Cosmic bubble and domain wall instabilities I: parametric amplification of linear fluctuations

被引:33
|
作者
Braden, Jonathan [1 ,2 ]
Bond, J. Richard [1 ]
Mersini-Houghton, Laura [3 ]
机构
[1] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada
[2] Univ Toronto, Dept Phys, Toronto, ON M5S 3H8, Canada
[3] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2015年 / 03期
关键词
cosmological phase transitions; Cosmic strings; domain walls; monopoles; cosmological applications of theories with extra dimensions; VACUUM; UNIVERSE; RESONANCE; STRINGS;
D O I
10.1088/1475-7516/2015/03/007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is the first paper in a series where we study collisions of nucleated bubbles taking into account the effects of small initial (quantum) fluctuations in a fully 3+1-dimensional setting. In this paper, we consider the evolution of linear fluctuations around highly symmetric though inhomogeneous backgrounds. In particular, we demonstrate that a large degree of asymmetry develops over time from tiny initial fluctuations superposed upon planar and SO(2; 1) symmetric backgrounds. These fluctuations are inevitable consequences of zero-point vacuum oscillations, so excluding them by enforcing a high degree of spatial symmetry is inconsistent in a quantum treatment. To simplify the analysis we consider the limit of two colliding planar walls, with mode functions for the fluctuations characterized by the wavenumber transverse to the collision direction and a longitudinal shape along the collision direction x, which we solve for. In the linear regime, the fluctuations obey a linear wave equation with a time-and space-dependent mass m(eff) (x,t). In situations where the walls collide multiple times, meff oscillates in time. We use Floquet theory to study the evolution of the fluctuations and generalize the calculations familiar from the preheating literature to the case with many coupled degrees of freedom. The inhomogeneous case has bands of unstable transverse wavenumbers k perpendicular to whose corresponding mode functions grow exponentially. By examining the detailed spatial structure of the mode functions in x, we identify both broad and narrow parametric resonance generalizations of the homogeneous m(eff) (t) case of preheating. The unstable k perpendicular to modes are longitudinally localized, yet can be described as quasiparticles in the Bogoliubov sense. We de fine an effective occupation number and show they are created in bursts for the case of well-defined collisions in the background. The transverse-longitudinal coupling accompanying nonlinearity radically breaks this localized particle description, with nonseparable 3D modes arising that will be studied in subsequent papers.
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页数:42
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