Complex Lagrangians and phantom cosmology

被引:31
作者
Andrianov, A. A. [1 ]
Cannata, F.
Kamenshchik, A. Y.
机构
[1] St Petersburg State Univ, VA Fock Dept Theoret Phys, St Petersburg 198904, Russia
[2] Dipartimento Fis, I-40126 Bologna, Italy
[3] Ist Nazl Fis Nucl, I-40126 Bologna, Italy
[4] Russian Acad Sci, LD Landau Theoret Phys Inst, Moscow 119334, Russia
来源
JOURNAL OF PHYSICS A-MATHEMATICAL AND GENERAL | 2006年 / 39卷 / 32期
关键词
D O I
10.1088/0305-4470/39/32/S02
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Motivated by the generalization of quantum theory for the case of non-Hermitian Hamiltonians with PT symmetry, we show how a classical cosmological model describes a smooth transition from ordinary dark energy to the phantom one. The model is based on a classical complex Lagrangian of a scalar field. Specific symmetry properties analogous to PT in non-Hermitian quantum mechanics lead to purely real equations of motion.
引用
收藏
页码:9975 / 9982
页数:8
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