48 research outputs found
Scalar fields in the de Sitter spacetime
We examine long-wavelength correlation functions of massive scalar fields in de Sitter spacetime. For the theory with a quartic self-interaction, the two-point function is calculated up to two loops. Comparing our results with the Hartree-Fock approximation and with the stochastic approach shows that the former resums only the cactus type diagrams, whereas the latter contains the sunset diagram as well and produces the correct result. We compare our results with the preceding results obtained for the massless scalar field
Higgs Starobinsky inflation
In this paper we point out that Starobinky inflation could be induced by quantum effects due to a large non-minimal coupling of the Higgs boson to the Ricci scalar. The Higgs Starobinsky mechanism provides a solution to issues attached to large Higgs field values in the early universe which in a metastable universe would not be a viable option. We verify explicitly that these large quantum corrections do not destabilize Starobinsky's potential
Modeling the quantum evolution of the universe through classical matter
It is well known that the canonical quantization of the
Friedmann-Lema\^itre-Robertson-Walker (FLRW) filled with a perfect fluid leads
to nonsingular universes which, for later times, behave as their classical
counterpart. This means that the expectation value of the scale factor
never vanishes and, as , we recover the classical expression for
the scale factor. In this paper, we show that such universes can be reproduced
by classical cosmology given that the universe is filled with an exotic matter.
In the case of a perfect fluid, we find an implicit equation of state (EoS). We
then show that this single fluid with an implict EoS is equivalent to two
non-interacting fluids, one of them representing stiff matter with negative
energy density. In the case of two non-interacting scalar fields, one of them
of the phantom type, we find their potential energy. In both cases we find that
quantum mechanics changes completely the configuration of matter for small
values of time, by adding a fluid or a scalar field with negative energy
density. As time passes, the density of negative energy decreases and we
recover the ordinary content of the classical universe. The more the initial
wave function of the universe is concentrated around the classical big bang
singularity, the more it is necessary to add negative energy, since this type
of energy will be responsible for the removal of the classical singularity.Comment: updated version as accepted by Gen. Relativ. Gravi
Gravitational Collapse of the Shells with the Smeared Gravitational Source in Noncommutative Geometry
We study the formation of the (noncommutative) Schwarzschild black hole from
collapsing shell {of the} generalized matters containing polytropic and
Chaplygin gas. We show that this collapsing shell depending on various
parameters forms either a black hole or a naked singular shell with the help of
the pressure.Furthermore, by considering the smeared gravitational sources, we
investigate the noncommutative black holes formation. Though this mild
noncommutative correction of matters cannot ultimately resolve the emergence of
the naked singularity, we show that in some parameter region the collapsing
shell evolves to a noncommutative black hole before becoming a naked singular
shell.Comment: 16 pages, LateX, 9 figures, Title changed in this published versio
AIC, BIC, Bayesian evidence against the interacting dark energy model
Recent astronomical observations have indicated that the Universe is in the
phase of accelerated expansion. While there are many cosmological models which
try to explain this phenomenon, we focus on the interacting CDM model
where the interaction between the dark energy and dark matter sectors takes
place. This model is compared to its simpler alternative---the CDM
model. To choose between these models the likelihood ratio test was applied as
well as the model comparison methods (employing Occam's principle): the Akaike
information criterion (AIC), the Bayesian information criterion (BIC) and the
Bayesian evidence. Using the current astronomical data: SNIa (Union2.1),
, BAO, Alcock--Paczynski test and CMB we evaluated both models. The
analyses based on the AIC indicated that there is less support for the
interacting CDM model when compared to the CDM model, while
those based on the BIC indicated that there is the strong evidence against it
in favor the CDM model. Given the weak or almost none support for the
interacting CDM model and bearing in mind Occam's razor we are
inclined to reject this model.Comment: LaTeX svjour3, 12 pages, 3 figure
Higgs field in cosmology
The accelerated expansion of the early universe is an integral part of modern
cosmology and dynamically realized by the mechanism of inflation. The simplest
theoretical description of the inflationary paradigm is based on the assumption
of an additional propagating scalar degree of freedom which drives inflation -
the inflaton. In most models of inflation the fundamental nature of the
inflaton remains unexplained. In the model of Higgs inflation, the inflaton is
identified with the Standard Model Higgs boson and connects cosmology with
elementary particle physics. A characteristic feature of this model is a
non-minimal coupling of the Higgs boson to gravity. I review and discuss
several phenomenological and fundamental aspects of this model, including the
impact of quantum corrections and the renormalization group, the derivation of
initial conditions for Higgs inflation in a quantum cosmological framework and
the classical and quantum equivalence of different field parametrizations.Comment: 36 pages, 9 figures; references added, typos corrected. Invited
contribution to the Heraeus-Seminar "Hundred Years of Gauge Theory", 30 July
- 3 August 2018, Physikzentrum Bad Honnef, organized by Silvia De Bianchi and
Claus Kiefer. To appear in the proceedings "100 Years of Gauge Theory. Past,
present and future perspectives" in the series `Fundamental Theories of
Physics' (Springer