PLB34363S0370-2693(19)30006-110.1016/j.physletb.2018.12.069The Author(s)TheoryRemark on the open string pair production enhancementQiangJiaJ.X.Lujxlu@ustc.edu.cnInterdisciplinary Center for Theoretical Study, University of Science and Technology of China, Hefei, Anhui 230026, ChinaInterdisciplinary Center for Theoretical StudyUniversity of Science and Technology of ChinaHefeiAnhui230026ChinaEditor: N. LambertAbstractRecent studies by one of the present authors along with his collaborators in [1–4] show that there exist the so-called open string pair production for a possible simplest system of two Dp branes, placed parallel at a separation and with each carrying different electric flux, in Type II superstring theories. Further this pair production can be greatly enhanced when a magnetic flux, sharing no common field strength index with the electric one, is added, implying then p≥3. Given this, one may wonder if further enhancement can be achieved by adding more magnetic flux(es) in a similar fashion. In this paper, we explore this possibility. It turns out that adding more such magnetic flux diminishes rather than enhances the pair production rate. This actually implies that the largest enhancement occurs at p=3 when the same realistic electric and magnetic fluxes are applied for all p≥3. Curiously one of D3 branes may be our own world and if so, the enhancement gives a possible opportunity to detect the pair production, therefore to test the underlying string theories.1IntroductionApplying a constant electric field to the vacuum of quantum electrodynamics (QED) gives rise to the so-called Schwinger pair production [5]. It is natural to ask if an analogous process exists in various string theories. This was pursued in unoriented bosonic string and type I superstring a while ago in [6,7]. We focus in this paper on Dp branes in the oriented Type II superstring theories for which the worldvolume electric and magnetic fluxes can be considered.A Dp brane in Type II superstring theories is a non-perturbative Bogomol'ny–Prasad–Sommereld (BPS) solitonic vacuum-like object (for example, see [8]), preserving one half of spacetime supersymmetry, and as such it is stable. Its dynamics can also be described by an oriented perturbative open string with its two ends obeying the so-called Neumann boundary conditions along the brane directions and the Dirichlet ones along the directions transverse to the brane [9] when the string coupling gs is small. This open string is charge-neutral in the sense that its two ends carry charge + and −, respectively, with total zero net-charge.Just like the virtual electron/positron pair in QED vacuum, we have here the pair of virtual open string/anti open string, created from the Dp brane vacuum at certain instant, existing for a short period of time, then annihilating back to the vacuum. An observer on the brane can only sense the ends, not the whole, of these open strings, as charged or anti charged particles. So the pair of virtual open string/anti open string appears to the brane observer as two pairs of virtual charged/anti charged particles, each of which consists of two nearby ends of the string pair. So the present quantum fluctuations are different from those in QED.In a spirit to the Schwinger pair production[5], one would also expect to produce the charged particle/anti-charged particle or the open string pair if a constant worldvolume electric field is applied to an isolated Dp brane. However, the stringy computations give a null result due to the open string being charge-neutral and its two ends experiencing the same electric field [3,6]. This is consistent with that a Dp carrying a constant electric field is a 1/2 BPS non-threshold bound state [10], therefore being stable rather than unstable. So this system cannot decay via the open string pair production. This can also be understood as the lack of the force on either of the open string or the anti open string in the pair to pull them apart since the net-force acting on either of them vanishes under the action of the constant applied electric flux less than its critical value.11When the applied electric flux reaches its critical value unity, the forces, equal in magnitude but opposite in direction, acting at the two ends of the open string or anti open string can break it and the pair production instability develops. However, in practice, we never reach this critical electric flux in laboratory and so this will not be an issue for the purpose of the present discussion. In other words, there is no Schwinger-type pair production here.In order to have the open string pair production, a possibility is to let the two ends of the open string experience different electric fields since the charge-neutral property of the string cannot be altered. A possible simplest setup for this is to consider a system of two Dp branes placed parallel at a separation and with each carrying a different electric flux. The open strings produced, if any, should come from those connecting the two Dp branes along the transverse directions, therefore related to the extra dimensions, from the viewpoint of the brane observer. Stringy computations do give a non-vanishing pair production rate [1] but it is usually vanishingly small for any realistic electric flux applied, which is usually much smaller than the critical one. This rate can however be greatly enhanced if we add also a magnetic flux in a way that the two fluxes do not share a common field strength index [2–4].We denote now the general worldvolume dimensionless flux on one Dp by Fˆ and on the other by Fˆ′, both being antisymmetric (1+p)×(1+p)-matrices with the same structure. For this enhancement, we can choose, without loss of generality, the non-vanishing components for Fˆ as(1)Fˆ01=−Fˆ10=−fˆ1,Fˆ23=−Fˆ32=−gˆ2, and the same non-vanishing components for Fˆ′ but denoting each with a prime. Here fˆ1 stands for the electric flux with |fˆ1|<1 and gˆ2 the magnetic flux with |gˆ2|<∞. Note that the dimensionless flux Fˆ or Fˆ′ is related to the corresponding laboratory one F or F′ via Fˆ=2πα′F and Fˆ′=2πα′F′ with α′ the Regge slope parameter, related to the fundamental string tension Tf as Tf=1/(2πα′). This structure of the fluxes concerning their non-vanishing components must imply p≥3.The study given in [4] for various cases of two fluxes on each brane indicates that the most efficient and direct enhancement of the pair production is by adding a magnetic flux on each brane as specified above. This structure makes us wonder if further enhancement can be possible.22In general, placing an infinitely extended Dp in spacetime will cause it to curve. For our purpose, we try to avoid this to happen at least to the probe distance in which we are interested. For this, we need to limit our discussion in this paper to p≤6 cases since these Dp branes have well-behaved supergravity configurations which are all asymptotically flat. Moreover, when the string coupling is small, i.e. gs≪1, placing one such Dp in spacetime will keep the spacetime flat even for a probe distance to the brane in the substringy scale α′1/2≫r≫gs1/(7−p)α′1/2 as discussed in section 2 of [11]. So this indeed meets our requirement. For example, for p≥5, we might have a further enhancement of the rate if we add one more magnetic flux, in addition to the above (1), of the form Fˆ45=−Fˆ54=−gˆ3 (and in a similar fashion for Fˆ′). As discussed in footnote 2, this is actually the only case possible for this purpose. Either answer of this investigation will be important for us to determine which system can give rise to the largest possible pair production.In this paper, we investigate this possible enhancement. It turns out that adding such additional magnetic flux diminishes rather than enhances the pair production, assuming the fluxes given in (1) remain the same. This result implies that the pair production rate computed using fluxes in (1), in the absence of the additional fluxes gˆ3 and gˆ3′, is the largest for each p≥5. Combined this with the previous result given in [3], we conclude that the rate for the system of two D3 branes is the largest among the p≥3 cases when we take the same fluxes as given in (1) for all the cases. Curiously this is interesting since one of the D3 can be our own 4-dimensional world. This also makes it a possibility for its detection.As mentioned earlier, the pair production is related to the open strings connecting the two Dp branes, therefore to the dimensions transverse to the branes. From the perspective of the brane observer, the open string pair appears as the charged particle/anti-charged particle pair and the transverse dimensions appear as extra-dimensions. So a detection of this pair production by the brane observer implies the existence of extra dimensions. It also provides a test of the underlying string theories.This paper is organized as follows. In section 2, we follow the steps outlined in [4] using the closed string boundary states to present first the closed string cylinder interaction amplitude in terms of various θ-functions between the two Dp branes with one additional magnetic flux on each brane for p≥5. We will specify the structure of these fluxes in this section explicitly. We then use Jacobi transformation to pass this amplitude to the open string annulus one for each case. In section 3, we will use this open string annulus amplitude to obtain the non-perturbative open string pair production rate following [2,3,7], analyze this rate and discuss its significance and implications. We discuss and conclude this paper in section 4.2The open string annulus amplitudeIn this section, we will obtain and study the open string annulus interaction amplitude between two Dp-branes, as specified earlier, with one additional magnetic flux on each brane for p≥5. The simpler approach, when both electric and magnetic fluxes are present, is to compute the corresponding closed string cylinder amplitude first. This is due to that each such Dp brane carrying these fluxes can be easily represented by its closed string boundary state (for example, see [12,13]). The cylinder amplitude can be easily obtained following the steps outlined in [4]. Once having this amplitude, we can obtain the corresponding open string annulus one simply by a Jacobi transformation on this one.2.1The closed string cylinder amplitudeFollowing [4], we now briefly outline the steps to compute the closed string cylinder interaction amplitude between two Dp, placed parallel at a separation and with one brane carrying the fluxes(2)Fˆ=[0−fˆ100000⋯fˆ1000000⋯000−gˆ2000⋯00gˆ20000⋯00000−gˆ30⋯0000gˆ300⋯0000000⋯⋮⋮⋮⋮⋮⋮⋮⋱](p+1)×(p+1), and the other carrying the fluxes(3)F′ˆ=[0−fˆ1′00000⋯fˆ1′000000⋯000−gˆ2′000⋯00gˆ2′0000⋯00000−gˆ3′0⋯0000gˆ3′00⋯0000000⋯⋮⋮⋮⋮⋮⋮⋮⋱](p+1)×(p+1). From the non-vanishing components of Fˆ or Fˆ′, it is clear p≥5. There are in general two contributions to this amplitude, one from the so-called NS–NS sector and the other from the R–R sector, respectively. The total closed string cylinder amplitude is the sum of the two after the so-called Gliozzi–Scherk–Olive (GSO) projection for each, namely,(4)Γ=ΓNSNS+ΓRR, where the GSO projected amplitudes in both NSNS-sector and RR-sector are(5)ΓNSNS=12[ΓNSNS(+)−ΓNSNS(−)],ΓRR=12[ΓRR(+)+ΓRR(−)]. Here ΓNSNS(±) and ΓRR(±) can be read, for the present case, from the corresponding general amplitudes, respectively, given in [4]. We have then, with ηη′=±,(6)ΓNSNS(η′η)=Vp+1[(1−fˆ12)(1−fˆ1′2)(1+gˆ22)(1+gˆ2′2)(1+gˆ32)(1+gˆ3′2)]12(8π2α′)1+p2∫0∞dtt9−p2e−y22πα′t|z|×∏n=1∞(1+η′η|z|2n−11−|z|2n)2∏a=13(1+λaη′η|z|2n−1)(1+λa−1η′η|z|2n−1)(1−λa|z|2n)(1−λa−1|z|2n), and(7)ΓRR(η′η)=Vp+1[(1−fˆ12)(1−fˆ1′2)(1+gˆ22)(1+gˆ2′2)(1+gˆ32)(1+gˆ3′2)]12(8π2α′)1+p20R〈B′,η′|B,η〉0R×∫0∞dtt9−p2e−y22πα′t∏n=1∞(1+η′η|z|2n1−|z|2n)2∏a=13(1+η′ηλa|z|2n)(1+η′ηλa−1|z|2n)(1−λa|z|2n)(1−λa−1|z|2n). In the above, Vp+1 denotes the volume of the brane worldvolume, |z|=e−πt<1, y the brane separation and the zero-mode contribution in the RR-sector can be evaluated with the fluxes given in (2) and (3), following [14,15], as(8)〈B′,η′|B,η〉0R0R≡〈Bsgh′,η′|Bsgh,η〉0R0R×0R〈Bψ′,η′|Bψ,η〉0R,=−24(1−fˆ1fˆ1′)(1+gˆ2gˆ2′)(1+gˆ3gˆ3′)(1−fˆ21)(1−fˆ1′2)(1+gˆ22)(1+gˆ2′2)(1+gˆ32)(1+gˆ3′2)δηη′,+, where |Bsgh,η〉 denotes the boundary state of superghosts β and γ while |Bψ,η〉 the boundary state of matter field ψμ. The λa for a=1,2,3 are given, respectively, as(9)λ1+λ1−1=2(1+fˆ12)(1+fˆ1′2)−4fˆ1fˆ1′(1−fˆ12)(1−fˆ1′2),λ2+λ2−1=2(1−gˆ22)(1−gˆ2′2)+4gˆ2gˆ2′(1+gˆ22)(1+gˆ2′2),λ3+λ3−1=2(1−gˆ32)(1−gˆ3′2)+4gˆ3gˆ3′(1+gˆ32)(1+gˆ3′2). We have then the total amplitude from (7), (6) and (4) as(10)Γ=Vp+1[(1−fˆ12)(1−fˆ′21)(1+gˆ22)(1+gˆ2′2)(1+gˆ32)(1+gˆ3′2)]122(8π2α′)1+p2∫0∞dtt9−p2e−y22πα′t×[|z|−1(∏n=1∞An−∏n=1∞Bn)−24cosπνcosπν′cosπν″∏n=1∞Cn], whereAn=(1+|z|2n−11−|z|2n)2∏a=13(1+λa|z|2n−1)(1+λa−1|z|2n−1)(1−λa|z|2n)(1−λa−1|z|2n),Bn=(1−|z|2n−11−|z|2n)2∏a=13(1−λa|z|2n−1)(1−λa−1|z|2n−1)(1−λa|z|2n)(1−λa−1|z|2n),(11)Cn=(1+|z|2n1−|z|2n)2∏a=13(1+λa|z|2n)(1+λa−1|z|2n)(1−λa|z|2n)(1−λa−1|z|2n). In the above, we have set λ1=e2πiν,λ2=e2πiν′ and λ3=e2πiν″, and we also make use of (8) and (9). We now express the amplitude in terms of various θ-functions and the Dedekind η-function, following their standard definitions given, for example, in [16]. We have then the amplitude (10) as(12)Γ=22iVp+1|fˆ1−fˆ1′||gˆ2−gˆ2′||gˆ3−gˆ3′|(8π2α′)1+p2∫0∞dtt9−p2e−y22πα′tη3(it)θ1(ν|it)θ1(ν′|it)θ1(ν″|it)×[θ3(0|it)θ3(ν|it)θ3(ν′|it)θ3(ν″|it)−θ4(0|it)θ4(ν|it)θ4(ν′|it)θ4(ν″|it)−θ2(0|it)θ2(ν|it)θ2(ν′|it)θ2(ν″|it)],=23iVp+1|f1−f1′||g2−g2′||g3−g3′|(8π2α′)1+p2∫0∞dtt9−p2e−y22πα′tη3(it)×θ1(ν+ν′+ν″2|it)θ1(ν−ν′−ν″2|it)θ1(ν−ν′+ν″2|it)θ1(ν+ν′−ν″2|it)θ1(ν|it)θ1(ν′|it)θ1(ν″|it), where in the last equality we have made use of the identity(13)2θ1(ν+ν′+ν″2|it)θ1(ν−ν′−ν″2|it)θ1(ν−ν′+ν″2|it)θ1(ν+ν′−ν″2|it)=[θ3(0|it)θ3(ν|it)θ3(ν′|it)θ3(ν″|it)−θ4(0|it)θ4(ν|it)θ4(ν′|it)θ4(ν″|it)−θ2(0|it)θ2(ν|it)θ2(ν′|it)θ2(ν″|it)], which is a special case of the more general identity given in [17]. Given (9), the parameter ν is actually imaginary and can be set as ν=iν0 with ν0∈[0,∞) while both ν′ and ν″ are real and for convenience can be set as ν′=ν1 and ν″=ν2 with ν1,ν2∈[0,1]. In terms of the applied fluxes, we have from (9)(14)coshπν0=1−fˆ1fˆ1′(1−fˆ12)(1−fˆ1′2),sinhπν0=|fˆ1−fˆ1′|(1−fˆ12)(1−fˆ′21);cosπν1=1+gˆ2gˆ2′(1+gˆ22)(1+gˆ2′2),sinπν1=|gˆ2−gˆ2′|(1+gˆ22)(1+gˆ′22);cosπν2=1+gˆ3gˆ3′(1+gˆ32)(1+gˆ3′2),sinπν2=|gˆ3−gˆ3′|(1+gˆ32)(1+gˆ′23). The last equality of the amplitude (12) can be expressed explicitly as(15)Γ=4KVp+1[coshπν0−cosπ(ν1+ν2)][coshπν0−cosπ(ν1−ν2)](8π2α′)1+p2∫0∞dtt9−p2e−y22πα′t∏n=1∞Dn, where(16)K=[(1−fˆ12)(1−fˆ1′2)(1+gˆ22)(1+gˆ2′2)(1+gˆ32)(1+gˆ3′2)]12, and(17)Dn=∏a=01∏b=01[1−2|z|2ne(−)aπν0cosπ(ν1+(−)bν2)+|z|4ne(−)a2πν0](1−|z|2n)2(1−2|z|2ncosh2πν0+|z|4n)∏i=12(1−2|z|2ncos2πνi+|z|4n). For large brane separation y, the main contribution to the amplitude (15) comes from the large t integration for which |z|=e−πt→0 and Dn≈1. It is then clear that Γ>0, giving an attractive interaction by our conventions between the two Dp branes as expected. For small y, the small t contributes also to the amplitude. Note that in Dn both 1−2|z|2ne±πν0cosπ(ν1±ν2)+|z|4ne±2πν0≥(1−|z|2ne±πν0)2>0 and (1−2|z|2ncos2πνi+|z|4n)≥(1−|z|2n)2>0 but the factor 1−2|z|2ncosh2πν0+|z|4n in the denominator can be negative for small enough t. So this gives an ambiguity about the nature of the interaction for small y since there are an infinite number of such factors appearing in infinite product in the amplitude. So we expect some interesting physics to occur for small y. As will be seen, this can be more transparent in the open string channel which we turn next.2.2The open string annulus amplitudeIn passing the last equality of the closed string cylinder amplitude in (12) to the open string annulus one, we need to use the Jacobi transformation t→t′=1t. For this, we also need the following relations for the θ1-function and the Dedekind η-function,(18)η(τ)=1(−iτ)1/2η(−1τ),θ1(ν|τ)=ie−iπν2/τ(−iτ)1/2θ1(ντ|−1τ). The open string annulus amplitude is then(19)Γ=−23Vp+1|fˆ1−fˆ1′||gˆ2−gˆ2′||gˆ3−gˆ3′|(8π2α′)p+12∫0∞dt′t′p−32e−y2t′2πα′×θ1(ν0−i(ν1+ν2)2t′|it′)θ1(ν0+i(ν1+ν2)2t′|it′)θ1(ν0−i(ν1−ν2)2t′|it′)θ1(ν0+i(ν1−ν2)2t′|it′)η3(it′)θ1(ν0t′|it′)θ1(iν1t′|it′)θ1(iν2t′|it′),=4Vp+1|fˆ1−fˆ1′||gˆ2−gˆ2′||gˆ3−gˆ3′|(8π2α′)p+12∫0∞dttp−32e−y2t2πα′E(ν0,ν1,ν2;t)∏n=1∞Zn, where in the last equality we have dropped the prime on t,(20)E(ν0,ν1,ν2;t)=[coshπ(ν1+ν2)t−cosπν0t][coshπ(ν1−ν2)t−cosπν0t]sinπν0tsinhπν1tsinhπν2t, and(21)Zn=∏a=01∏b=01[1−2|z|2ne(−)aπ(ν1+(−)bν2)tcosπν0t+|z|4ne(−)a2π(ν1+(−)bν2)t](1−|z|2n)2(1−2|z|2ncos2πν0t+|z|4n)∏i=12(1−2|z|2ncosh2πνit+|z|4n). Note that Zn>0 since n≥1, |z|=e−πt and ν1,ν2∈[0,1]. The interesting physics comes from the factor E(ν0,ν1,ν2;t) given in (20). For large t, E(ν0,ν1,ν2;t) has an exponentially growing factor of eπ|ν1−ν2|t, indicating the appearance of a tachyonic shift33In the case of a single magnetic field, a tachyonic shift(s) has been uncovered in the context of unoriented Type I superstring in [20]. This shift can be used to understand the appearance of the present tachyonic one from E(ν0,ν1,ν2;t) for large t for the following reason. For simplicity, we take gˆ3=gˆ3′=0 in (2) and (3) (now ν2=0). The charge-neutral open string connecting the two Dp-branes has its two ends coupled with the respective magnetic field on each brane and gives two coupling parameters, for example, β1=gˆ2 and β2=−gˆ2′, where the charges at the two ends are +1 and −1, respectively. If we rewrite β1=gˆ2=e1gˆ,β2=−gˆ2′=e2gˆ, the present charge-neutral string along the brane directions looks equivalent to the type I superstring with its two ends carrying charge e1 and e2, respectively, in a single magnetic field gˆ. Moreover, combined with the pure electric pair production rate given in [6], this provides us a way to understand qualitatively the property of the rate enhancement found in this paper, namely adding additional magnetic fluxes gˆ3 and gˆ3′ causes the rate with less enhancement, which will be discussed in the following section. Given the above, we would also like to point out that the explicit computations for the open string annulus amplitudes given in [2–4] and here in (19), and the corresponding open string pair production rates facilitate the findings of the respective rate enhancement and the enhancement property uncovered in this paper. as discussed previously in [2–4]. This tachyonic shift is the key factor for the pair production rate enhancement, especially when ν0≪1. The absolute difference |ν1−ν2| in this shift says that adding the additional fluxes gˆ3,gˆ3′ will make the difference smaller, which can also be drawn from [20] in a similar spirit. This hints that the shift will be less effective in enhancing the rate. We will see that this is indeed true in the following section.In the integral representation of the amplitude (19), we have t>0. E(ν0,ν1,ν2;t) blows up at points tk=k/ν0 with k=1,2⋯, which are determined from the zeros of the factor sinπν0t in its denominator. In other words, the integrand has an infinite number of simple poles along the positive t-axis. This indicates that the amplitude has an imaginary part which gives rise to the decay of the underlying system. As we will turn to the next section, this decay is to release the excess energy due to the applied fluxes, via the so-called open string pair production, to relax the underlying system to become a new BPS one.3The open string pair production enhancementGiven what has been said in the previous section, we now compute the non-perturbative decay or the so-called pair production rate from the open string annulus amplitude given in the second equality of (19). Following [6], this rate of pair production per unit worldvolume can be obtained as the imaginary part of this amplitude and is given as the sum of the residues of the poles of the integrand times π,(22)W=−2ImΓVp+1,=8|fˆ1−fˆ1′‖gˆ2−gˆ2′‖gˆ3−gˆ3′|(8π2α′)p+12∑k=1∞(−)k−1(ν0k)p−52e−ky22πα′ν0Ek∏n=1∞Zn,k, where(23)Ek=[coshπ(ν1+ν2)kν0−(−)k][coshπ(ν1−ν2)kν0−(−)k]ksinhπν1kν0sinhπν2kν0, and(24)Zn,k=(1−e−2πnkν0)−4∏a=01[1−(−)ke−2πkν0(n−(−)aν1+ν22)]2[1−(−)ke−2πkν0(n−(−)aν1−ν22)]2[1−e−2kπν0(n−(−)aν1)][1−e−2kπν0(n−(−)aν2)]. Recall here p≥5. As in the previous studies [2–4], for given fluxes, the larger the brane separation y is and/or the larger the integer k is, the smaller the rate is since the corresponding open string, whose mass is given by kyTf with Tf=1/(2πα′) the fundamental string tension, is more massive, therefore more difficult to be produced. The larger |fˆ1−fˆ1′| is, therefore the larger ν0, the larger the rate is. When either of fˆ1 or fˆ1′ reaches its critical value unity, we have ν0=∞ from the first two equations in (14). Then Zn,k blows up for odd k and so does the rate, the occurring of the pair production instability as mentioned earlier in footnote 1. This rate becomes the one given in [4] when we set gˆ3=gˆ3′=0 for which ν2=0 from (14).For realistic laboratory electric fluxes, we expect in general |fˆ1|,|fˆ1′|≪1 and |fˆ1−fˆ1′|≪1. So we have ν0≪1 from (14) which implies Zn,k≈1 and the rate can be approximated by the leading k=1 term. We have also |gˆ2|,|gˆ3|,|gˆ2′|,|gˆ3′|≪1. So ν1 and ν2 are both small and we can replace both |gˆ2−gˆ2′| and |gˆ3−gˆ3′| by their respective πν1 and πν2 from (14). So we have the rate (22) as(25)W≈8π2|fˆ1−fˆ1′|ν1ν2(8π2α′)p+12ν0p−52e−y22πα′ν0[coshπ(ν1+ν2)ν0+1][coshπ(ν1−ν2)ν0+1]sinhπν1ν0sinhπν2ν0. Note that the above rate is symmetric to ν1 and ν2 as it should be. So without loss of generality, we assume ν1≥ν2 from now on. This is consistent with the actual practice in that we always want to obtain the largest enhancement before turning on the second set of magnetic fluxes gˆ3 and gˆ3′. This also gives us the option to set gˆ3=gˆ3′=0 (so ν2=0) in the above rate. With these, we are now ready to compare this rate (25) with gˆ3,gˆ3′≠0 with the one given in [4] for which gˆ3=gˆ3′=0 (also ν2=0) to see the effect of the added fluxes gˆ3,gˆ3′≠0. This latter rate is(26)W(gˆ3=gˆ3′=0)≈8π|fˆ1−fˆ1′|ν1(8π2α′)p+12ν0p−32e−y22πα′ν0[coshπν1ν0+1]2sinhπν1ν0, which is valid for p≥3. For each given p≥5, we have(27)W(gˆ3,gˆ3′≠0)W(gˆ3=gˆ3′=0)=πν2ν0[coshπ(ν1+ν2)ν0+1][coshπ(ν1−ν2)ν0+1][coshπν1ν0+1]2sinhπν2ν0. Let us examine this ratio. For example, if πν2/ν0≪1 while holding fixed a fairly large πν1/ν0 (∼O(5)), we have it to be unity. In other words, adding the additional fluxes doesn't help. We consider now the other case when πν1/ν0≫1 and πν2/ν0∼O(1) or larger. Now the above ratio ∼(πν2/ν0)/sinh(πν2)/ν0)<1. Further when πν2/ν0≫1 (noting ν1≥ν2), this ratio becomes vanishingly small. So adding magnetic fluxes gˆ3 and gˆ3′ in general diminishes rather than enhances the rate.Let us enforce this further. As discussed in detail in [3] in the absence of gˆ3 and gˆ3′, the ratio of dimensionless rates for p=5 and for p=3 for the same applied fluxes is(28)r=(2πα′)3Wp=5(2πα′)2Wp=3=ν04π, which can also be read from the rate given in (26). Let us give an estimate how small this ratio is. For simplicity, we assume fˆ1′=0 and fˆ1=2πα′E with E the laboratory electric field. Note that the current constant electric field limit in laboratory is 8 order of magnitude smaller than the one required for producing the Schwinger pair production which is E∼me2∼10−7GeV2 with me the electron mass. The current constraint for string scale Ms=1/α′ is from a few TeV upto the order of 1016∼1017 GeV (for example, see [18]). If we take one of D3 branes as our own world, even taking E∼10−7GeV2 and α′=1/Ms∼10−3GeV−1, we have the above ratio r=ν0/4π∼10−11, very tiny. Note that adding the additional magnetic fluxes makes us to move from p=3 to p=5. This is worth the effort only if the further enhancement is much greater than 1/r∼1011. However, our earlier discussion above says that this is impossible. In other words, adding fluxes gˆ3 and gˆ3′, giving ν2≤ν1, has no advantage at all over the p=3 rate in the absence of them.So combining this with the previous studies given in [3,4] in the absence of gˆ3 and gˆ3′, we must conclude that the largest rate occurs for the system of two D3 branes considered when the applied fluxes remain the same for all p≥3. This gives us also the advantage to actually test this pair production since one of the D3 can be our own world.4Discussion and conclusionIn this paper, we consider a system of two Dp branes, placed parallel at a separation and with each carrying certain electric and magnetic fluxes, and seek to obtain further enhancement of the open string pair production in the aim of its practical use such as its potential detection. Our previous experience indicates that the most efficient and direct way realizing this is to add the additional magnetic fluxes gˆ3 and gˆ3′ in a way as given in (2) and (3). However, on the contrary, it turns out that adding such magnetic fluxes diminishes rather than further enhances the enhanced pair production in the absence of them.This has important implications. It first shows that for each given p≥3 and the same applied electric fluxes fˆ1 and fˆ1′, the largest possible open string pair production is the one when we set gˆ3=gˆ3′=0 in (2) and (3), and keep the magnetic fluxes gˆ2 and gˆ2′ to give the largest possible ν1 in practice. Combining this with the previous results of the enhanced open string pair production in the absence of gˆ3 and gˆ3′, we conclude that the largest pair production is for the p=3 case if we keep the same electric and magnetic fluxes for all allowed p≥3 cases. This is interesting since for p=3, one of D3 branes can be our own 4-dimensional world and this also makes the detection of the pair production a potential reality, an advantage over any other p>3 cases. As discussed recently in [19], from the perspective of a brane observer, the open string pair appears as the charged particle/anti-charged particle one and the dimensions transverse to the brane are the extra-dimensions. So a positive detection of this pair production by the brane observer will indicate the existence of extra-dimensions since the open strings so produced, as mentioned earlier, are those connecting the two D3 branes in the directions transverse to the branes. This will further give a test of the underlying string theories since the computations are stringy ones.AcknowledgementsWe would like to thank Zihao Wu, Li Zhao and Xiaoying Zhu for discussions. The authors acknowledge support by grants from the NSF of China with Grant No. 11775212 and 11235010.References[1]J.X.LuB.NingR.WeiS.S.XuInteraction between two non-threshold bound statesPhys. Rev. D792009126002arXiv:0902.1716 [hep-th][2]J.X.LuS.S.XuThe open string pair-production rate enhancement by a magnetic fluxJ. 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