Production of Magnetic Monopoles via Photon Fusion: Implementation in MadGraph ^†

Abstract

If the Dirac magnetic monopoles exist, they can be probed in the collider experiments. Earlier, only the Drell–Yan production mechanism of magnetic monopoles was used to look for magnetic monopoles. However, the photon fusion production mechanism of magnetic monopoles is the dominant production mechanism at the LHC energy. I will discuss the photon fusion production of spin 0, 1/2, and 1 monopoles using the MadGraph event generator. I will also show the kinematic distributions of magnetic monopoles having those three spins. The comparison between the Drell–Yan process and the photon fusion process will also be done.

1. Introduction

In 1931, Dirac [1] gave a concrete formulation of magnetic monopoles as a quantum mechanical source of magnetic poles. Yet, today, the magnetic monopole remains a hypothetical particle. Dirac conceived of the monopole as a point-like particle. Its spin and mass are not determined by theory.

Since monopoles are yet to be found, many experiments have searched or are searching for this object. Most collider experiments considered only the Drell–Yan (DY) production mechanism of the monopole production in order to search for magnetic monopoles. However, in the collider energy of the LHC, the cross-section for the monopole production mechanism of Photon Fusion (PF) is higher than that of the DY production mechanism [2].

In previous searches for CDF [3], ATLAS [4,5], and MoEDAL [6,7] experiments, different monopole models of the DY production mechanism were simulated using MadGraph  [8,9]. It should be stressed that due to the large coupling constant between the photon and monopole, the perturbative calculation is not possible. Therefore, only tree-level Feynman-like diagrams of DY have been repeatedly used in extracting monopole mass limits in collider experiments.

Since the collider experiments will extend the search for magnetic monopoles using the PF mechanism along with the DY mechanism, it is important that the PF mechanism also be implemented through MadGraph. In this report, a brief description of the implementation of the PF mechanism in MadGraph is given. This report is based on the paper [10] describing the PF MadGraph models.

2. MadGraph Universal FeynRules Output Model

The DY production mechanism was implemented in MadGraph using the Fortran code setup. However, this implementation was inadequate to describe the bosonic monopole production, as it requires a four-particle vertex in the tree level calculation. The PF mechanism was implemented though the Universal FeynRules Output (UFO) model of MadGraph [11].

2.1. Monopole Couplings

In Dirac’s magnetic monopole model, the relation between the elementary electric charge ($q_e$) and the basic magnetic charge (g) is given by:

$$q_e\times g=2\pi n,n\in \mathbb{Z}.$$

(1)

Here, Heaviside–Lorentz units have been used, the convention followed by MadGraph. Hence, from Equation (1), the unit of magnetic charge is:

$$g_D=2\pi /q_e.$$

(2)

In Heaviside–Lorentz units, the electromagnetic vertex is $c_{em}=q_e$. Similarly, in these units, the monopole-photon coupling becomes $c_{mm}=g$. The electric charge is given by $\sqrt{4\pi \alpha }$ where $\alpha$ is the fine structure constant. Then, from Equation (2), one gets:

$$g_D=2\pi /\sqrt{4\pi \alpha }=\sqrt{\pi /\alpha }.$$

(3)

In Equation (3), the monopole velocity $\beta$ has not been used. However, if one considers the photon-monopole coupling to be $\beta$-dependent, then the value of $g_D$ simply becomes $\beta \sqrt{\pi /\alpha }$. The velocity $\beta$ can be found from the Mass (M) of the monopole using the following equation:

$$\beta =\sqrt{1-4M^2/\widehat{s}}$$

(4)

where $\widehat{s}$ is the square of the center-of-mass energy of the colliding particles.

Here, it should be mentioned that the presence of velocity in photon-monopole coupling is debated. If one follows the symmetry argument of the electron and monopole, the photon-monopole coupling should not be velocity dependent as photon-electron coupling is not velocity dependent. However, Milton [12] described the monopole-electron scattering. By comparing the expressions with Rutherford scattering, he found that the photon-monopole coupling is velocity dependent. Here, we follow an agnostic approach, i.e., simulate the production of monopoles with both velocity-dependent and -independent coupling.

2.2. Generation and Validation of the MadGraph UFO Model

The FeynRules interface [13] for the Mathematica package has been used to generate the UFO models. Here, the parameters of a model (i.e., masses of particles, spins, electric charges, magnetic charges, coupling constants, etc.) and the corresponding Lagrangian are written to a text file in a way that Mathematica can understand the variables. FeynRules generates the UFO model from that text file.

The $\beta$ is defined as a form factor to the coupling [14]. The value of $\widehat{s}$ has been obtained from the following equation:

$$\widehat{s}=2(P_1·P_2).$$

(5)

Here, $P_1$ and $P_2$ are the four-momentum of the two colliding particles.

To generate the UFO model, one needs to feed the Lagrangian to the FeynRules. Therefore, the UFO model for the scalar monopole was generated by using this Lagrangian [10]:

$${\mathcal{L}}^{S=0}=-\frac{1}{4}{F}_{\mu \nu }{F}^{\mu \nu }+(\partial -ig\left(\beta \right){\mathcal{A}}_{\mu }){\varphi }^{†}(\partial +ig\left(\beta \right){\mathcal{A}}_{\mu })\varphi -M^2{\varphi }^{†}\varphi$$

(6)

where ${\mathcal{A}}_{\mu }$ is the photon field, whose field strength tensor is given by $F_{\mu \nu }={\partial }_{\mu }{\mathcal{A}}_{\nu }-{\partial }_{\nu }{\mathcal{A}}_{\mu }$ and $\varphi$ is the scalar monopole field. Here, $g\left(\beta \right)$ is simply g for $\beta$-independent photon-monopole coupling and for $\beta$-dependent coupling, $g\left(\beta \right)$ is $g\beta$.

Once generated, the UFO model needs to be validated. This was done by comparing the cross-sections from the theoretical predictions and the cross-sections obtained from MadGraph, when no Parton Distribution Function (PDF)was used. The Feynman diagrams from the spin 0 UFO model is shown in Figure 1. The cross-section values for the $\beta$-independent coupling are shown in

Table 1. The cross-section for the spin 0 monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-independent coupling when no PDF is used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of the UFO model to that of the theoretical prediction. These ratios are very close to 1, suggesting excellent agreement between the theory and the MadGraph model [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory
1000	$1.518\times {10}^4$	$1.5039\times {10}^4$	$1.009$
2000	$1.202\times {10}^4$	$1.1945\times {10}^4$	$1.006$
3000	9218	$9108.09$	$1.012$
4000	7366	$7218.79$	$1.020$
5000	6558	$6519.68$	$1.006$
6000	5378	$5325.76$	$1.010$

.

In a similar fashion, the $\beta$-dependent coupling model was compared with the theory. The cross-section values are compared in

Table 2. The cross-section for the spin 0 monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-dependent coupling constant, when no PDF is used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of the UFO model to that of the theoretical prediction. These ratios are very close to 1, suggesting excellent agreement between the theory and the MadGraph model. Here, the sixth column shows the ratio of cross-sections as obtained by the UFO model for $\beta$-dependent coupling to $\beta$-independent coupling (shown in Table 1). This ratio varies as ${\beta }^4$, as expected from the theory [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory	$\mathit{\beta }$	Ratio $\mathit{\beta }$-dep/$\mathit{\beta }$-ind (UFO Model)
1000	$1.4493\times {10}^4$	$1.4336\times {10}^4$	$0.99$	0.9881	0.9547 (~$0.{9881}^4$)
2000	$9.851\times {10}^3$	$9.791\times {10}^3$	$1.006$	0.9515	0.8196 (~$0.{9515}^4$)
3000	$5.685\times {10}^3$	$5.640\times {10}^3$	$1.007$	0.8871	0.6167 (~$0.{8871}^4$)
4000	2847	$2810.5$	$1.013$	0.7882	0.3866 (~$0.{7882}^4$)
5000	1094	1087	$1.006$	0.639	0.1658 (~$0.{639}^4$)
6000	$117.8$	$116.53$	$1.011$	0.3846	0.022 (~$0.{3846}^4$)

. The ratio of cross-sections for the $\beta$-dependent coupling to the $\beta$-independent coupling should be of the order of ${\beta }^4$. This was confirmed in the sixth column of Table 2.

Similarly, the spin ½ monopole model was validated by comparing the cross-sections with the theoretical predictions with no PDF and the center-of-mass energy of 13 TeV. Here, the Lagrangian is in the following equation [10]:

$${\mathcal{L}}^{S=1/2}=-\frac{1}{4}{F}_{\mu \nu }{F}^{\mu \nu }+\overline{\psi }(i\cancel{D}-m)\psi -i\frac{1}{4}g\left(\beta \right)\kappa F_{\mu \nu }\overline{\psi }[{\gamma }^{\mu },{\gamma }^{\nu }]\psi ,$$

(7)

where $F_{\mu \nu }$ is the electromagnetic field tensor, $\cancel{D}={\gamma }^{\mu }({\partial }_{\mu }-ig\left(\beta \right){\mathcal{A}}_{\mu })$ is the total derivative, and a commutator of the $\gamma$ matrices is given by $[{\gamma }^{\mu },{\gamma }^{\nu }]$. The last term in the above Lagrangian is a magnetic moment-generating term [10]. Unless otherwise stated, the value of $\kappa$ for spin ½ monopoles is taken to be zero. The diagrams considered for spin ½ are shown in Figure 2.

The cross-sections comparisons are shown in

Table 3. The cross-section for the spin ½ monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-independent coupling when no PDF is used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of the UFO model to that of the theoretical prediction. As the ratios are very close to 1, this suggests excellent agreement between the theory and the MadGraph model [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory
1000	$1.431\times {10}^5$	$1.425\times {10}^5$	$1.004$
2000	$1.018\times {10}^5$	$1.007\times {10}^5$	$1.010$
3000	$7.755\times {10}^4$	$7.679\times {10}^4$	$1.010$
4000	$5.830\times {10}^4$	$5.7404\times {10}^4$	$1.016$
5000	$3.817\times {10}^4$	$3.797\times {10}^4$	$1.005$
6000	$1.691\times {10}^4$	$1.6705\times {10}^4$	$1.012$

(for $\beta$-independent coupling) and

Table 4. The cross-section for the spin ½ monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-dependent coupling constant, when no PDF is used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of the UFO model to that of the theoretical prediction. As these ratios are very close to 1, they suggest excellent agreement between the theory and the MadGraph model. Here, the sixth column shows the ratio of cross-sections as obtained by the UFO model for $\beta$-dependent coupling to $\beta$-independent coupling (shown in Table 3). This ratio varies as ${\beta }^4$, as expected from the theory [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory	$\mathit{\beta }$	Ratio $\mathit{\beta }$-dep/$\mathit{\beta }$-ind (UFO Model)
1000	$1.364\times {10}^5$	$1.358\times {10}^5$	$1.004$	0.9881	0.9531 (~$0.{9881}^4$)
2000	$8.341\times {10}^4$	$8.2551\times {10}^4$	$1.010$	0.9515	0.8193 (~$0.{9515}^4$)
3000	$4.803\times {10}^4$	$4.7554\times {10}^4$	$1.010$	0.8871	0.6193 (~$0.{8871}^4$)
4000	$2.251\times {10}^4$	$2.2156\times {10}^4$	$1.012$	0.7882	0.3861 (~$0.{7882}^4$)
5000	6362	6331	$1.005$	0.639	0.1667 (~$0.{639}^4$)
6000	370	$365.5$	$1.012$	0.3846	0.0219 (~$0.{3846}^4$)

(for $\beta$-dependent coupling). The ratios of the cross-sections of the UFO model and the theoretical predictions are very close to one. This means that the spin ½ UFO model is also well-modeled.

The cross-section ratios for $\beta$-dependent coupling to $\beta$-independent coupling are also shown in Table 4. These ratios are very close to ${\beta }^4$, suggesting that the $\beta$-dependence in the coupling has been well-modeled, as well.

After the spin 0 and spin ½ monopole models, we look at the spin 1 magnetic monopole scenario. Here, the Lagrangian is given by the following equation [10]:

$${\mathcal{L}}^{S=1}=-\frac{1}{2}\left(\frac{\partial {\mathcal{A}}_{\mu }}{\partial x_{\nu }}\right)\left(\frac{\partial {\mathcal{A}}_{\nu }}{\partial x_{\mu }}\right)-\frac{1}{2}{G}_{\mu \nu }^{†}{G}_{\mu \nu }-M^2{W}_{\mu }^{†}{W}^{\mu }-ig\left(\beta \right)\kappa F_{\mu \nu }{W}_{\mu }^{†}{W}_{\nu }.$$

(8)

Here, the tensor $F_{\mu \nu }$ represents the Abelian electromagnetic field strength. The $G^{\mu \nu }$ is $(D^{\mu }{W}^{\nu }-D^{\nu }{W}^{\mu })$ with $D_{\mu }={\partial }_{\mu }-ig\left(\beta \right){\mathcal{A}}_{\mu }$, the covariant derivative of $U\left(1\right)$, providing the coupling of the magnetically-charged vector field $W^{\mu }$ to the gauge field ${\mathcal{A}}_{\mu }$. This plays the role of the ordinary photon. The last term is the magnetic moment term, proportional to $\kappa$, to keep the discussion general [10]. Unless otherwise stated, the default value of $\kappa$ for the spin 1 monopole is taken to be one.

The Feynman diagrams as generated by MadGraph for the spin 1 magnetic monopole model is shown in Figure 3. Just like the spin 0 and spin ½ magnetic monopole models, we compare the cross-sections obtained by spin 1 UFO model with the predictions from the theory. The comparisons are shown in

Table 5. The cross-section for the spin 1 monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-independent coupling when no PDF is used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of the UFO model to that of the theoretical prediction. The ratios, being very close to 1, suggest excellent agreement between the theory and the MadGraph model [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory
1000	$1.131\times {10}^7$	$1.131\times {10}^7$	$1.000$
2000	$2.765\times {10}^6$	$2.747\times {10}^6$	$1.007$
3000	$1.164\times {10}^6$	$1.151\times {10}^6$	$1.011$
4000	$5.879\times {10}^5$	$5.835\times {10}^5$	$1.008$
5000	$3.161\times {10}^5$	$3.109\times {10}^5$	$1.017$
6000	$1.39\times {10}^5$	$1.378\times {10}^5$	$1.009$

(for $\beta$-independent coupling) and

Table 6. The cross-section for the spin 1 monopole as obtained by the theory and the MadGraph UFO model for the $\beta$-dependent coupling constant, when no PDF was used and the center-of-mass energy is 13 TeV. The fourth column shows the ratio of the cross-sections of UFO model to that of the theoretical prediction. The ratios, being very close to 1, suggest excellent agreement between the theory and the MadGraph model. Here, the sixth column shows the ratio of cross-sections as obtained by the UFO model for $\beta$-dependent coupling to $\beta$-independent coupling (shown in Table 5). This ratio varies as ${\beta }^4$, as expected from the theory [10].

Mass (GeV)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (UFO Model)	$\mathit{\sigma }$ (pb) $\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-}$ (Theory Values)	Ratio UFO Model/Theory	$\mathit{\beta }$	Ratio $\mathit{\beta }$-dep/$\mathit{\beta }$-ind (UFO Model)
1000	$1.078\times {10}^7$	$1.0781\times {10}^7$	$0.999$	0.9881	0.9531 (~$0.{9881}^4$)
2000	$2.277\times {10}^6$	$2.2520\times {10}^6$	$1.011$	0.9515	0.8235 (~$0.{9515}^4$)
3000	$7.214\times {10}^5$	$7.1290\times {10}^5$	$1.012$	0.8871	0.6198 (~$0.{8871}^4$)
4000	$2.275\times {10}^5$	$2.2523\times {10}^5$	$1.010$	0.7882	0.3870 (~$0.{7882}^4$)
5000	$5.256\times {10}^4$	$5.1833\times {10}^4$	$1.014$	0.639	0.1663 (~$0.{639}^4$)
6000	$3.034\times {10}^3$	$3.014\times {10}^3$	$1.007$	0.3846	0.0218 (~$0.{3846}^4$)

(for $\beta$-dependent coupling). This was done with no PDF and a center-of-mass energy of 13 TeV. The tables show that the cross-sections obtained by the spin 1 magnetic monopole UFO model are in excellent agreement with the theoretical predictions for both the $\beta$-independent and $\beta$-dependent coupling cases.

2.3. LHC Phenomenology

After we validate the MadGraph UFO model, we need to look at the kinematic and angular distributions of PF process and compare them with the DY process. This is an important aspect for the monopole searches at the collider experiments as the geometrical acceptance and efficiency of a detector is not uniform in the solid angle around the interaction point.

2.3.1. Kinematic Distributions

Since the monopole search results in the collider experiments have been interpreted using the DY production process, we need to compare the kinematic and angular distributions of DY and PF processes and identify the differences. In order to compare the kinematic and angular distributions of the PF and DY method, PDFs were used to get meaningful distributions. For the DY method, the PDF was set to NNPDF23 at lowest order (LO)  [15]. For the PF method, LUXqed [16] was used. This was done as LUXqed provides a relatively small uncertainty in the photon distribution function of the proton [17]. For spin ½ plots, the value of the $\kappa$ parameter was taken to be zero, and for spin 1 plots, the value of the $\kappa$ parameter was taken to be one.

The kinetic energy distribution comparison between PF and DY processes is shown in Figure 4. The pseudorapidity distribution ($\eta$) comparison is shown in Figure 5.

2.3.2. Limiting Case of Large $\kappa$ and Small $\beta$ for Photon Fusion

In this section, we want to see the cross-section and kinematic distributions of the PF process for the large $\kappa$ and small $\beta$ scenario for the spin ½ and 1 monopole cases. If the cross-section is finite at this limit, then this may open a way to potential perturbatively-consistent search in colliders.

a. Spin ½ monopole scenario: A magnetic moment-generating term $\kappa$ has been added to the Lagrangian of the spin ½ monopole case (Equation (7)). A dimensionless parameter $\tilde{\kappa }=\kappa M$ with M being the mass of the monopole has been varied from 0–10,000 for the photon fusion process with a photon-photon collision energy of 13 TeV. The cross-section for $\tilde{\kappa }=0$ (the Standard Model scenario) goes to zero at $\beta \to 0$ very fast, as can be seen from the third column of

Table 7. Photon fusion production cross-sections at a photon-photon collision energy of 13 TeV for the spin ½ monopole, $\beta$-dependent coupling, and various values of the $\tilde{\kappa }$ parameter [10].

Monopole	$\mathit{\beta }$	$\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-},\mathit{\sigma }\left(\mathbf{pb}\right)$
Mass (GeV)		$\tilde{\mathit{\kappa }}=0$	$\tilde{\mathit{\kappa }}=10$	$\tilde{\mathit{\kappa }}=100$	$\tilde{\mathit{\kappa }}=10,000$
1000	0.9881	$1.37\times {10}^5\pm 4.6\times {10}^2$	$1.639\times {10}^{24}\pm 3.3\times {10}^{21}$	$1.639\times {10}^{28}\pm 3.3\times {10}^{25}$	$1.639\times {10}^{36}\pm 3.3\times {10}^{33}$
2000	0.9515	$8.303\times {10}^4\pm 4.5\times {10}^2$	$1.61\times {10}^{24}\pm 3.1\times {10}^{21}$	$1.61\times {10}^{28}\pm 3.1\times {10}^{25}$	$1.61\times {10}^{36}\pm 3.1\times {10}^{33}$
3000	0.8871	$4.78\times {10}^4\pm 3.5\times {10}^2$	$1.356\times {10}^{24}\pm 2.5\times {10}^{21}$	$1.356\times {10}^{28}\pm 2.5\times {10}^{25}$	$1.356\times {10}^{36}\pm 2.5\times {10}^{33}$
4000	0.7882	$2.237\times {10}^4\pm 1.9\times {10}^2$	$8.612\times {10}^{23}\pm 2.1\times {10}^{21}$	$8.613\times {10}^{27}\pm 2.1\times {10}^{25}$	$8.613\times {10}^{35}\pm 2.1\times {10}^{33}$
5000	0.639	$6396\pm 61$	$3.154\times {10}^{23}\pm 1.1\times {10}^{21}$	$3.154\times {10}^{27}\pm 1.1\times {10}^{25}$	$3.154\times {10}^{35}\pm 1.1\times {10}^{33}$
5500	0.5329	$2256\pm 22$	$1.247\times {10}^{23}\pm 4.5\times {10}^{20}$	$1.247\times {10}^{27}\pm 4.5\times {10}^{24}$	$1.247\times {10}^{35}\pm 4.5\times {10}^{32}$
5800	0.4514	$886.5\pm 7.8$	$5.28\times {10}^{22}\pm 2.5\times {10}^{20}$	$5.28\times {10}^{26}\pm 2.5\times {10}^{24}$	$5.28\times {10}^{34}\pm 2.5\times {10}^{32}$
6000	0.3846	$367.2\pm 3$	$2.294\times {10}^{22}\pm 7.6\times {10}^{19}$	$2.294\times {10}^{26}\pm 7.6\times {10}^{23}$	$2.294\times {10}^{34}\pm 7.6\times {10}^{31}$
6200	0.3003	$97.19\pm 0.77$	$6.43\times {10}^{21}\pm 3.3\times {10}^{19}$	$6.43\times {10}^{25}\pm 3.3\times {10}^{23}$	$6.43\times {10}^{33}\pm 3.3\times {10}^{31}$
6400	0.1747	$5.846\pm 0.025$	$4.065\times {10}^{20}\pm 1.5\times {10}^{18}$	$4.065\times {10}^{24}\pm 1.5\times {10}^{22}$	$4.065\times {10}^{32}\pm 1.5\times {10}^{30}$
6490	$0.0554$	$0.017\pm 2.27\times {10}^{-5}$	$1.27\times {10}^{18}\pm 8.74\times {10}^{14}$	$1.27\times {10}^{22}\pm 8.74\times {10}^{18}$	$1.27\times {10}^{30}\pm 8.74\times {10}^{26}$

. However, for the non-zero $\tilde{\kappa }$, the cross-section values remain finite, even if the $\beta$ goes to zero. The same conclusion can be obtained from the left plot of Figure 6, where the cross-section has been plotted against the monopole mass for the proton-proton collision energy of 13 TeV.

The central and right-hand side plots of Figure 6 show the transverse momentum distribution and pseudorapidity distribution for different $\tilde{\kappa }$ scenarios. Here, $\tilde{\kappa }=0$ shows the Standard Model case. The $p_T$ spectrum is harder than the Standard Model case when $\tilde{\kappa }\ne 0$. The pseudorapidity distribution is more central for $\tilde{\kappa }\ne 0$ than the Standard Model case of $\tilde{\kappa }=0$.

b. Spin 1 monopole scenario: Similar to the spin ½ monopole scenario, the spin 1 monopole also has a magnetic moment term in the Lagrangian (Equation (8)). For the spin 1 monopole, $\kappa =1$ is the Standard Model case. Here, the cross-section for the $\kappa =1$ case goes to zero very fast as $\beta$ goes to zero (as seen from the third column of

Table 8. Photon fusion production cross-sections at a photon-photon collision energy of 13 TeV for the spin 1 monopole, $\beta$-dependent coupling, and various values of the $\kappa$ parameter [10].

Monopole Mass (GeV)	$\mathit{\beta }$	$\mathit{\gamma }\mathit{\gamma }\to {\mathbf{mm}}^{+}{\mathbf{mm}}^{-},\mathit{\sigma }\left(\mathbf{pb}\right)$
		$\mathbf{\kappa }=\mathbf{1}$	$\mathbf{\kappa }=\mathbf{100}$	$\mathbf{\kappa }=\mathbf{10},\mathbf{000}$
1000	0.9881	$1.086\times {10}^7\pm 1.4\times {10}^5$	$4.939\times {10}^{15}\pm 1\times {10}^{13}$	$5.033\times {10}^{23}\pm 2.1\times {10}^{21}$
2000	0.9515	$2.275\times {10}^6\pm 1.6\times {10}^4$	$2.844\times {10}^{14}\pm 4.9\times {10}^{11}$	$2.879\times {10}^{22}\pm 9.8\times {10}^{19}$
3000	0.8871	$7.198\times {10}^5\pm 6.6\times {10}^3$	$4.518\times {10}^{13}\pm 1.5\times {10}^{11}$	$4.536\times {10}^{21}\pm 1.2\times {10}^{19}$
4000	0.7882	$2.273\times {10}^5\pm 2.2\times {10}^3$	$9.079\times {10}^{12}\pm 2.7\times {10}^{10}$	$9.002\times {10}^{20}\pm 3.2\times {10}^{18}$
5000	0.639	$5.232\times {10}^4\pm 4.9\times {10}^2$	$1.513\times {10}^{12}\pm 9.2\times {10}^9$	$1.5\times {10}^{20}\pm 9.3\times {10}^{17}$
5500	0.5329	$1.785\times {10}^4\pm 1.6\times {10}^2$	$4.49\times {10}^{11}\pm 1.7\times {10}^9$	$4.466\times {10}^{19}\pm 2.9\times {10}^{17}$
5800	0.4514	$7118\pm 62$	$1.658\times {10}^{11}\pm 1.1\times {10}^9$	$1.624\times {10}^{19}\pm 8.4\times {10}^{16}$
6000	0.3846	$3025\pm 24$	$6.72\times {10}^{10}\pm 2.5\times {10}^8$	$6.627\times {10}^{18}\pm 3.7\times {10}^{16}$
6200	0.3003	$836.9\pm 6.3$	$1.764\times {10}^{10}\pm 1\times {10}^8$	$1.733\times {10}^{18}\pm 1\times {10}^{16}$
6400	0.1747	$53.42\pm 0.23$	$1.066\times {10}^9\pm 3.9\times {10}^6$	$1.05\times {10}^{17}\pm 3.8\times {10}^{14}$
6490	$0.0554$	$0.1694\pm 0.00065$	$3.293\times {10}^6\pm 5.6\times {10}^3$	$3.244\times {10}^{14}\pm 5.6\times {10}^{11}$

) at a photon-photon collision energy of 13 TeV. However, when $\kappa >1$, the cross-section remains finite as $\beta$ goes to zero. A similar conclusion can be drawn from the cross-section vs. monopole mass plot of Figure 7 (left), where the proton-proton collision energy of 13 TeV has been used.

The transverse momentum distribution and the pseudorapidity distribution have been compared for different values of $\kappa$ for the spin 1 monopole case at the proton-proton collision energy of 13 TeV and are shown in the central and right plots of Figure 7. Here, similar to the spin ½ scenario, models with $\kappa >1$ values yield a $p_T$ spectrum harder than the Standard Model scenario when $\kappa =1$. The pseudorapidity distribution is more central for $\kappa \ne 1$ than the Standard Model case of $\kappa =1$.

3. Conclusions

In this report, an overview of the phenomenological study of magnetic monopoles with the help of MadGraph models is given. In the first part, the details of the generation of MadGraph UFO models were described. Subsequently, those models were successfully validated by checking the cross-section values given by the models against the theoretical predictions.

In the second part, the LHC phenomenology of these models was described. The kinetic energy and pseudorapidity distribution comparisons between the DY method and PF method have been shown. Furthermore, a potential perturbative limit was given when $\kappa$ was high, but monopole velocity $\beta$ was very low. In that limit, the cross-sections for the spin ½ and spin 1 monopoles were finite. This proceeding also showed the kinetic and pseudorapidity distribution comparisons for different $\kappa$ values for the spin ½ and spin 1 monopoles.

The UFO models can be used by the collider experiments to simulate the photon fusion production mechanism of magnetic monopoles. The MoEDAL experiment at the LHC is using these models to interpret its latest data. The MoEDAL paper is in preparation.