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Constraining exotic spin dependent interactions of muons and electrons

  • H. YanEmail author
  • G. A. Sun
  • S. M. Peng
  • H. Guo
  • B. Q. Liu
  • M. Peng
  • H. Zheng
Open Access
Letter

Abstract

Many experiments have been performed to search for the exotic spin-dependent interactions in ranges from \(\sim \upmu \)m to astrophysical range which corresponds to the energy scale of less than \(\sim \)10 eV. At present, nearly all known experiments searching for these new interactions at the macroscopic range are for protons, neutrons, and electrons. Constraints at this range for other fermions such as muons are scarce, though muons might be the most suspicious particles which might take part in new interactions, considering their involvement of several well-known puzzles of modern physics. We use the anomalous magnetic moment and electric dipole moment (EDM) to study the exotic spin-dependent interactions for muons and electrons. The muon’s magnetic moment might indicate existing of the pseudo-scalar–pseudo-scalar (PP) type interaction. We set up a constraint for the scalar–pseudo-scalar (SP) type interaction at the interested range for muons. For the PP type interaction of electrons, we obtained a new constraint at the range of \(\sim \) nm to \(\sim \) 1 mm. Since all the present experiments searching for the new forces give zero results, it is reasonable to consider that these new interactions might only couple to muons. We propose to further search for the new interactions using the muon spin rotation techniques.

1 Introduction

New interactions beyond the Standard Model are possible. Suggested solutions for several important problems of modern physics have led to new interactions mediated by new particles [1]. Exotic macroscopic forces mediated by WISPs (weakly-interacting slim particles) is an example. Reference [2] classified the new interactions into 16 different types and most of them are spin dependent. These new interactions have ranges from nanometers to astronomical distance which corresponds to the mediating-boson mass of \(\sim 10^{-18}\) eV to \(\sim 100\) eV. Methods of precision measurement such as the torsion pendulum [3], co-magnetometer of polarized noble gases [4, 5], SERF magnetometer [6], polarized \(^3\)He atom beam [7], etc are convenient to probe these new interactions at a much lower energy scale than the high energy physics.

According to Refs. [2, 8], new interactions between fermions can be induced via the coupling:
$$\begin{aligned} {\mathcal {L}}_{I}={\bar{\psi }}(g_{s}+ig_{p}\gamma _{5})\psi \phi . \end{aligned}$$
(1)
\(\phi \) which mediates the new interaction, is the ALP (Axion-Like Particle). To probe the new force is equivalent to detect the ALP which leads to solutions of some very important problems in modern physics. On one hand, axions are possible candidates for the dark matter which remains to be one of the most important unsolved problems in both particle physics and astrophysics [1, 9]. On the other hand, axions have attracted a lot of attention in high energy physics since they probably provide the most promising solution to preserve the CP-symmetry in strong interactions [10].
Due to \({\mathcal {L}}_I\), there could be the monopole–monopole, dipole–dipole and monopole–dipole interactions, originated from the SS (Scalar–Scalar) , PP (Pseudo-scalar–Pseudo-scalar) and SP (Scalar–Pseudo-scalar) coupling respectively and the last two are spin dependent. The SP interaction or the monopole–dipole interaction has attracted much scientific interest recently. At low energy, the interaction between polarized and unpolarized fermions can be expressed as the potential [2, 8]:
$$\begin{aligned} V_{SP}(r)=\frac{\hbar ^{2}g_{S}g_{P}}{8\pi m_1}\left( \frac{1}{\lambda r}+\frac{1}{r^{2}}\right) \exp {(-r/\lambda )}\vec {\sigma }\cdot {\hat{r}} \end{aligned}$$
(2)
where \(\lambda =\hbar /m_{\phi }c\) is the interaction range, \(m_{\phi }\) the mass of the new scalar boson, \(\vec {s}=\hbar \vec {\sigma }/2\) the spin of the polarized fermion, \(m_1\) the mass of the polarized fermion and r the distance between the interacting particles. The spin–spin dependent potential induced by the PP interaction is:
$$\begin{aligned} V_{PP}(r)= & {} \frac{\hbar ^{3}g_{P}g_{P}}{16\pi c m_1m_2}\left[ \left( \frac{1}{\lambda r^2}+\frac{1}{r^{3}}\right) \vec {\sigma }_1\cdot \vec {\sigma }_2\right. \\&\left. -\left( \frac{1}{\lambda ^2 r}+\frac{3}{\lambda r^{2}}+\frac{1}{r^{3}}\right) (\vec {\sigma }_1\cdot {\hat{r}})(\vec {\sigma }_2\cdot {\hat{r}})\right] \\&\times \exp {(-r/\lambda )} \end{aligned}$$
In order to detect \(V_{SP}\), either the source or the probe fermion has to be spin polarized. While to search for \(V_{PP}\), both particles need to be polarized. Furthermore, the source and probe fermion have to be close enough which is limited by the force range \(\lambda \). Recently, various experiments have been performed or proposed to search for these new interactions which could couple to the spin of the neutron/electron [3, 4, 5, 6, 7, 11, 12, 13, 14, 15, 16, 17, 18]. However, studies of these long-range, spin-dependent new interactions for other fermions are scarce. Muons are probably the most suspicious fermion which new interactions might be involved. The charge radius puzzles of the muonic hydrogen [19] and deuteron [20] nucleus are well-known examples [21, 22]. Although parity-violating muonic forces mediated by new massive gauge bosons of MeV–GeV have been proposed to solve the proton charge radius puzzle, to our best knowledge, no studies have been conducted to search for these new interactions in ranges greater than \(\sim \) nm which corresponds to a mass scale of less than \(\sim 100\) eV yet.

In this work, we discuss the possibility that the anomalous magnetic moment of the muon might indicate existing of the new SS or PP interaction mediated by ALPs lighter than \(\sim 100\) eV. By using the muon’s EDM (Electric Dipole Moment), we could establish a constraint for the parity-violating monopole–dipole interaction mediated by ALPs lighter than \(\sim 100\) eV for muons. When applying the method to the electrons, constraints of \(g_S^{e}g_S^{e}\) and \(g_P^{e}g_P^{e}\) are obtained for the range between \(\sim \)1 and \(\sim \)1 mm.

2 The anomalous magnetic moment and EDM induced by new interactions

The leading order contribution to the electromagnetic vertex from the new interactions is shown in Fig. 1. The new boson line could induce SS, SP and PP type vertexes.
Fig. 1

The electromagnetic vertex correction contributed by new interactions

The new interactions, if exist, would not only change the anomalous magnetic moment of the fundamental fermion but also induce the EDM which has been measured for many particles [1]. According to Refs. [23, 24, 25], the general formula corresponding to the Feynman diagram shown in Fig. 1 can be expressed as:
$$\begin{aligned}&{\bar{u}}(p')\Lambda ^\mu u(p) \\&\quad = {\bar{u}}(p')\left[ \gamma ^\mu F_1(q^2)+i\frac{\sigma ^{\mu \nu }q_\nu }{2m}F_2(q^2)\right. \\&\qquad \left. +\gamma ^5\frac{\sigma ^{\mu \nu }q_\nu }{2m}F_3(q^2)+\gamma ^5(q^2\gamma ^\mu -2m\gamma ^5q^\mu )F_4(q^2)\right] u(p) \end{aligned}$$
where \(q=p'-p\). Here \(eF_1(0)\) gives the renormalized charge, and \(F_4(0)\) which is called the anapole moment [25], is the possible axial current induced by the new interactions which do not necessarily conserve the parity. These two terms are irrelevant to this work. e\(F_2(0)\)/2m is the anomalous magnetic moment, and \(-\)e\(F_3(0)\)/2m the EDM.
Using the well known Gordon decomposition formula and techniques presented in Ref. [26], one can derive the anomalous magnetic moment induced by the SS and PP interaction as [27]
$$\begin{aligned} F_2(0)= & {} -\frac{g_Sg_S}{8\pi ^2}SS(x) \end{aligned}$$
(3)
$$\begin{aligned} F_2(0)= & {} -\frac{g_Pg_P}{8\pi ^2}PP(x) \end{aligned}$$
(4)
where SS(x) and PP(x) are defined as:
$$\begin{aligned} SS(x)= & {} \frac{3}{2}-x^2+x^2(x^2-3)\ln {x}+x(x^2-1)\sqrt{x^2-4}\\&\times \left[ \tanh ^{-1}{\left( \frac{x}{\sqrt{x^2-4}}\right) }-\tanh ^{-1}{\left( \frac{x^2-2}{x\sqrt{x^2-4}}\right) }\right] \\ PP(x)= & {} \frac{1}{2}+x^2-x^2(x^2-1)\ln {x}+\frac{x^3(3-x^2)}{\sqrt{x^2-4}}\\&\times \left[ \tanh ^{-1}{\left( \frac{x}{\sqrt{x^2-4}}\right) }-\tanh ^{-1}{\left( \frac{x^2-2}{x\sqrt{x^2-4}}\right) }\right] . \end{aligned}$$
with \(x={m_{\phi }}/{m}\).
EDM can be induced by the possible new interactions. In this case, implementing similar techniques as before, for the SP type new interaction, we obtain [27]
$$\begin{aligned} F_3(0)=\frac{g_Sg_P}{4\pi ^2}SP(x) \end{aligned}$$
(5)
where
$$\begin{aligned} SP(x)= & {} 1-x^2\ln {x}-\frac{x(x^2-2)}{\sqrt{x^2-4}}\\&\times \left[ \tanh ^{-1}{\left( \frac{x}{\sqrt{x^2-4}}\right) }-\tanh ^{-1}\left( \frac{x^2-2}{x\sqrt{x^2-4}}\right) \right] . \end{aligned}$$

3 Applications to the muon and electron

There is a \(\sim 3.7\sigma \) [1, 28, 29] difference between the experimental measurement and the theoretical prediction from the Standard Model for the anomalous magnetic moment \(a_\mu \) of the muon. According to Ref. [30], this difference is explicitly given by
$$\begin{aligned} a_\mu ^{exp}-a_\mu ^{SM}=2.74\pm 0.73\times 10^{-9} \end{aligned}$$
(6)
where \(a_\mu ^{exp}\) is the experimentally measured value and \(a_\mu ^{SM}\) the Standard Model prediction. If the contribution from the long-range new interaction of \(V_{PP}\) is considered, then the difference might be explained as a nonzero \(g_{S}^{\mu }g_{S}^{\mu }\) or \(g_{P}^{\mu }g_{P}^{\mu }\) of:
$$\begin{aligned}&|g_{S}^{\mu }g_{S}^{\mu }|=1.44\pm 0.38\times 10^{-7}, \end{aligned}$$
(7)
$$\begin{aligned}&|g_{P}^{\mu }g_{P}^{\mu }|=4.32\pm 1.16\times 10^{-7}, \end{aligned}$$
(8)
with \(m_\phi<\)100 eV(\(\lambda>\)1nm).
Plugging in the best known muon EDM [31],
$$\begin{aligned} |d_\mu |<1.8\times 10^{-19}e.cm,95\% C.L. \end{aligned}$$
(9)
a constraint for \(g_S^{\mu }g_P^{\mu }\) can be established as shown in Fig. 2. It is interesting to notice that \(g_P^{\mu }g_P^{\mu }\) is not zero while \(g_S^{\mu }g_P^{\mu }\) is, all at a \(\sim 10^{-7}\) level.
Fig. 2

A constraint to the coupling constant product \(|g_S^{\mu }g_P^{\mu }|\) as a function of the interaction range \(\lambda \) (ALP mass). The (red) dashed line is the result of this work for the muon. The dark grey area is excluded from this work

Fig. 3

Constraints to the coupling constant product \(|g_S^{e}g_S^{e}|\) a function of the interaction range \(\lambda \) (ALP mass). The (red) dashed line is the result of this work

Fig. 4

Constraints to the coupling constant product \(|g_S^{e}g_P^{e}|\) a function of the interaction range \(\lambda \) (ALP mass). The (red) dashed line is the result of this work. The (blue) solid line is the result of Ref. [3]. The dark grey area is excluded by this work and grey area is excluded by Ref. [3]

We also apply this method to the electron. Theoretically, the anomalous magnetic moment and EDM of the electron can be predicted by the Standard Model [32, 33, 34]. Combined with the best known experimental measurement given in Ref. [35], the possible contributions due to new physics beyond the standard model are
$$\begin{aligned}&|a_e^{exp}-a_e^{SM}|<2.66\times 10^{-12}, 95\% C.L. \end{aligned}$$
(10)
$$\begin{aligned}&|d_e|<1.2\times 10^{-29}e.cm, 95\% C.L. \end{aligned}$$
(11)
Fig. 5

Schematic of the experimental setup to probe the new spin-dependent interactions for muons. The incoming muon beam which is spin-polarized triggers the clock which defines time zero. A sample is placed close to the muon beam and its polarization can be rotated if new spin-dependent interactions exist. The rotation angle of the muon polarization can be measured from the positron counter

By using the anomalous magnetic moment, constraints of \(|g_S^{e}g_S^{e}|\) and \(|g_P^eg_P^e|\) for electrons can be established as shown in Figs. 3 and 4, respectively. One can see that this method could derive a new constraint for \(V_{PP}\) in the range between \(\sim \)nm to \(\sim \)mm. When using the electron EDM, the derived constraint for \(g_S^eg_P^e\) at the interested force range is at a level of \(\sim 10^{-17}\). It gives a constraint \(\sim \)3 orders more stringent than a recent experimental work [36] in the range near \(\sim \mu \)m. At long interaction ranges(\(m_\phi <\sim \) keV), using data from atomic and molecular EDM experiments [37], Ref. [38] gives a constraint on \(g_S^eg_P^e\) \(\sim \)3 times more stringent than this work. At very short ranges(\(m_\phi >\sim \)MeV), the loop induced EDM dominates thus the method presented in this work might work better [39]. For the new boson heavier than \(\sim \)MeV, it is more convenient to be detected by the method of high energy physics and obviously out of the scope of this work.

4 Conclusion and discussion

The 3.7\(\sigma \) difference between the theoretical prediction and the experimental measurement of the anomalous magnetic moment of muons might indicate nonzero new interactions of SS or PP type with a range larger than \(\sim \)1 nm. We constrain the monopole–dipole type interaction (originated from the SP) for muons, as shown in Fig. 2. Previously, many experiments and studies have been performed for spin-dependent new interactions associated with electrons, protons, and neutrons only. Although short-range muonic forces with an energy scale larger than \(\sim \) MeV have been proposed to solve the proton radius puzzle, studies considering macroscopic range muonic interactions mediated by ALPs have not been conducted yet, according to our best knowledge. The charge radius puzzles of the muonic hydrogen and deuteron and the anomalous magnetic moment of muons suggest that new physics or new interactions might exist for muons.

It would be fascinating to include muons into the searching business for the macroscopic new spin dependent interactions which are mediated by ALPs or other new light bosons. Low energy muon beams with 100% polarization are frequently used in condensed matter physics [40] and fundamental physics [29]. If a nonmagnetic mass-source can be put in the region close to muon beams as in Fig. 5 [7], constraints on \(g_Sg_P^\mu \) at long distances can be obtained by measuring changes of the muon polarization. Furthermore, if polarized electron spin-density sources, as the \(\mu \)-metal shielded \(\hbox {SmCo}_5\) [3, 41], are used in experiments, then constraints on \(g_P^eg_P^\mu \) can be established. It is not hard to imagine that the muonic new interactions mediated by light vector particles can also be searched for using experimental schemes as in Ref. [7].

Using the same method, we can also give constraints of \(g_S^eg_S^e\) and \(g_P^eg_P^e\) for electrons. This method works at small distances from \(\sim \) nm to \(\sim \) mm. Moreover, it can give pure constraints only between the electrons, while many other methods cannot easily isolate the contributions from other fermions like protons or neutrons. Our results for the electron are consistent with zero.

The fact that no new interactions have been detected for electrons, neutrons and protons indicates the muon might be an interesting target for these new forces at long ranges. It is possible that these new interactions might be muonic which means they only couple to the muons. Though studies have performed for muonic new interactions at very short ranges (new boson mass heavier than \(\sim \) MeV), to the best of our knowledge, no experiments have ever been done to search for these spin-dependent new interactions at long ranges (new boson mass lighter than \(\sim \)100 eV).

Notes

Acknowledgements

We acknowledge support from the National Natural Science Foundation of China, under Grant 91636103, 11675152, 11875238. This work was also supported by National Key Program for Research and Development (Grant 2016YFA0401504). We thank Dr. Queiroz and Dr. Stadnik for providing us useful references. We thank Dr. Stadnik for helpful discussions.

Supplementary material

10052_2019_7442_MOESM1_ESM.pdf (193 kb)
Supplementary material 1 (pdf 192 KB)

References

  1. 1.
    M. Tanabashi et al., Particle Data Group. Phys. Rev. D 98, 030001 (2018)Google Scholar
  2. 2.
    B. Dobrescu, I. Mocioiu, J. High Energy Phys. 11, 005 (2006)ADSCrossRefGoogle Scholar
  3. 3.
    W.A. Terrano, E.G. Adelberger, J.G. Lee, B.R. Heckel, Phys. Rev. Lett. 115, 201801 (2015)ADSCrossRefGoogle Scholar
  4. 4.
    M. Bulatowicz et al., Phys. Rev. Lett. 111, 102001 (2013)ADSCrossRefGoogle Scholar
  5. 5.
    K. Tullney et al., Phys. Rev. Lett. 111, 100801 (2013)ADSCrossRefGoogle Scholar
  6. 6.
    G. Vasilakis, J.M. Brown, T.W. Kornack, W. Ketter, M.V. Romalis, Phys. Rev. Lett. 104, 261801 (2009)ADSCrossRefGoogle Scholar
  7. 7.
    H. Yan et al., Eur. Phys. J. C 74, 3088 (2014)ADSCrossRefGoogle Scholar
  8. 8.
    J.E. Moody, F. Wilczek, Phys. Rev. D 30, 130 (1984)ADSCrossRefGoogle Scholar
  9. 9.
    C. Fu et al., Phys. Rev. Lett. 119, 181806 (2017)ADSCrossRefGoogle Scholar
  10. 10.
    J.E. Kim, G. Carosi, Rev. Mod. Phys. 82, 557 (2010)ADSCrossRefGoogle Scholar
  11. 11.
    S.A. Hoedl, F. Fleischer, E.G. Adelberger, B.R. Heckel, Phys. Rev. Lett. 106, 041801 (2011)ADSCrossRefGoogle Scholar
  12. 12.
    G. Raffelt, Phys. Rev. D 86, 015001 (2012)ADSCrossRefGoogle Scholar
  13. 13.
    M.P. Ledbetter, M.V. Romalis, D.F.J. Kimball, Phys. Rev. Lett. 110, 040402 (2013)ADSCrossRefGoogle Scholar
  14. 14.
    T.M. Leslie, E. Weisman, R. Khatiwada, J.C. Long, Phys. Rev. D 89, 114022 (2014)ADSCrossRefGoogle Scholar
  15. 15.
    P.-H. Chu, E. Weisman, C.-Y. Liu, J.C. Long, Phys. Rev. D 91, 102006 (2015)ADSCrossRefGoogle Scholar
  16. 16.
    S. Kotler, R. Ozeri, D.F.J. Kimball, Phys. Rev. Lett. 115, 081801 (2015)ADSCrossRefGoogle Scholar
  17. 17.
    P.-H. Chu, Y.J. Kim, I. Savukov, Phys. Rev. D 94, 036002 (2016)ADSCrossRefGoogle Scholar
  18. 18.
    F. Ficek, D.F.J. Kimball, M.G. Kozlov, N. Leefer, S. Pustelny, D. Budker, Phys. Rev. A 95, 032505 (2017)ADSCrossRefGoogle Scholar
  19. 19.
    A. Antognini et al., Science 339, 417 (2013)ADSCrossRefGoogle Scholar
  20. 20.
    R. Pohl et al., Science 353, 669 (2016)ADSCrossRefGoogle Scholar
  21. 21.
    B. Batell, D. McKeen, M. Pospelov, Phys. Rev. Lett. 107, 011803 (2011)ADSCrossRefGoogle Scholar
  22. 22.
    V. Barger, C.W. Chiang, W.Y. Keung, D. Marfatia, Phys. Rev. Lett. 108, 081802 (2012)ADSCrossRefGoogle Scholar
  23. 23.
    W. Bernreuther, M. Suzuki, Rev. Mod. Phys. 63, 313 (1991)ADSCrossRefGoogle Scholar
  24. 24.
    C. Itzykson, J.-B. Zuber, Quantum Field Theory (McGraw-Hill Inc, New York, 1980)zbMATHGoogle Scholar
  25. 25.
    M. Knecht, arXiv:hep-ph/0307239, (2003)
  26. 26.
    A. Zee, Quantum Field Theory in a Nutshell (Princeton University Press, Princeton, 2010)zbMATHGoogle Scholar
  27. 27.
    Supplementary Material for “Constraining New Muonic Interactions mediated by Axion-Like-Particles”, which includes Refs. [23, 24, 26]Google Scholar
  28. 28.
    M. Lindner, M. Platscher, F.S. Queiroz, arXiv: 1610.06587, (2016)
  29. 29.
    A.M. Baldini et al., The MEG Collaboration. Eur. Phys. J. C 76, 223 (2016)Google Scholar
  30. 30.
    T.Blum et al. (RBC and UKQCD Bollaborations), Phys. Rev. Lett. 121, 022003 (2018)Google Scholar
  31. 31.
    G.W. Bennett et al. (Muon (g-2) Collaboration), Phys. Rev. D 80, 052008 (2009)Google Scholar
  32. 32.
    T. Aoyama, M. Hayakawa, T. Kinoshita, M. Nio, Phys. Rev. D 96, 011901(E) (2017)CrossRefGoogle Scholar
  33. 33.
    T. Aoyama, M. Hayakawa, T. Kinoshita, M. Nio, Phys. Rev. D 91, 033006 (2015)ADSCrossRefGoogle Scholar
  34. 34.
    T. Aoyama, M. Hayakawa, T. Kinoshita, M. Nio, Phys. Rev. Lett. 109, 111807 (2012)ADSCrossRefGoogle Scholar
  35. 35.
    The ACME collaboration, Nature 562, 355–360 (2018)Google Scholar
  36. 36.
    X. Rong et al., Nat. Commun. 9, 739 (2018)ADSCrossRefGoogle Scholar
  37. 37.
    V.A. Dzuba, V.V. Flambaum, I.B. Samsonov, Y.V. Stadnik, Phys. Rev. D 98, 035048 (2018)ADSCrossRefGoogle Scholar
  38. 38.
    Y.V. Stadnik, V.A. Dzuba, V.V. Flambaum, Phys. Rev. Lett. 120, 013202 (2018)ADSCrossRefGoogle Scholar
  39. 39.
    Y.V. Stadnik, private communicationGoogle Scholar
  40. 40.
    D. Andreica, Encycl. Condens. Matter Phys. (2005)Google Scholar
  41. 41.
    W. Ji et al., Phys. Rev. Lett. 121, 261803 (2018)ADSCrossRefGoogle Scholar

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© The Author(s) 2019

Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.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.

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Authors and Affiliations

  • H. Yan
    • 1
    Email author
  • G. A. Sun
    • 1
  • S. M. Peng
    • 2
  • H. Guo
    • 3
  • B. Q. Liu
    • 1
  • M. Peng
    • 1
  • H. Zheng
    • 1
  1. 1.Key Laboratory of Neutron PhysicsInstitute of Nuclear Physics and Chemistry, CAEPMianyangChina
  2. 2.Institute of Nuclear Physics and Chemistry, CAEPMianyangChina
  3. 3.Department of PhysicsSoutheast UniversityNanjingChina

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