Yoshinobu Habara
Kyoto University
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Featured researches published by Yoshinobu Habara.
Physics Letters B | 2012
Yoshinobu Habara; Hikaru Kawai; Masao Ninomiya; Yasuhiro Sekino
Abstract We propose a mechanism for the generation of temperature fluctuations of cosmic microwave background. We consider a large number of fields, such as Kaluza–Klein modes and string excitations. Each field contributes to the gravitational potential by a small amount, but an observable level of temperature fluctuations is achieved by summing up the contribution of typically of order 1014 fields. Tensor fluctuations are hardly affected by these fields. Our mechanism is based on purely quantum effects of the fields which are classically at rest, and is different from the one in slow-roll inflation. Using the observed data, we find constraints on the parameters of this model, such as the size of the extra dimensions and the string scale. Our model predicts a particular pattern of non-gaussianity with a small magnitude.
International Journal of Modern Physics A | 2008
Yoshinobu Habara; Yukinori Nagatani; Holger Bech Nielsen; Masao Ninomiya
Bosonic formulation of the negative energy sea, so-called Dirac sea, is proposed by constructing a hole theory for bosons as a new formulation of the second quantization of bosonic fields. The original idea of Dirac sea for fermions, where the vacuum state is considered as a state completely filled by fermions of negative energy and holes in the sea are identified as antiparticles, is extended to boson case in a consistent manner. The bosonic vacuum consists of a sea filled by negative energy bosonic states, while physical probabilities become always positive definite. We introduce a method of the double harmonic oscillator to formulate the hole theory of bosons. Our formulation is also applicable to supersymmetric field theory. The sea for supersymmetric theories has an explicit supersymmetry. We suggest applications of our formulations to the anomaly theories and the string theories.
Journal of High Energy Physics | 2015
Yoshinobu Habara; Hikaru Kawai; Masao Ninomiya
A bstractIt is shown that the inflationary era in early universe is realized due to the effect of backreaction of quantized matter fields. In fact we start by quantizing a free scalar field in the Friedmann-Robertson-Walker space-time, and the field is fluctuating quantum mechanically around the bottom of the mass potential. We then obtain the vacuum expectation value of the energy density of the scalar field as a functional of the scale factor a(t) of the universe. By plugging it into the Einstein equation, a self-consistent equation is established in which the matter fields determine the time evolution of the universe. We solve this equation by setting few conditions and find the following solution: the universe expands à la de Sitter with e-folding number ≳ 60 and then it turns to shrink with a decreasing Hubble parameter H(t) which rapidly goes to zero.
Physical Review D | 2012
Yoshinobu Habara; Yasuhiro Sekino; Masao Ninomiya; Hikaru Kawai
We point out that the temperature fluctuations of cosmic microwave background (CMB) can be generated in a way that is different from the one usually assumed in slow-roll inflation. Our mechanism is based on vacuum fluctuations of fields which are at rest at the bottom of the potential, such as Kaluza-Klein modes or string excited states. When there are a large number (typically of order
International Journal of Modern Physics A | 2008
Yoshinobu Habara; Yukinori Nagatani; Holger Bech Nielsen; Masao Ninomiya
N\sim 10^{14}
International Journal of Modern Physics | 2015
Yoshinobu Habara; Holger Bech Nielsen; Masao Ninomiya
) of fields with small mass in unit of Hubble parameter during the inflationary era, this effect can give significant contributions to the CMB temperature fluctuations. This number
International Journal of Modern Physics A | 2006
Yoshinobu Habara; Holger Bech Nielsen; Masao Ninomiya
N
Progress of Theoretical Physics | 2006
Yoshinobu Habara
makes it possible to enhance scalar perturbation relative to tensor perturbation. Comparison with the observed amplitudes suggests that models with string scale of order
International Journal of Modern Physics A | 2004
Yoshinobu Habara; Holger Bech Nielsen; Masao Ninomiya
10^{-5}
arXiv: High Energy Physics - Theory | 2015
Yoshinobu Habara; Masao Ninomiya; Holger Bech Nielsen
of 4D Planck scale are favorable.