4,012 research outputs found
The Debate around Nihilism in 1860s Russian Literature
This investigation investigates the extent to which literature and criticism were politically charged in 1860s Russia. Ideology was clearly present within both literature and literary criticism, despite claims to the contrary. Pisarev, despite his claims to view a text without ideology, in his criticism demonstrated his preference for the Nihilist movement to which he belonged. The fact that Turgenevâs novel sparked such a furore shows how tense society was during this period. The controversy caused shows the extent to which Russia was in need of reform through the degree of division in the national response. Turgenev explained how âone critic even brought forth the fact that I made Bazarov lose at cards to Father Alexey. âHe just doesnât know how to wound and humiliate enough! He doesnât even know how to play cards!â There is absolutely no doubt that if I had made Bazarov win, the same critic would triumphantly exclaim: âIsnât it clear? The author wants to suggest that Bazarov is a cheat!
Abundance Uncertainties Obtained With the PizBuin Framework For Monte Carlo Reaction Rate Variations
Uncertainties in nucleosynthesis models originating from uncertainties in
astrophysical reaction rates were estimated in a Monte Carlo variation
procedure. Thousands of rates were simultaneously varied within individual,
temperature-dependent errors to calculate their combined effect on final
abundances. After a presentation of the method, results from application to
three different nucleosynthesis processes are shown: the -process and
the s-process in massive stars, and the main s-process in AGB stars
(preliminary results). Thermal excitation of nuclei in the stellar plasma and
the combined action of several reactions increase the final uncertainties above
the level of the experimental errors. The total uncertainty, on the other hand,
remains within a factor of two even in processes involving a large number of
unmeasured rates, with some notable exceptions for nuclides whose production is
spread over several stellar layers and for s-process branchings.Comment: 8 pages, 4 figures; Proceedings of OMEG 2017, Daejeon, Korea, June
27-30, 2017; to appear in AIP Conf. Pro
The development of a ânormative battlegroundâ between the EU and Russia from 2004 to 2014
This thesis will chart the development of a ânormative battlegroundâ between the European
Union and Russia within Ukraine. This ânormative battlegroundâ stems from the clashing
securitising projects both the EU and Russia are implementing within Ukraine in order to shape
the development of the country according to their own interests. The EU and Russia are widely
believed to carry out securitising projects from within different international relations spheres.
For this thesis, these are the EUâs âpostmodernâ/âKantianâ security project, which is
incompatible with the Russian âmodernâ/âHobbesianâ security project. These security projects
are manifesting themselves in the norms each side is promoting, and this is where the clash is
particularly visible, this is the ânormative battlegroundâ. This thesis seeks to provide a holistic
conceptualisation of the term ânormative battlegroundâ within the framework of Buzanâs English
School Triad and to tie its development with the contrasting securitising projects being
implemented within Ukraine.http://www.ester.ee/record=b4701254*es
Phase transition of the susceptible-infected-susceptible dynamics on time-varying configuration model networks
We present a degree-based theoretical framework to study the
susceptible-infected-susceptible (SIS) dynamics on time-varying (rewired)
configuration model networks. Using this framework, we provide a detailed
analysis of the stationary state that covers, for a given structure, every
dynamic regimes easily tuned by the rewiring rate. This analysis is suitable
for the characterization of the phase transition and leads to three main
contributions. (i) We obtain a self-consistent expression for the
absorbing-state threshold, able to capture both collective and hub activation.
(ii) We recover the predictions of a number of existing approaches as limiting
cases of our analysis, providing thereby a unifying point of view for the SIS
dynamics on random networks. (iii) We reinterpret the concept of hub-dominated
phase transition. Within our framework, it appears as a heterogeneous critical
phenomenon : observables for different degree classes have a different scaling
with the infection rate. This leads to the successive activation of the degree
classes beyond the epidemic threshold.Comment: 14 pages, 11 figure
Uncertainties in the Production of p Nuclides in SN Ia Determined by Monte Carlo Variations
© Springer Nature Switzerland AG 2019Several thousand tracers from a 2D model of a thermonuclear supernova were used in a Monte Carlo post-processing approach to determine p-nuclide abundance uncertainties originating from nuclear physics uncertainties in the reaction rates.Final Accepted Versio
Xe diffusion and bubble nucleation around edge dislocations in UO2
AbstractRecently it has been suggested that dislocations, generated by radiation damage, may increase the rate of fission gas diffusion from the fuel grains, an affect which is at present not incorporated into fuel performance codes. Therefore, we perform molecular dynamics simulations employing empirical potentials to investigate the diffusion of Xe atoms around edge dislocations in UO2 to establish the importance of this pathway for fission gas release. The results suggest that for isolated atoms near the dislocation the activation energy for Xe diffusion is dramatically reduced relative to the bulk. However, Xe atoms diffusing along the dislocation cluster together to form small bubbles, these bubbles incorporate all of the isolated mobile Xe atoms thereby inhibiting fast diffusion of Xe along the dislocation core
The s-process nucleosynthesis : Impact of the uncertainties in the nuclear physics determined by monte carlo variations
We investigated the impact of uncertainties in neutron-capture and weak reactions (on heavy elements) on the s-process nucleosynthesis in low-mass stars and massive stars using a Monte-Carlo based approach. We performed extensive nuclear reaction network calculations that include newly evaluated temperature-dependent upper and lower limits for the individual reaction rates. We found ÎČ-decay rate uncertainties affect only a few nuclei near s-process branchings, whereas most of the uncertainty in the final abundances is caused by uncertainties in the neutron capture rates. We suggest a list of uncertain rates as candidates for improved measurement by future experiments.Peer reviewe
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