Schwinger effect by an SU(2) gauge field during inflation

被引:36
|
作者
Lozanov, K. D. [1 ]
Maleknejad, A. [1 ]
Komatsu, E. [1 ,2 ]
机构
[1] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85741 Garching, Germany
[2] Univ Tokyo, Kavli IPMU, WPI, UTIAS, Chiba 2778583, Japan
关键词
Cosmology of Theories beyond the SM; Nonperturbative Effects; Spontaneous Symmetry Breaking; FLATNESS; UNIVERSE; HORIZON; VACUUM;
D O I
10.1007/JHEP02(2019)041
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Non-Abelian gauge fields may exist during inflation. We study the Schwinger effect by an SU(2) gauge field coupled to a charged scalar doublet in a (quasi) de Sitter background and the possible backreaction of the generated charged particles on the homogeneous dynamics. Contrary to the Abelian U(1) case, we find that both the Schwinger pair production and the induced current decrease as the interaction strength increases. The reason for this suppression is the isotropic vacuum expectation value of the SU(2) field which generates a (three times) greater effective mass for the scalar field than the U(1). In the weak interaction limit, the above effect is negligible and both the SU(2) and U(1) cases exhibit a linear increase of the current and a constant conductivity with the interaction strength. We conclude that the Schwinger effect does not pose a threat to the dynamics of inflationary models involving an SU(2) gauge field.
引用
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页数:33
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