Weak-field limit of Kaluza-Klein models with spherical compactification: experimental constraints

We investigate the classical gravitational tests for the six-dimensional Kaluza-Klein model with spherical (of a radius $a$) compactification of the internal space. The model contains also a bare multidimensional cosmological constant $\Lambda_6$. The matter, which corresponds to this ansatz, can be simulated by a perfect fluid with the vacuum equation of state in the external space and an arbitrary equation of state with the parameter $\omega_1$ in the internal space. For example, $\omega_1=1$ and $\omega_1=2$ correspond to the monopole two-forms and the Casimir effect, respectively. In the particular case $\Lambda_6=0$, the parameter $\omega_1$ is also absent: $\omega_1=0$. In the weak-field approximation, we perturb the background ansatz by a point-like mass. We demonstrate that in the case $\omega_1>0$ the perturbed metric coefficients have the Yukawa type corrections with respect to the usual Newtonian gravitational potential. The inverse square law experiments restrict the parameters of the model: $a/\sqrt{\omega_1}\lesssim 6\times10^{-3}\ {{cm}}$. Therefore, in the Solar system the parameterized post-Newtonian parameter$\gamma$is equal to 1 with very high accuracy. Thus, our model satisfies the gravitational experiments (the deflection of light and the time delay of radar echoes) at the same level of accuracy as General Relativity. We demonstrate also that our background matter provides the stable compactification of the internal space in the case$\omega_1>0$. However, if$\omega_1=0$, then the parameterized post-Newtonian parameter$\gamma=1/3$, which strongly contradicts the observations.Comment: 8 pages, no figures, revised version, equations and references added, accepted for publication in Phys. Rev. D. arXiv admin note: significant text overlap with arXiv:1107.338

Asymptotic latent solitons, black strings and black branes in f(R)-gravity

We investigate nonlinear f(R) theories in the Kaluza-Klein models with toroidal compactification of extra dimensions. A point-like matter source has the dust-like equation of state in our three dimensions and nonzero equations of state in the extra dimensions. We obtain solutions of linearized Einstein equations with this matter source taking into account effects of nonlinearity of the model. There are two asymptotic regions where solutions satisfy the gravitational tests at the same level of accuracy as General Relativity. According to these asymptotic regions, there are two classes of solutions. We call these solutions asymptotic latent solitons. The asymptotic latent solitons from the first class generalize the known result of the linear theory. The asymptotic black strings and black branes are particular cases of these asymptotic solutions. The second class of asymptotic solitons exists only in multidimensional nonlinear models. The main feature for both of these classes of solutions is that the matter sources have tension in the extra dimensions.Comment: RevTex4 5 pages, no figure

Kaluza-Klein models: can we construct a viable example?

In Kaluza-Klein models, we investigate soliton solutions of Einstein equation. We obtain the formulas for perihelion shift, deflection of light, time delay of radar echoes and PPN parameters. We find that the solitonic parameter k should be very big: |k|\geq 2.3\times10^4. We define a soliton solution which corresponds to a point-like mass source. In this case the soliton parameter k=2, which is clearly contrary to this restriction. Similar problem with the observations takes place for static spherically symmetric perfect fluid with the dust-like equation of state in all dimensions. The common for both of these models is the same equations of state in our three dimensions and in the extra dimensions. All dimensions are treated at equal footing. To be in agreement with observations, it is necessary to break the symmetry between the external/our and internal spaces. It takes place for black strings which are particular examples of solitons with k\to \infty. For such k, black strings are in concordance with the observations. Moreover, we show that they are the only solitons which are at the same level of agreement with the observations as in general relativity. Black strings can be treated as perfect fluid with dust-like equation of state p_0=0 in the external/our space and very specific equation of state p_1=-(1/2)\epsilon in the internal space. The latter equation is due to negative tension in the extra dimension. We also demonstrate that dimension 3 for the external space is a special one. Only in this case we get the latter equation of state. We show that the black string equations of state satisfy the necessary condition of the internal space stabilization. Therefore, black strings are good candidates for a viable model of astrophysical objects (e.g., Sun) if we can provide a satisfactory explanation of negative tension for particles constituting these objects.Comment: 11 pages, Revtex4, no figures, appendix and references adde

Bouncing inflation in nonlinear R2+R4R^2+R^4 gravitational model

We study a gravitational model with curvature-squared $R^2$ and curvature-quartic $R^4$ nonlinearities. The effective scalar degree of freedom $\phi$ (scalaron) has a multi-valued potential $U(\phi)$ consisting of a number of branches. These branches are fitted with each other in the branching and monotonic points. In the case of four-dimensional space-time, we show that the monotonic points are penetrable for scalaron while in the vicinity of the branching points scalaron has the bouncing behavior and cannot cross these points. Moreover, there are branching points where scalaron bounces an infinite number of times with decreasing amplitude and the Universe asymptotically approaches the de Sitter stage. Such accelerating behavior we call bouncing inflation. For this accelerating expansion there is no need for original potential $U(\phi)$ to have a minimum or to check the slow-roll conditions. A necessary condition for such inflation is the existence of the branching points. This is a new type of inflation. We show that bouncing inflation takes place both in the Einstein and Brans-Dicke frames.Comment: RevTex 13 pages, 13 figures, a few comments and references adde

Weak-field limit of f(R)-gravity in three and more spatial dimensions

We investigate a point-like massive source in non-linear f(R) theories in the case of arbitrary number of spatial dimensions D\geq 3. If D>3 then extra dimensions undergo toroidal compactification. We consider a weak-field approximation with Minkowski and de Sitter background solutions. In both these cases point-like massive sources demonstrate good agreement with experimental data only in the case of ordinary three-dimensional (D=3) space. We generalize this result to the case of perfect fluid with dust-like equations of state in the external and internal spaces. This perfect fluid is uniformly smeared over all extra dimensions and enclosed in a three-dimensional sphere. In ordinary three dimensional (D=3) space, our formulas are useful for experimental constraints on parameters of f(R) models.Comment: 8 pages, Revtex4, no figure

Restrictions on dilatonic brane-world models

We consider dilatonic brane-world models with a non-minimal coupling between a dilaton and usual matter on a brane. We demonstrate that variation of the fundamental constants on the brane due to such interaction leads to strong restrictions on parameters of models. In particular, the experimental bounds on variation of the fine structure constant rule out non-minimal dilatonic models with a Liouville-type coupling potential f(varphi) = exp (b varphi) where b is order of 1.Comment: MiKTeX2-LaTeX2e, 10 pages, minor changes, improved references, to appear in IJMP

Multidimensional cosmological models: cosmological and astrophysical implications and constraints

We investigate four-dimensional effective theories which are obtained by dimensional reduction of multidimensional cosmological models with factorizable geometry and consider the interaction between conformal excitations of the internal space (geometrical moduli excitations) and Abelian gauge fields. It is assumed that the internal space background can be stabilized by minima of an effective potential. The conformal excitations over such a background have the form of massive scalar fields (gravitational excitons) propagating in the external spacetime. We discuss cosmological and astrophysical implications of the interaction between gravexcitons and four-dimensional photons as well as constraints arising on multidimensional models of the type considered in our paper. In particular, we show that due to the experimental bounds on the variation of the fine structure constant, gravexcitons should decay before nucleosynthesis starts. For a successful nucleosynthesis the masses of the decaying gravexcitons should be m>10^4 GeV. Furthermore, we discuss the possible contribution of gravexcitons to UHECR. It is shown that, at energies of about 10^{20}eV, the decay length of gravexcitons with masses m>10^4 GeV is very small, but that for m <10^2 GeV it becomes much larger than the Greisen-Zatsepin-Kuzmin cut-off distance. Finally, we investigate the possibility for gravexciton-photon oscillations in strong magnetic fields of astrophysical objects. The corresponding estimates indicate that even the high magnetic field strengths of magnetars are not sufficient for an efficient and copious production of gravexcitons.Comment: 16 pages, LaTeX2e, minor changes, improved references, to appear in PR

ОСУЧАСНЕННЯ ТА МОДЕРНІЗАЦІЯ СИСТЕМИ ЕЛЕКТРОННИХ ПЛАТЕЖІВ НАЦІОНАЛЬНОГО БАНКУ УКРАЇНИ ЗА ЄВРОПЕЙСЬКИМ ДОСВІДОМ У КОНТЕКСТІ ГЛОБАЛІЗАЦІЙНИХ ПРОЦЕСІВ

Today for the System of Electronic Payments of the National Bank of Ukraine is actual modernization and updating according to the real needs of payment system participants in the current economic situation in Ukraine. For improvement forms of interbank payments important is a restructuring of the national payment system in accordance with international and EU standards. The article analyzes the functioning of the payment system TARGET2, discloses its advantages and principles of organization. The authors conducted a comparative analysis of payment systems TARGET2 and The System of Electronic Payments of the National Bank of Ukraine, as well as provided recommendations for improving the domestic payment system based on the experience of the European Union The NBU’s Electronic Payment System is quite modern and efficient, but the existence of a certain time in the payment process, insufficient level of regulatory and information support of the electronic payment system participants and its control lead to the possibility of opaque financial transactions in the system itself. The lack of organizational and financial mechanisms today is also a serious drawback in his work. In Ukraine, the technological level of the NBU system of calculations does not quite allow to use qualitatively most of the means of supporting intraday liquidity. This is a significant disadvantage of EPS compared to its foreign counterpart TARGET2. An analysis of the functioning of TARGET2 and SEP enabled us to examine in more detail the positives and negatives of both payment systems. A significant advantage of TARGET2 is its liquidity management system, which, under certain conditions, is an effective tool in the planning of settlement operations. This allows system members to prevent problems during the calculations and to solve them effectively. Optimization of liquidity management in the SEP is negligible. The National Bank of Ukraine, unlike the European Central Bank, does not provide full information on EPS, which indicates the closedness of the payment system and the NBU’s unwillingness to provide the most transparent settlement mechanism. Today, the TARGET2 settlement system is more modern and open compared to the NBU’s Electronic Payment System.На сьогодні для Системи електронних платежів Національного банку України актуальною є модернізація та осучаснення відповідно до реальних потреб учасників платіжної системи в умовах сучасної економічної ситуації в Україні. Для вдосконалення форм міжбанківських розрахунків важливою є перебудова національної платіжної системи відповідно до міжнародних стандартів і стандартів ЄС. Проведено аналіз функціонування платіжної системи ТАРГЕТ2, розкрито її переваги і принципи організації. Проведено порівняльний аналіз платіжних систем ТАРГЕТ2 та системи електронних платежів Національного банку, а також надано рекомендації щодо вдосконалення вітчизняної платіжної системи на основі досвіду Європейського Союзу. Система електронних платежів НБУ є досить сучасною та ефективною, але існування певного часу у проходженні платежу, недостатньо високий рівень нормативного та інформаційного забезпечення учасників системи електронних платежів та її контролю призводять до можливості непрозорих фінансових операцій у самій системі. В Україні технологічний рівень розрахункової системи НБУ не зовсім дозволяє якісно використовувати більшість із засобів підтримки внутрішньоденної ліквідності, що є значним недоліком СЕП у порівнянні з її зарубіжним аналогом — ТАРГЕТ2. Аналіз функціонування ТАРГЕТ2 та СЕП надав змогу більш детально розглянути позитивні і негативні моменти обох платіжних систем. Значною перевагою ТАРГЕТ2 є система управління ліквідністю, що за певних умов є дієвим інструментом при плануванні розрахункових операцій. Це дозволяє учасникам системи попереджувати виникнення проблем під час розрахунків та ефективно розв’язувати їх. Оптимізація управління ліквідністю у СЕП є незначною. Національний банк України, на відміну від Європейського центрального банку, надає інформацію стосовно СЕП не в повному обсязі, що свідчить про закритість платіжної системи та неготовність НБУ забезпечувати максимально прозорий механізм розрахунків. На сьогодні система розрахунків ТАРГЕТ2 є більш сучасною та відкритою у порівнянні із Cистемою електронних платежів НБУ

Slow-roll inflation in (R+R*4) gravity

We reconsider the toy-model of topological inflation, based on the R*4-modified gravity. By using its equivalence to the certain scalar-tensor gravity model in four space-time dimensions, we compute the inflaton scalar potential and investigate a possibility of inflation. We confirm the existence of the slow-roll inflation with an exit. However, the model suffers from the eta-problem that gives rise to the unacceptable value of the spectral index n_s of scalar perturbations.Comment: 12 pages, 3 figures, LaTeX, misprints corrected and references update

Anisotropic Inflation and the Origin of Four Large Dimensions

In the context of (4+d)-dimensional general relativity, we propose an inflationary scenario wherein 3 spatial dimensions grow large, while d extra dimensions remain small. Our model requires that a self-interacting d-form acquire a vacuum expectation value along the extra dimensions. This causes 3 spatial dimensions to inflate, whilst keeping the size of the extra dimensions nearly constant. We do not require an additional stabilization mechanism for the radion, as stable solutions exist for flat, and for negatively curved compact extra dimensions. From a four-dimensional perspective, the radion does not couple to the inflaton; and, the small amplitude of the CMB temperature anisotropies arises from an exponential suppression of fluctuations, due to the higher-dimensional origin of the inflaton. The mechanism triggering the end of inflation is responsible, both, for heating the universe, and for avoiding violations of the equivalence principle due to coupling between the radion and matter.Comment: 24 pages, 2 figures; uses RevTeX4. v2: Minor changes and added references. v3: Improved discussion of slow-rol