In this paper we calculate the particle creation as seen by a stationary observer in an anisotropic universe. By using an observer and geometry dependent time to quantize a massive scalar field we show that a discrete energy spectrum shift occurs. The length scale associated with the geometry provides the energy scale by which the spectrum is shifted. The beta(p, q) coefficient for the Bogolubov transformation calculated is proportional to a series of delta functions whose argument contains p and q and half multiples of the root of the curvature.
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Lanzhou Univ, Inst Theoret Phys, Sch Phys Sci & Technol, 222 South Tianshui Rd, Lanzhou 730000, Peoples R China
Univ Lisbon, Fac Cincias, Inst Astrofis & Cincias Espao, Ed C8, P-1769016 Lisbon, PortugalLanzhou Univ, Inst Theoret Phys, Sch Phys Sci & Technol, 222 South Tianshui Rd, Lanzhou 730000, Peoples R China
Delliou, Morgan Le
Deliyergiyev, Maksym
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Univ Geneva, Dept Phys Nucl & Corpusculaire, CH-1211 Geneva, SwitzerlandLanzhou Univ, Inst Theoret Phys, Sch Phys Sci & Technol, 222 South Tianshui Rd, Lanzhou 730000, Peoples R China
Deliyergiyev, Maksym
del Popolo, Antonino
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Univ Catania, Dipartimento Fis & Astron, Viale Andrea Doria, I-95125 Catania, Italy
Russian Acad Sci, Inst Astron, Pyatnitskaya Str 48, Moscow 119017, Russia
INFN Sez Catania, Via S Sofia 64, I-95123 Catania, ItalyLanzhou Univ, Inst Theoret Phys, Sch Phys Sci & Technol, 222 South Tianshui Rd, Lanzhou 730000, Peoples R China