The soft notion of China's 'soft power'

· Although debates over Chinese soft power have increased in recent years, there is no shared definition of what ‘soft power’ actually means. The definition seems to change depending on what the observer wants to argue. · External analyses of soft power often include a focus on economic relations and other material (hard) sources of power and influence. · Many Chinese analyses of soft power focus on the promotion of a preferred (positive) understanding of China’s interests and identities overseas. · Unpacking broad and inclusive definitions of soft power allows for the identification of different types and sources of power including national image promotion, normative power promotion and ‘imagined power’. · China’s emergence as an alternative economic partner seems to be the major source of attraction for other developing states, though it remains difficult to separate hard material factors from softer attraction to values and world-views

Assessment of Soft Power Strategies: Towards an Aggregative Analytical Model for Country-Focused Case Study Research

The paper advances a realist analytical model for case studies of national soft power policies. First, it argues that for the purposes of realist analysis, a soft power policy must be considered as a rational strategy pursued under the conditions of competition. Furthermore, it emphasises the importance of taking into account the specificities of the recipient state as well as the fact that a soft power strategy is targeted at both its elite and its public. In addition, the article substantiates the necessity to draw a clear-cut distinction between soft power sources and instruments and shows possible shortcomings that research can have should this distinction fail to be made. Finally, the paper discusses the impact of a competitor’s presence on a soft power strategy and specifies the terms under which disregarding this impact may engender a wrong conclusion

The affective underpinnings of soft power

The concept of soft power occupies a prominent place in International Relations, foreign policy, and security studies. Primarily developed by Joseph S. Nye, the concept is typically drawn upon to emphasize the more intangible dimensions of power in a field long dominated by overtly material (i.e. military) power. Recently, some scholars have reframed soft power — specifically the key notion of attraction — as a narrative and linguistic process. This literature, however, has downplayed some of the other deep-seated underpinnings of soft power, which this article argues lie in the dynamics of affect. Building upon the International Relations affect and aesthetics literatures, this article develops the concept of soft power as rooted in the political dynamics of emotion and introduces the concept of affective investment. The attraction of soft power stems not only from its cultural influence or narrative construction, but more fundamentally from audiences’ affective investments in the images of identity that it produces. The empirical import of these ideas is offered in an analysis of the construction of American attraction in the war on terror

Detection of distinct power spectra in soft and hard X-ray bands in the hard state of GRS 1915+105

The well-known black hole X-ray binary GRS 1915+105 is a unique source in the sense that it cannot be classified within the standard picture of black hole binary states. In this work we study archival XMM-Newton observations taken between 2003 and 2004 of the \c{hi} variability class of GRS 1915+105, which corresponds to the hard state in the standard black hole X-ray binary state classification. The crucial point of our study is that by using XMM-Newton data we can access the variability below 3 keV, an energy range that is not covered with RXTE. We focus on the study of the power spectral shape in the soft and hard X-ray band, in light of our work done with Swift on MAXI J1659-152. In the hard band (above 2.5 keV) power density spectra consist of band-limited noise and quasi-periodic oscillations, corresponding to the power spectral shape seen in the hard or intermediate state, while in the soft band the averaged power density spectrum is consistent with a power-law noise, corresponding to the power spectral shape usually seen in the soft state. The coexisting of two different power spectral shapes in the soft and hard band, where the soft band power spectrum is dominated by a power-law noise, is consistent with MAXI J1659-152, and confirms the energy dependence of power spectral states. Our additional spectral analysis shows that the disc component does contribute to the soft band flux. These findings support that the observed black hole power spectral state depends on which spectral component we are looking at, which implies that power spectral analysis is probably a more sensitive method than spectral modeling to trace the emergence of the disc component in the hard or intermediate state.Comment: 9 pages, 5 figures, submitted to MNRA

Understanding the UK's soft power: more than Shakespeare and the Royal Family

Do we understand enough about what soft power is? Gary Rawnsley explains that although the focus has so far been on cultural icons and stories, there is another important aspect to soft power: the actions of the British government. These are seen as a reflection of the values the UK upholds, and so influence opinions overseas. He argues that understanding this dimension of soft power is becoming more urgent as Brexit approaches

Subleading Power Factorization with Radiative Functions

The study of amplitudes and cross sections in the soft and collinear limits allows for an understanding of their all orders behavior, and the identification of universal structures. At leading power soft emissions are eikonal, and described by Wilson lines. Beyond leading power the eikonal approximation breaks down, soft fermions must be added, and soft radiation resolves the nature of the energetic partons from which they were emitted. For both subleading power soft gluon and quark emissions, we use the soft collinear effective theory (SCET) to derive an all orders gauge invariant bare factorization, at both amplitude and cross section level. This yields universal multilocal matrix elements, which we refer to as radiative functions. These appear from subleading power Lagrangians inserted along the lightcone which dress the leading power Wilson lines. The use of SCET enables us to determine the complete set of radiative functions that appear to $\mathcal{O}(\lambda^2)$ in the power expansion, to all orders in $\alpha_s$. For the particular case of event shape observables in $e^+e^-\to$ dijets we derive how the radiative functions contribute to the factorized cross section to $\mathcal{O}(\lambda^2)$.Comment: 62 pages + appendices, many pretty and colorful figures. v2: journal versio

Soft X-ray spectral variations of the narrow line Seyfert l galaxy Markarian 766

The X-ray variability of the narrow-line Seyfert 1 galaxy Markarian 766 is studied using nine ROSAT PSPC data sets. The spectrum is well described by a power law combined with a blackbody (kT ∼ 70 eV) soft excess. Examination of flux ratio changes and variability amplitude in three X-ray bands shows that the power-law component varies continuously on time-scales of ∼ 5000 s and is steeper when it is brighter. In contrast, variability of the soft excess is not detected. Spectral modelling of 31 spectra from different observations and at a range of count rates is also consistent with a picture in which the power law is steeper when it is brighter, and in which the soft-excess component does not vary. The power-law variability can be explained if the power law is produced by variable thermal or non-thermal Comptonization of soft photons. This behaviour is similar to that of Galactic black hole candidates in the low state. The X-ray and multiwavelength properties of Markarian 766 are shown to be very similar to those of other narrow-line Seyfert 1s. This may mean that the rapid X-ray variability seen in other narrow-line Seyfert 1s may also not originate in their strong soft-excess components

Diaspora as soft power a case study of Indian diaspora in the US

Atrás han quedado los días cuando el poder estaba definido por las fuentes militares, es decir, el poder duro. Ahora el poder en términos de ideas, la persuasión definida como poder suave, influye en el mundo. El presente artículo es un intento de estudiar y analizar el poder blando como una herramienta de política exterior y cómo la diáspora india (ID), como un poder blando, ha desempeñado un papel importante en la promoción de la relación bilateral entre la India y los EE. UU.Gone are the days, when power was defined by military sources, in other words, hard power. Now, power in terms of ideas, persuasion, which is defined as soft power, influences the world. The present paper is an attempt to study and analyze soft power as a foreign policy tool, and how Indian Diaspora (ID) as a soft power, has played a role in the promotion of bilateral relationship between India and the US

What Makes Autocracies’ Soft Power Strategies Special? Evidence from Russia and China

The paper problematizes the national soft power strategies of authoritarian states arguing that many of their features stem from those countries’ political regime. In particular, the author focuses on such features as actors involved in soft power policies, the public media’s international and domestic rhetoric, the presence or absence of ideological commitments, strategies’ proactiveness/reactiveness as well as their long- and short-termness. The author presents his argumentation in a fashion similar to what is called theory-building process tracing: first, he shows causal links between an autocratic political regime and each of those features, and then illustrates them with relevant examples taken from case studies and media publications on the soft power strategies of contemporary Russia and China

The puzzle of the soft X-ray excess in AGN: absorption or reflection?

The 2-10 keV continuum of AGN is generally well represented by a single power law. However, at smaller energies the continuum displays an excess with respect to the extrapolation of this power law, called the ''soft X-ray excess''. Until now this soft X-ray excess was attributed, either to reflection of the hard X-ray source by the accretion disk, or to the presence of an additional comptonizing medium, giving a steep spectrum. An alternative solution proposed by Gierlinski and Done (2004) is that a single power law well represents both the soft and the hard X-ray emission and the impression of the soft X-ray excess is due to absorption of a primary power law by a relativistic wind. We examine the advantages and drawbacks of reflection versus absorption models, and we conclude that the observed spectra can be well modeled, either by absorption (for a strong excess), or by reflection (for a weak excess). However the physical conditions required by the absorption models do not seem very realistic: we would prefer an ''hybrid model''.Comment: 4 pages, 3 figures, abstracts SF2A-2005, published by EDP-Sciences Conference Serie