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This article revisits the cutting-edge 'capture or kill' debate in the field of IHL, offering a fresh outlook that reconstrues the notion of 'human enhancement of soldiers' from a normative standpoint. After sketching the debate and inquiring into its root causes, the article analyses the interplay between military necessity and humanity, in order to endow the latter with its own content drawing on the notions of military honour and human dignity. Finally, it presents a proposal for the moral education of soldiers during military training.

Cet article revisite le débat moderne du « capturer ou tuer » dans le domaine du droit international humanitaire. Il propose une vision nouvelle qui réinterprète d'un point de vue normatif la notion d'amélioration des capacités humaines à des fins militaires. Après avoir initié le débat et recherché son origine, l'auteur analyse l'interaction entre nécessité militaire et humanité, afin de doter cette dernière de son propre contenu, en se basant sur les notions d'honneur militaire et de dignité humaine. Enfin, l'auteur formule une proposition d'éducation morale des militaires au cours de leur entraînement.

In dit artikel wordt het toonaangevende debat over "gevangennemen of doden" op het gebied van het IHR herbekeken en wordt aan de hand van een nieuw perspectief het begrip 'mensverbetering van soldaten' geherinterpreteerd vanuit een normatief standpunt. Na het debat kort te hebben beschreven en de diepere oorzaken ervan te hebben onderzocht, analyseert het artikel de wisselwerking tussen militaire noodzaak en menselijkheid, om aan dit laatste begrip een eigen inhoud te geven die gebaseerd is op de begrippen militaire eer en menselijke waardigheid. Ten slotte wordt een voorstel gedaan voor de morele opvoeding van soldaten tijdens de militaire opleiding.

El artículo aborda una vez más el afilado debate en torno a "captura o mata" en el ámbito del DIH, ofreciendo una visión renovada que vuelve a construir el concepto de "Realce Humano de los Soldados" desde una nueva perspectiva normativa. Tras examinar los presupuestos del debate e indagar sobre sus causas remotas, el artículo analiza la interacción entre necesidad militar y humanidad, con la finalidad de profundizar en esto último partiendo de la base de los conceptos de honor militar y dignidad humana. Por último, se presenta una propuesta a seguir en la educación moral de los soldados durante el periodo de formación.

Questo articolo rivisita l'innovativo dibattito sul tema della 'Cattura o Uccisione' nel diritto internazionale umanitario, offrendo una nuova prospettiva che ricostruisce il concetto della 'valorizzazione umana dei soldati' da un punto di vista normativo. Dopo aver delineato il dibattito e indagato le sue cause alla radice, l'articolo analizza l'interazione tra necessità militare e umanità, al fine di dotare quest'ultima di elementi propri, attingendo alle nozioni di onore militare e dignità umana. Infine, presenta una proposta per l'educazione morale dei soldati durante l'addestramento militare.

Dieser Artikel nimmt die brandaktuelle "gefangen nehmen oder töten"-Debatte im Bereich des humanitären Völkerrechts erneut unter die Lupe und bietet eine neue Perspektive, die den Begriff "Verbesserung der menschlichen Fähigkeiten für Militärzwecke" aus normativem Standpunkt rekonstruiert. Nach einer Skizzierung der Debatte und einer Untersuchung ihrer Ursachen analysiert der Artikel das Zusammenspiel zwischen militärischer Notwendigkeit und Menschlichkeit, um letzterer einen eigenen Inhalt zu geben, der sich auf die Begriffe militärische Ehre und Menschenwürde stützt. Schließlich legt er einen Vorschlag zur moralischen Erziehung der Soldaten während der militärischen Ausbildung vor.

This article traces the impact of superpowers' foreign aid on India and Pakistan during the early decades of the Cold War. It shows how the American policy-makers have drawn their initial strategies to bring India under the Western fold and later, when the Indian leadership resisted by adopting the foreign policy non-alignment, charted a new approach to keep it at an adequate distance from the Soviet influence—particularly by exploiting its food insecurity and inability to complete the five-year plans. In contrast, the Soviet Union extended project-aid to India which assisted it to build much required large industrial base and attain self-sufficiency in the long run. By adhering to the non-aligned doctrine, India not only managed a negotiable balance with the superpower politics but also extracted considerable benefits for its overall development. On the other hand, aligned Pakistan had shown least enthusiasm with regard to self-sufficiency and pursued policies imbued with militarism which ended up it as a rent-seeking dependent state.

Armano, M., et al. ; We report on the first subpicometer interferometer flown in space. It was part of ESA's Laser Interferometer Space Antenna (LISA) Pathfinder mission and performed the fundamental measurement of the positional and angular motion of two free-falling test masses. The interferometer worked immediately, stably, and reliably from switch on until the end of the mission with exceptionally low residual noise of 32.0-1.7+2.4 fm/Hz, significantly better than required. We present an upper limit for the sensor performance at millihertz frequencies and a model for the measured sensitivity above 200 mHz. ; The Albert-Einstein-Institut acknowledges the support of the German Space Agency, DLR. The work is supported by the Federal Ministry for Economic Affairs and Energy based on a resolution of the German Bundestag (FKZ 50OQ0501 and FKZ 50OQ1601). The French contribution has been supported by the CNES (Accord Specific de projet CNES 1316634/CNRS 103747), the CNRS, the Observatoire de Paris, and the University Paris-Diderot. E. P. and H. I. would also like to acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). The Italian contribution has been supported by Agenzia Spaziale Italiana and Istituto Nazionale di Fisica Nucleare. The Spanish contribution has been supported by Contracts No. AYA2010-15709 (MICINN), No. ESP2013-47637-P, No. ESP2015-67234-P, and No. ESP2017-90084-P (MINECO). Support from AGAUR (Generalitat de Catalunya) Contract No. 2017-SGR-1469 is also acknowledged. M. N. acknowledges support from Fundacion General CSIC (Programa ComFuturo). F. R. acknowledges an FPI contract from MINECO. The Swiss contribution acknowledges the support of the ETH Research Grant No. ETH-05 16-2 and the Swiss Space Office (SSO) via the PRODEX Programme of European Space Agency. L. F. is supported by the Swiss National Science Foundation. The UK groups wish to acknowledge support from the United Kingdom Space Agency (UKSA), the Scottish Universities Physics Alliance (SUPA), the University of Glasgow, the University of Birmingham, and Imperial College London. J. I. T. and J. S. acknowledge the support of the U.S. National Aeronautics and Space Administration (NASA). N. K. is thankful for the support from a CNES Fellowship.

20 pages, 18 figures.-- et al. ; Baryon Acoustic Oscillations (BAOs) provide a "standard ruler" of known physical length, making it one of the most promising probes of the nature of dark energy (DE). The detection of BAOs as an excess of power in the galaxy distribution at a certain scale requires measuring galaxy positions and redshifts. "Transversal" (or "angular") BAOs measure the angular size of this scale projected in the sky and provide information about the angular distance. "Line-of-sight" (or "radial") BAOs require very precise redshifts, but provide a direct measurement of the Hubble parameter at different redshifts, a more sensitive probe of DE. The main goal of this paper is to show that it is possible to obtain photometric redshifts with enough precision (σz) to measure BAOs along the line of sight. There is a fundamental limitation as to how much one can improve the BAO measurement by reducing σz . We show that σz ~ 0.003(1 + z) is sufficient: a much better precision will produce an oversampling of the BAO peak without a significant improvement on its detection, while a much worse precision will result in the effective loss of the radial information. This precision in redshift can be achieved for bright, red galaxies, featuring a prominent 4000 Å break, by using a filter system comprising about 40 filters, each with a width close to 100 Å, covering the wavelength range from ~4000 to ~8000 Å, supplemented by two broad-band filters similar to the Sloan Digital Sky Survey u and z bands. We describe the practical implementation of this idea, a new galaxy survey project, Physics of the Accelerating Universe (PAU): http://www.ice.cat/pau, to be carried out with a telescope/camera combination with an etendue about 20 m2 deg2, equivalent to a 2 m telescope equipped with a 6 deg2 field of view camera, and covering 8000 deg2 in the sky in four years. We expect to measure positions and redshifts for over 14 million red, early-type galaxies with L > L* and i(AB) ~ 10–3 Mpc–3 h3 galaxies within the 9 Gpc3 h–3 volume to be sampled by our survey, ensuring that the error in the determination of the BAO scale is not limited by shot noise. By itself, such a survey will deliver precisions of order 5% in the dark-energy equation of state parameter w, if assumed constant, and can determine its time derivative when combined with future cosmic microwave background measurements. In addition, PAU will yield high-quality redshift and low-resolution spectroscopy for hundreds of millions of other galaxies, including a very significant high-redshift population. The data set produced by this survey will have a unique legacy value, allowing a wide range of astrophysical studies. ; This work was carried out in the framework of the PAU Consolider Collaboration, supported in part by the Spanish Ministry of Education and Science (MEC) through the Consolider Ingenio-2010 program, under project CSD2007-00060 "Physics of the Accelerating Universe (PAU)". Additional support comes from the Barcelona Supercomputer Center, as well as from the European Commission, the Spanish High Council for Scientific Research (CSIC), and the regional governments of Andalusia, Aragon, Catalonia, Madrid, and Valencia. ; Peer reviewed