Academic Journal

Aspects of Cosmic Inflation in Expanding

التفاصيل البيبلوغرافية
العنوان: Aspects of Cosmic Inflation in Expanding
المؤلفون: Bose-einstein Condensates, Michael Uhlmann, Yan Xu, Ralf Schützhold
المساهمون: The Pennsylvania State University CiteSeerX Archives
المصدر: http://arxiv.org/pdf/quant-ph/0509063v1.pdf.
سنة النشر: 2005
المجموعة: CiteSeerX
الوصف: Phonons in expanding Bose-Einstein condensates with wavelengths much larger than the healing length behave in the same way as quantum fields within a universe undergoing an accelerated expansion. This analogy facilitates the application of many tools and concepts known from general relativity (such as horizons) and the prediction of the corresponding effects such as the freezing of modes after horizon crossing and the associated amplification of quantum fluctuations. Basically the same amplification mechanism is (according to our standard model of cosmology) supposed to be responsible for the generation of the initial inhomogeneities – and hence the seeds for the formation of structures such as our galaxy – during cosmic inflation (i.e., a very early epoch in the evolution of our universe). After a general discussion of the analogy (analogue cosmology), we calculate the frozen and amplified density-density fluctuations for quasi-two dimensional (Q2D) and three dimensional (3D) condensates which undergo a free expansion after switching off the (longitudinal) trap.
نوع الوثيقة: text
وصف الملف: application/pdf
اللغة: English
Relation: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.251.9929; http://arxiv.org/pdf/quant-ph/0509063v1.pdf
الاتاحة: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.251.9929
http://arxiv.org/pdf/quant-ph/0509063v1.pdf
Rights: Metadata may be used without restrictions as long as the oai identifier remains attached to it.
رقم الانضمام: edsbas.4D36BDBA
قاعدة البيانات: BASE