Time-dependent particle production and particle number in cosmological de Sitter space

نویسندگان

چکیده

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Particle Production and Classical Condensates in De Sitter Space

The cosmological particle production in a k = 0 expanding de Sitter universe with a Hubble parameter H0 is considered for various values of mass or conformal coupling of a free, scalar field. One finds that, for a minimally coupled field with mass 0 ≤ m2 < 9H2 0/4 (except for m2 = 2H2 0 ), the onemode occupation number grows to unity soon after the physical wavelength of the mode becomes larger...

متن کامل

Finite particle creation in 3 + 1 de Sitter space

In this paper we calculate the particle creation as seen by a stationary observer in 3+1 de Sitter space. This particle creation is calculated using an observer dependent geometrically based definition of time which is used to quantize a field on two different spacelike surfaces. The Bogolubov transformation relating these two quantizations is then calculated and the resulting particle creation...

متن کامل

Particle Creation in de Sitter Spacetime and Time Quantization

In this paper,we discussed the particle creation in de Sitter spacetime. When discussing the particle creation in a very short span, in used of the temperature of de Sitter space, We found that we must quantize the time.

متن کامل

Super algebra and Harmonic Oscillator in Anti de Sitter space

The harmonic oscillator in anti de Sitter space(AdS) is discussed. We consider the harmonic oscillator potential and then time independent Schrodinger equation in AdS space. Then we apply the supersymmetric Quantum Mechanics approach to solve our differential equation. In this paper we have solved Schrodinger equation for harmonic oscillator in AdS spacetime by supersymmetry approach. The shape...

متن کامل

The Dirac particle on de Sitter background

We show that the Dirac equation on de Sitter background can be analytically solved in a special static frame where the energy eigenspinors can be expressed in terms of usual angular spinors known from special relativity, and a pair of radial wave functions.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: International Journal of Modern Physics D

سال: 2015

ISSN: 0218-2718,1793-6594

DOI: 10.1142/s0218271815500315