalous B + L violation [20]. These processes must also decouple once the equilibrium is achieved, otherwise they will washout the asymmetry. Hence, we demand the rate of such processes at T f , σqi M n f , is less than the expansion rate of the universe, H (T f ) = T f2/C MP , which implies (19) (20) (21) 4 Conclusion In this paper we have postulated the existence of electroweak monopoles regularized within the Born–Infeld hypercharge extension of the Standard Model. Such monopoles (and antimonopoles) must be copiously produced during the electroweak phase transition and can drive local nonequilibrium in plasma. The production of the monopoles cost in energy, thus postponing electroweak phase transition. We have shown that if the monopole mass, defined through the Born–Infeld mass parameter, is within a narrow range 0.9 · 104 TeV < M < 2.3 · 104 TeV, sphaleron mediated processes can be made ineffective, thus preventing washout of the previously generated matter–antimatter asymmetry, while still satisfying the nucleosynthesis constraints. We have also verified that anomalous B + L violation processes due to the quark/lepton–monopole scatterings, while being active during the phase transition at ∼ Tc, become suppressed in the broken phase (T < Tc) due to the efficient enough monopole–antimonopole annihilation. If the electroweak phase transition is indeed accompanied by the production of the electroweak monopoles of mass, M ∼ 104 TeV, a new mechanism for the electroweak baryogenesis can be realized. Namely, out-of-equilibrium quark/lepton scatterings off monopoles may generate nonzero B + L number due to the anomaly. The issue of CP violation, which left outside this paper, must be considered carefully. We plan to study this mechanism in more detail in future work. Acknowledgements We would like to thank Tsutomu Yanagida for useful discussions. This work was partially supported by the Australian Research Council. Note added After the submission of this paper, a new, more stringent constraint on the lower bound of the Born–Infeld parameter, √β, has been obtained in [21] by considering light-by-light scattering at the LHC. However, the monopole masses considered in this paper, M ∼ 104 TeV, are unaffected. Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecomm ons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. Funded by SCOAP3. M < 4π BT f α3 , where α ≈ 1/137 is the fine structure constant. Taking into account Eq. (19), one immediately sees that the above inequality is always satisfied, without implying any extra constraint. 2 Here, for the sake of simplicity, we ignore the potential imbalance between the monopole and antimonopole number densities due to CP violation. 14. A. Rajantie, Phys. Rev. D 68, 021301 (2003). doi:10.1103/ PhysRevD.68.021301. arXiv:hep-ph/0212130 15. H. Kim, Phys. Rev. D 61, 085014 (2000). doi:10.1103/PhysRevD. 61.085014. arXiv:hep-th/9910261 16. F. 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Suntharan Arunasalam, Archil Kobakhidze. Electroweak monopoles and the electroweak phase transition, The European Physical Journal C, 2017, 444, DOI: 10.1140/epjc/s10052-017-4999-y