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Fractionally charged extended objects and superselection rules

Fractionally charged extended objects and superselection rules
Narendra Sahu? and Urjit A. Yajnik?
Department of Physics, Indian Institute of Technology, Mumbai 400076 INDIA Topological objects resulting from symmetry breakdown may be either stable or metastable depending on the pattern of symmetry breaking. However, if they trap zero-energy modes of fermions, and in the process acquire non-integer fermionic charge, the metastable con?gurations also get stabilized. In the case of Dirac fermions the spectrum of the number operator shifts by 1/2. In the case of majorana fermions it becomes useful to assign negative values of fermion number to a ?nite number of states occupying the zero-energy level, constituting a majorana pond. We determine the parities of these states and prove a superselection rule. Thus decay of objects with half-integer fermion number is not possible in isolation or by scattering with ordinary particles. The result has important bearing on cosmology as well as condensed matter physics.
PACS numbers: 11.27.+d, 11.30.Er, 11.30.Fs, 98.80.Cq

arXiv:hep-th/0208027v3 9 Aug 2004


Solitons present the possibility of extended objects as stable states within Quantum Field Theory. Although these solutions are obtained from semi-classical arguments in weak coupling limit, their validity as quantal states is justi?ed based on the associated topological conservation laws. A more curious occurrence is that of fermionic zero-energy modes trapped on such solutions. Their presence requires, according to well known arguments[1][2], an assignment of half-integer fermion number to the solitonic states. In the usual treatment, the back reaction of the fermion zero-modes on the soliton itself is ignored. However, the fractional values of the fermionic charge have interesting consequence for the fate of the soliton if the latter is not strictly stable. The reason for this is that if the con?guration were to relax to trivial vacuum in isolation, there is no particle-like state available for carrying the fractional value of the fermionic charge. Dynamical stability of such objects was pointed out in [3], in cosmological context in [4], [5] and more recently in [6][7][8]. Fractional fermion number phenomenon also occurs in condensed matter systems and its wide ranging implications call for a systematic understanding of the phenomenon. The impossibility of connecting half-integer valued states to integer valued states suggests that a superselection rule[9] [10] is operative. In a theory with a conserved charge (global or local), a superselection rule operates among sectors of distinct charge values because the conservation of charge is associated with the inobservability of rescaling operation Ψ → eiQ Ψ. For the case of the Dirac fermions, the gauge symmetry is broken, however the overall phase corresponding to the fermion number continues to be a symmetry of the effective theory. This permits independent rescaling of the sectors with different values of the fermionic number; thus superselecting bosonic from fermionic sectors. In the case at hand, half-integer values occur, preventing such states from decaying in isolation to the trivial ground state [3] [4]. For the case of majorana fermions where the number operator is not conserved by interactions the validity of such results is far from obvious. However, the occurrence of half-integral values can be shown to be intimately connected to the charge

conjugation invariance[11] of the theory. Here we show that in such a case it is possible to assign parities to the lowest energy solitonic sector which are compatible with parity assignment in the vacuum sector. A superselection rule can then be proved for majorana fermions. In the following we begin with constructing explicit examples of cosmic strings which are metastable and have odd number of zero-modes, for both the cases of Dirac and Majorana masses. The masses in each case are derived from spontaneous symmetry breaking. We then discuss assignment of fermion number to topological objects, including the need for a ?nite spectrum of negative values for states of trapped majorana fermions. Subsequently we derive the required superselection rule. The paper ends with summary and conclusion.


Here we construct two examples in which the topological objects of a low energy theory are metastable due to the embedding of the low energy symmetry group in a larger symmetry group at higher energy. Examples of this kind were considered in [14]. Borrowing the strategies for bosonic sector from there, we include appropriate fermionic content to ensure the zero-modes.

A Dirac fermions

Consider ?rst the theory of two scalars Σ and σ respectively real triplet and complex doublet under a local SU(2). The Lagrangian is taken to be

L= ?

1 ?νa a 1 F F?ν + D? Σ · D? Σ + D? σ? D? σ 4 2 ? λ1 (Σ · Σ ? η2 )2 ? λ2(σ? σ ? η2 )2 1 2 + λ12 η1 Σ · σ? τσ


where isovector notation is used and τ are the Pauli matrices. It is assumed that η1 ? η2 and that the coupling λ12 > 0 satis?es λ12 η2 ? λ2 η2 1 2

2 The vacuum expectation value (VEV) Σ = (0 0 η1 )T breaks the SU(2) to the U(1) generated by exp(iτ3 α/2). The effective theory of the σ can be rewritten as the theory of two complex scalar σu and σd for the up and and the down components respectively. The potential of the effective theory favors the minimum σu = η2 , σd = 0 (2) possess a majorana mass. Thus fermions that are asymptotically seen as majorana particles can possess odd number of zero mode on the vortex. Finally we present the case where majorana mass is spontaneously generated at the same scale at which the vortex forms. Consider an SU(3) theory (global or local) which is broken to identity by two scalars, Φ an octet acquiring a VEV η1 λ3 (λ3 ? here being the third Gell-Mann matrix) and φ, a 3, acquiring k = η δk2 , with η ? η . Thus the VEV φ 2 2 1 8 3 SU(3) ?→ U(1) ?→ I (6)

In the effective theory σu enjoys a U(1) invariance σu → eiα σu which is broken by the above VEV to Z ≡ {e2nπi }, n = 1, 2, . . .. This makes possible vortex solutions with an ansatz in the lowest winding number sector σu (r, θ) = η2 f (r)e


The vortex con?guration is a local minimum, however it can decay by spontaneous formation of a monopole-antimonopole pair [14]. These monopoles are permitted by the ?rst breaking SO(3) → SO(2) in the Σ sector. Paraphrasing the discussion of [14], we have SU(2) →U(1) → Z. The vortices are stable in the low energy theory because π1 (U(1)/Z) is nontrivial. But 3 in the SU(2), the Z lifts to {e4nπiτ /2 } = I making it possible to unwind the vortex by crossing an energy barrier. Consider now the introduction of a doublet of fermion species ψL ≡ (NL , EL ) assumed to be left handed and a singlet right handed species NR . The Yukawa coupling of these to the σu is given by hNR σ? ψL , which in the vortex sector reads

It can be checked that this pattern of VEVs can be generically obtained from the quartic scalar potential of the above Higgses. The ?rst phase of breaking gives rise to monopoles, while the second gives rise to cosmic strings. The strings however are unstable because the vacuum manifold of the full theory is simply connected. Now add a multiplet of left-handed fermions belonging to 15. Its mass terms arise from the following coupling to the 3

L Majorana = hM ψC k ψ{lm} φr (εilr δn δk ) n j m

{i j}


L σ?ψ ? hη2 f (r)(eiθ NR NL + h.c.)


The lowest energy bound states resulting from this coupling are characterized by a topological index, [12] I ≡ nL ? nR where nL and nR are the zero modes of the left handed and the right handed fermions respectively. This index can be computed using the formula [12][13]

The indices symmetric under exchange have been indicated by curly brackets. No mass terms result from the 8 because it cannot provide a singlet from tensor product with 15 ? 15 [15]. After substituting the φ VEV a systematic enumeration {22} {22} shows that all but the two components ψ1 and ψ3 acquire majorana masses at the second stage of the breaking. Speci?cally we ?nd the majorana mass matrix to be indeed rank 13. Thus, using either of the results [16] or [13] i.e., eq. (5) we can see that there will be 13 zero modes present in the lowest winding sector of the cosmic string.


1 (ln detM)|2π θ=0 2πi


where M is the position dependent effective mass matrix for the fermions. In the present case this gives rise to a single zero-energy mode for the fermions of species N. According to well known reasoning [1] to be recapitulated below, this requires the assignment of either of the values ±1/2 to the fermion number of this con?guration. We shall show below that this induces stability of the vortex against spontaneous decay in isolation.
B Majorana fermions

We now recapitulate the reasoning behind the assignment of fractional fermion number. We focus on the Majorana fermion case, which is more nettlesome, while the treatment of the Dirac case is standard [1][2]. In the prime example in 3 + 1 dimensions of a single left-handed fermion species coupled to an abelian Higgs model according to

L ψ = iψγ? D? ψ ? (hφψC ψ + h.c.)


the following result has been obtained[16]. For a vortex oriented along the z-axis, and in the winding number sector n, the fermion zero-modes are of the form 1 ψ0 (x) = U(r)eilθ + V ? (r)ei(n?1?l)θ gl (z + t) (9) 0 In the presence of the vortex, τ3 (here representing Lorentz transformations on spinors) acts as the matrix which exchanges solutions of positive frequency with those of negative frequency. It is therefore identi?ed as the “particle conjugation” operator. In the above ansatz, the ψ in the zerofrequency sector are charge self-conjugates, τ3 ψ = ψ, and

The example above can be extended to the case where the N is a majorana fermion. Being a singlet N admits a mass term C MM NR NR , MM signifying majorana mass. This could also be a spontaneously generated mass due to the presence of a neuC tral scalar χ with coupling terms hM NR NR χ + h.c.. If this χ acquires a VEV at energies higher than the Σ, the N particles

3 have an associated left moving zero mode along the vortex. The functions satisfying τ3 ψ = ?ψ are not normalizable. The situation is reversed when the winding sense of the scalar ?eld is reversed, ie, for σu ?e?inθ . In the winding number sector n, regular normalizable solutions[16] exist for for 0 ≤ l ≤ n ? 1. The lowest energy sector of the vortex is now 2n -fold degenerate, and each zero-energy mode needs to be interpreted as contributing a value ±1/2 to the total fermion number of the individual states[1]. This conclusion is dif?cult to circumvent if the particle spectrum is to re?ect the charge conjugation symmetry of the theory [11]. The lowest possible value of the induced number in this sector is ?n/2. Any general state of the system is built from one of these states by additional integer number of fermions. All the states in the system therefore possess half-integral values for the fermion number if n is odd. One puzzle immediately arises, what is the meaning of negative values for the fermion number operator for Majorana fermions? In the trivial vacuum, particles are identi?ed with anti-particles according to the Majorana condition with the simplest choice of phases. Now we ?nd

C c C ? C |? = C |+ ? ±c(C |? ) = (C |+ )
This relation has the simplest non-trivial solution
? C |? = ηC |? + C |+ = ηC |+

(16) (17)



? + where, for the consistency of (15) and (17) ηC and ηC must satisfy ? + ± (ηC )?1 ηC = 1


Finally we verify that we indeed get values ±1/2 for N. The standard fermion number operator 1 NF = [ψ? ψ ? ψψ?] 2 acting on these two states gives, (20)

C ψC ? = ±ψ

(10) 1 1 (c c? ? c? c) |± = ± |± 2 2 (21)

making negative values for the number meaningless. Here C is the charge conjugation operator and the choice between + and ? on the right hand side has to be determined from experiment. We shall ?rst verify that in the zero-mode sector we must indeed assign negative values to the number operator. It is suf?cient to treat the case of a single zero-mode, which generalizes easily to any larger number of zero-modes. The number operator possesses the properties [N, ψ] = ?ψ and [N, ψ? ] = ψ? (11) (12)

C NC ? = N

Had it been the Dirac case, there should be a minus sign on the right hand side of eq. (12). This is absent due to the Majorana condition. The fermion ?eld operator is now expanded as ψ = cψ0 +

The number operator indeed lifts the degeneracy of the two states. For s number of zero modes, the ground state becomes 2s -fold degenerate, and the fermion number takes values in integer steps ranging from ?s/2 to +s/2. For s odd the values are therefore half-integral. Although uncanny, these conclusions accord with some known facts. They can be understood as spontaneous symmetry breaking for fermions[17]. The negative values of the number thus implied occur only in the zero-energy sector and do not continue inde?nitely to ?∞. Instead of an unfathomable Dirac sea we have a small Majorana pond at the threshold.


∑ aκ,sχκ,s (x) + ∑ bk,s uk,s(x) + h.c.
κ,s k,s


where the ?rst summation is over all the possible bound states of non-zero frequency with real space-dependence of the form ? e?κ·x⊥ in the transverse space directions x⊥ , and the second summation is over all unbound states, which are asymptotically plane waves. Note that hermitian conjugates of the operators aκ,s and bk,s are included above in the “h.c.” but not that of the solitary mode operator c. Then the Majorana condition (10) requires that we demand

C c C ? = ±c


C c? C ? = ±c?


Unlike the Dirac case, the c and c? are not exchanged under charge conjugation. The only non-trivial irreducible realization of this algebra is to require the existence of a doubly degenerate ground state with states |? and |+ satisfying c|? = |+ and c? |+ = |? (15)

As a step towards deriving our superselection rule, we determine the parities of the zero-energy states. Majorana fermions can be assigned a unique parity [10], either of the values ±i. Let us choose i to be the parity of the free single fermion states in the trivial vacuum. The fermion spectrum should look the same as trivial vacuum far away from the vortex [21]. In turn the parities of the latter states should be taken to be the same as those of the trivial ground state. Next, any of these asymptotic free fermions is capable of being absorbed by the vortex (see for instance [18]). In the zero energy sector this absorption would cause a transition from | ? 1/2 to |1/2 and cause a change in parity by i. Thus the level carrying fermion number +1/2 should be assigned a parity eiπ/2 relative to the ?1/2 state. Symmetry between the two states suggests that we assign parity eiπ/4 to the NF = 1/2 and e?iπ/4 to the NF = ?1/2 states. We now show the inappropriateness of superposing states of half-integer valued fermion number and integer valued

4 fermion number [9]. The operation P 4 , parity transformation performed four times must return the system to the original state, upto a phase. Consider forming the state 1 ΨS = √2 (|1/2 + |1 ) from states of half-integer and integer value for the fermion number. But calculated in [14]. In condensed matter systems the best known example is of charge carriers of charge half the electronic charge in polyacetylene [20] where the underlying solitons have been identi?ed as stable kinks. It would be interesting to ?nd intrinsically metastable objects stabilized by this mechanism. Finally it is interesting to conjecture about the fate of loops of cosmic strings. The zero modes on closed string loops have not been studied in detail, though dynamical stability due to superconductivity has been identi?ed. If loops carry fractional fermion number and get stabilized by this mechanism that also would present very interesting possibilities for Cosmology. We thank thank Sumit Das and P. Ramadevi for their for critical comments on the manuscript.

P 4 ΨS = √ (?|1/2 + |1 )

1 2


Thus this operation identi?es a state with another orthogonal to it. Similarly, application of P 2 which should also leave the physical content of a state unchanged results in yet an1 other linearly independent state, √2 (i|1/2 ? |1 ). Thus the space of superposed states collapses to a trivial vector space. The conclusion therefore is that it is not possible to superpose such sectors. In turn there can be no meaningful operator possessing non-trivial matrix elements between the two spaces. This completes our proof of the theorem.

? ?

Metastable classical lumps, also referred to as embedded defects can be found in several theories. The conditions on the geometry of the vacuum manifold that give rise to such defects were spelt out in [14]. We have studied the related question of fermion zero-energy modes on such objects. It is possible to construct examples of cosmic strings in which the presence of zero-modes signals a fractional fermion number both for Dirac and Majorana masses. It then follows that such a cosmic string cannot decay in isolation because it belongs to a distinct superselected Quantum Mechanical sector. Thus a potentially metastable object can enjoy induced stability due to its bound state with fermions. Although decay is not permitted in isolation, it certainly becomes possible when more than one such objects come together in appropriate numbers. In the early Universe such objects could have formed depending on the unifying group and its breaking pattern. Their disappearance would be slow because it can only proceed through encounters between objects with complementary fermion numbers adding up to an integer. Another mode of decay is permitted by change in the ground state in the course of a phase transition. When additional Higgs ?elds acquire a vacuum expectation value, in turn altering the boundary conditions for the Dirac or Majorana equation, the number of induced zero modes may change from being odd to even[22], thus imparting the loops an integer fermion number. The decay can then proceed at the rates

[1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22]

Electronic address: narendra@phy.iitb.ac.in Electronic address: yajnik@phy.iitb.ac.in R. Jackiw and C. Rebbi, Phys Rev. D13, 3398 (1976) R. Jackiw, Rev. Mod. Phys. 49, 681(1977) H. de Vega, Phys. Rev. D18, 2932 (1978) A. Stern; Phys. Rev. Lett.52, 2118(1983) A. Stern and U. A. Yajnik, Nucl. Phys. B267, 158 (1986) S. C. Davis, A. C. Davis and W. B. Perkins, Phys. Lett. B 408, 81 (1997) A. C. Davis, S. C. Davis and W. B. Perkins, Proceedings of COSMO99, arXiv:hep-ph/0005091 A. C. Davis, T. W. B. Kibble, M. Pickles and D. A. Steer, Phys. Rev. D62 083516 (2000) G. C. Wick, A. S. Wightman and E. P. Wigner, Phys. Rev. 88, 101 (1952) S. Weinberg, The Quantum Theory of ?elds, Vol. I, Cambridge University Press, 1996 E. C. G. Sudarshan and U. A. Yajnik, Phys. Rev. D33, 1830 (1986) E. J. Weinberg, Phys. Rev. D24, 2669 (1981) N. Ganoulis and G. Lazarides, Phys. Rev. D38 547 (1988) J. Preskill and A. Vilenkin, Phys. Rev. D47, 2324 (1993) R. Slansky, Phys. Rept. 79, 1 (1981). R. Jackiw and P. Rossi, Nucl. Phys.B190, 681 (1981) R. MacKenzie and F. Wilczek, Phys. Rev. D 30, 2194 (1984) S. C. Davis, W. B. Perkins and A. C. Davis, Phys. Rev. D 62, 043503 (2000) U. A. Yajnik, H. Widyan, D. Choudhari, S. Mahajan and A. Mukherjee, Phys. Rev. D 59, 103508 (1999) R. Jackiw and J. R. Schrieffer, Nucl. Phys. B 190 (1981) 253. This should be understood to be the clustering property of local ?eld theory being obeyed by the vortex ground state. Such a possibility, though for topologically stable string can be found for realistic uni?cation models in [5] [6] [18] [19].



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