Rivalry in International Relations: A Mimetic Approach to the Case of the Rivalry in Northern Ireland (1963-2020)

This PhD dissertation explores how rivalry, understood as a protracted intractable conflict, emerges, and develops. It takes issue with current approaches to rivalry in International Relations (IR) and Peace and Conflict Studies (P&CS) to advance an alternative, innovative, and interdisciplinary Mimetic Rivalry Framework (MRF) that draws on René Girard’s Mimetic Theory. In contrast to existing research on rivalry in IR and P&CS, the MRF argues for the distinctive nature of rivalry vis-àvis other forms of conflict. It challenges several common assumptions – such as the rationalist assumption on human agency, the materialist assumption on rivalry emergence, and the reification of identity as a difference marker – while embracing complexity, relationality, and mimeticism. Informed by several multi-disciplinary theories – namely, Clyde Kluckhohn’s Social Value Theory, Gabriel Tarde’s Theory of Value, and Leon Festinger’s Social-Comparison Theory – the MRF offers a set of indicators able to empirically trace the stages leading an inter-group dyad from a state of non-competition to the stage of rivalry emergence and, finally, to a full-fledged rivalry. To test the empirical robustness of the framework, the thesis then investigates the rivalry between Republicans/Nationalists/Catholics and Loyalists/Unionists/Protestants in Northern Ireland as it developed around two intractable issues: that of territory (1964-1998), and that of language (1998-2020). In contrast to the existing literature, the MRF shows that the atypical intractability of the Northern Ireland rivalry is a product of the extreme similarity of desires, rather than of their difference. Because intractable difference is an artefact of mimetic rivalry, this dissertation argues that the politics in Northern Ireland remains prone to rivalry’s chronic intractability unless the underlying mimetic matrix of mutually exclusive identities is unveiled and challenged. Finally, the thesis suggests that recent developments in communal relations in the Irish language community indicate that the Irish language has the potential for enabling communal reconciliation

Photospheric activity, rotation, and star-planet interaction of the planet-hosting star CoRoT-6

The CoRoT satellite has recently discovered a hot Jupiter that transits across the disc of a F9V star called CoRoT-6 with a period of 8.886 days. We model the photospheric activity of the star and use the maps of the active regions to study stellar differential rotation and the star-planet interaction. We apply a maximum entropy spot model to fit the optical modulation as observed by CoRoT during a uninterrupted interval of about 140 days. Photospheric active regions are assumed to consist of spots and faculae in a fixed proportion with solar-like contrasts. Individual active regions have lifetimes up to 30-40 days. Most of them form and decay within five active longitudes whose different migration rates are attributed to the stellar differential rotation for which a lower limit of \Delta \Omega / \Omega = 0.12 \pm 0.02 is obtained. Several active regions show a maximum of activity at a longitude lagging the subplanetary point by about 200 degrees with the probability of a chance occurrence being smaller than 1 percent. Our spot modelling indicates that the photospheric activity of CoRoT-6 could be partially modulated by some kind of star-planet magnetic interaction, while an interaction related to tides is highly unlikely because of the weakness of the tidal force.Comment: 9 pages, 7 figures, accepted to Astronomy & Astrophysic

Event generator to construct cross sections for the multiphonon excitation of a set of collective vibrational modes

The construction of differential cross sections as a function of excitation energy for systems with a collection of low- and high-lying intrinsic vibrational modes has been attempted in the past. A prescription is proposed that simplifies the implementation of such calculation schemes with a remarkable reduction in computational time.Comment: 6 pages, 3 figures, to be published in Phys. Rev.

Mimetic rivalry in practice: The case of Kosovo

In this article, we advance a framework that highlights the relational nature of rivalry emergence and its ongoing manifestations, before illustrating this framework in practice through an analysis of the rivalry between Serbs and Albanians over the issue of Kosovo. We argue that the locus of rivalry lies in the inherently social character of human desire and the destructive reciprocity elicited by human mimetic behaviour. The manner in which rivals portray their plight, and legitimise their cause, is, we argue, a function of their desire to acquire that which they imagine the other has. As such, rather than adhering to the conventional view that rivalries are characterised by difference, we argue that rivals share a set of common goals/desires. Thus, though rivalries are characterised by mutual antipathy – and the attendant devotion to constructing self-serving myths – this is but a superficial manifestation of an underlying mimetic dynamic. To focus only on how myths are constructed and instrumentally employed, is not sufficient when seeking to explain the persistence of rivalries. Rather, we must understand the underlying desires the respective rivals seek to fulfill through the proliferation of these myths if we are to truly understand the nature of the rivalry

Photospheric activity, rotation and magnetic interaction in LHS 6343 A

Context. The Kepler mission has recently discovered a brown dwarf companion transiting one member of the M4V+M5V visual binary system LHS 6343 AB with an orbital period of 12.71 days. Aims. The particular interest of this transiting system lies in the synchronicity between the transits of the brown dwarf C component and the main modulation observed in the light curve, which is assumed to be caused by rotating starspots on the A component. We model the activity of this star by deriving maps of the active regions that allow us to study stellar rotation and the possible interaction with the brown dwarf companion. Methods. An average transit profile was derived, and the photometric perturbations due to spots occulted during transits are removed to derive more precise transit parameters. We applied a maximum entropy spot model to fit the out-of-transit optical modulation as observed by Kepler during an uninterrupted interval of 500 days. It assumes that stellar active regions consist of cool spots and bright faculae whose visibility is modulated by stellar rotation. Results. Thanks to the extended photometric time series, we refine the determination of the transit parameters and find evidence of spots that are occulted by the brown dwarf during its transits. The modelling of the out-of-transit light curve of LHS 6343 A reveals several starspots rotating with a slightly longer period than the orbital period of the brown dwarf, i.e., 13.13 +- 0.02 days. No signature attributable to differential rotation is observed. We find evidence of a persistent active longitude on the M dwarf preceding the sub- companion point by 100 deg and lasting for at least 500 days. This can be relevant for understanding how magnetic interaction works in low-mass binary and star-planet systems.Comment: 14 pages, 16 figure

Activity cycles in members of young loose stellar associations

Magnetic cycles have been detected in tens of solar-like stars. The relationship between the cycle properties and global stellar parameters is not fully understood yet. We searched for activity cycles in 90 solar-like stars with ages between 4 and 95 Myr aiming to investigate the properties of activity cycles in this age range. We measured the length $P_{ cyc}$ of a given cycle by analyzing the long-term time-series of three activity indexes. For each star, we computed also the global magnetic activity index that is proportional to the amplitude of the rotational modulation and is a proxy of the mean level of the surface magnetic activity. We detected activity cycles in 67 stars. Secondary cycles were also detected in 32 stars. The lack of correlation between $P_{ cyc}$ and $P_{ rot}$ suggest that these stars belong to the Transitional Branch and that the dynamo acting in these stars is different from the solar one. This statement is also supported by the analysis of the butterfly diagrams. We computed the Spearman correlation coefficient $r_{ S}$ between $P_{ cyc}$, and different stellar parameters. We found that $P_{ cyc}$ is uncorrelated with all the investigated parameters. The index is positively correlated with the convective turn-over time-scale, the magnetic diffusivity time-scale $\tau_{ diff}$, and the dynamo number $D_{ N}$, whereas it is anti-correlated with the effective temperature $T_{ eff}$, the photometric shear $\Delta\Omega_{\rm phot}$ and the radius $R_{ C}$ at which the convective zone is located. We found that $P_{ cyc}$ is about constant and that decreases with the stellare age in the range 4-95 Myr. We investigated the magnetic activity of AB Dor A by merging ASAS time-series with previous long-term photometric data. We estimated the length of the AB Dor A primary cycle as $P_{ cyc} = 16.78 \pm 2 \rm yr$.Comment: 19 pages , 15 figures, accepte

Determination of rotation periods in solar-like stars with irregular sampling: the Gaia case

We present a study on the determination of rotation periods (P) of solar-like stars from the photometric irregular time-sampling of the ESA Gaia mission, currently scheduled for launch in 2013, taking into account its dependence on ecliptic coordinates. We examine the case of solar-twins as well as thousands of synthetic time-series of solar-like stars rotating faster than the Sun. In the case of solar twins we assume that the Gaia unfiltered photometric passband G will mimic the variability of the total solar irradiance (TSI) as measured by the VIRGO experiment. For stars rotating faster than the Sun, light-curves are simulated using synthetic spectra for the quiet atmosphere, the spots, and the faculae combined by applying semi-empirical relationships relating the level of photospheric magnetic activity to the stellar rotation and the Gaia instrumental response. The capabilities of the Deeming, Lomb-Scargle, and Phase Dispersion Minimisation methods in recovering the correct rotation periods are tested and compared. The false alarm probability (FAP) is computed using Monte Carlo simulations and compared with analytical formulae. The Gaia scanning law makes the rate of correct detection of rotation periods strongly dependent on the ecliptic latitude (beta). We find that for P ~ 1 d, the rate of correct detection increases with ecliptic latitude from 20-30 per cent at beta ~ 0{\deg} to a peak of 70 per cent at beta=45{\deg}, then it abruptly falls below 10 per cent at beta > 45{\deg}. For P > 5 d, the rate of correct detection is quite low and for solar twins is only 5 per cent on average.Comment: 12 pages, 18 figures, accepted by MNRA