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arXiv 0704.2273hep-phastro-phhep-th
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宇宙对称性破缺、伪标度不变性、暗能量与标准模型

Cosmological Symmetry Breaking, Pseudo-scale invariance, Dark Energy and the Standard Model

Pankaj Jain, Subhadip Mitra

摘要:

今天宇宙的能量密度可能是由一个缓慢滚动的标量场的真空能量决定的。围绕这样一个含时解进行量子展开会破坏量子场论的基本对称性。我们称这种机制为宇宙学对称性破缺,并认为它不同于标准的自发对称性破缺现象。我们用一个玩具标量场理论来说明这一点,它的作用呈现U(1)对称性。我们确定了一种对称性,称为伪尺度不变性,它使宇宙学常数在经典理论和量子理论中都精确地等于零。这种对称性在宇宙学上也被打破,并导致非零真空或暗能量。慢滚条件与观测到的暗能量值一起导致背景标量场的值为普朗克质量的量级。我们还考虑了U(1)规范对称性模型。在这种情况下,宇宙学对称性破缺会导致向量场的质量不为零。我们还表明,宇宙学破碎的伪尺度不变性可以产生广泛的群众。

英文摘要:

The energy density of the universe today may be dominated by the vacuum energy of a slowly rolling scalar field. Making a quantum expansion around such a time dependent solution is found to break fundamental symmetries of quantum field theory. We call this mechanism cosmological symmetry breaking and argue that it is different from the standard phenomenon of spontaneous symmetry breaking. We illustrate this with a toy scalar field theory, whose action displays a U(1) symmetry. We identify a symmetry, called pseudo-scale invariance, which sets the cosmological constant exactly equal to zero, both in classical and quantum theory. This symmetry is also broken cosmologically and leads to a nonzero vacuum or dark energy. The slow roll condition along with the observed value of dark energy leads to a value of the background scalar field of the order of Planck mass. We also consider a U(1) gauge symmetry model. Cosmological symmetry breaking, in this case, leads to a non zero mass for the vector field. We also show that a cosmologically broken pseudo-scale invariance can generate a wide range of masses.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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