Le revenu minimum garanti et les problèmes juridiques de sa mise en oeuvre

L'évolution de la protection sociale, au Canada et au Québec, en direction d'un revenu minimum garanti se heurte, en l'état actuel des choses, à de formidables obstacles. Ces obstacles tiennent à la fragmentation et à complexité du système de sécurité sociale, à la souplesse et à la malléabilité que lui confère le recours à quatre techniques différentes de sécurité sociale, et surtout aux difficultés d'ordre constitutionnel et politique découlant principalement du partage des compétences législatives. Ce constat s'appuie sur une analyse du cadre juridique actuel de la protection sociale de base. Celle-ci comprend notamment l'assistance sociale, dont le cadre actuel au Québec est la Loi sur la sécurité du revenu. Parmi les principaux problèmes juridiques que suscite ou suscitera vraisemblablement cette loi, sont examinés : l'incidence des droits fondamentaux, celle du Régime d'assistance publique du Canada, et les exigences de la légalité administrative. Sont ensuite brièvement analysées les autres composantes de la protection sociale de base : les prestations de sécurité de la vieillesse et les prestations familiales. Le texte rappelle ensuite les caractéristiques des quatre techniques de sécurité sociale pratiquées au Canada et au Québec : l'assurance sociale, les prestations universelles, l'assistance sociale et la garantie de revenu. Ce rappel, qui vise à mettre en relief l'effet de complémentarité obtenu par le recours aux quatre techniques, débouche sur la critique de leurs inconvénients respectifs, qui dans aucun cas ne semblent en justifier l'abandon aux yeux du public et des dirigeants politiques. Enfin, le texte revient sur les tentatives de mise au point d'une formule de revenu minimum garanti pendant les années 1970. Il conclut de l'échec de ces tentatives, entreprises pourtant dans un climat politique et économique relativement favorable, qu'il n'y a pas lieu d'escompter l'aboutissement prochain de propositions nouvelles dans le même sens.Major obstacles currently hinder the development of a guaranteed minimum income (GMI) out of the existing Canadian and Quebec social security system. Obstacles flow from the system's fragmentation and complexity ; others stem from the very advantages of the system, namely the flexibility and comprehensiveness offered by the combination of four different techniques of social security : above all, obstacles to any move towards GMI are built in the constitutional and political constraints of federalism. This point is grounded on an analysis of the existing legal framework of basic-level social security in Canada. This mainly involves social assistance schemes in the provinces. The Quebec Income Security Act of 1988 is a fairly typical example of these. The paper surveys some of the major actual or foreseeable legal issues arising out ofthat scheme : its relationship to fundamental rights, to the Canada Assistance Plan and to the requirements of the rule of law in administrative action. Other components of basic-level social security — Old Age Security and family benefits — are then briefly outlined. The paper then proceeds to discuss the specific features of each of the four techniques implemented in the Canada and Quebec social security system : social insurance, universal benefits, social assistance and guaranteed income. The discussion brings out the complementary relationship between the four techniques, as well as their respective drawbacks and concludes that in the eyes of the general public and political leaders, the later do not justify abandoning any of the four. Finally, the paper goes back over the intergovernmental negotiations on GMI during the 1970s. The unfruitfulness of these negotiations, in spite of an initially favourable political and economic climate, suggests that current conditions are unlikely to favour early progress towards a GMI scheme

A generic frequency dependence for the atmospheric tidal torque of terrestrial planets

Thermal atmospheric tides have a strong impact on the rotation of terrestrial planets. They can lock these planets into an asynchronous rotation state of equilibrium. We aim at characterizing the dependence of the tidal torque resulting from the semidiurnal thermal tide on the tidal frequency, the planet orbital radius, and the atmospheric surface pressure. The tidal torque is computed from full 3D simulations of the atmospheric climate and mean flows using a generic version of the LMDZ general circulation model (GCM) in the case of a nitrogen-dominated atmosphere. Numerical results are discussed with the help of an updated linear analytical framework. Power scaling laws governing the evolution of the torque with the planet orbital radius and surface pressure are derived. The tidal torque exhibits i) a thermal peak in the vicinity of synchronization, ii) a resonant peak associated with the excitation of the Lamb mode in the high frequency range, and iii) well defined frequency slopes outside these resonances. These features are well explained by our linear theory. Whatever the star-planet distance and surface pressure, the torque frequency spectrum -- when rescaled with the relevant power laws -- always presents the same behaviour. This allows us to provide a single and easily usable empirical formula describing the atmospheric tidal torque over the whole parameter space. With such a formula, the effect of the atmospheric tidal torque can be implemented in evolutionary models of the rotational dynamics of a planet in a computationally efficient, and yet relatively accurate way.Comment: Accepted for publication in Astronomy & Astrophysics, 23 pages, 9 figure

Strategies as Resource Terms, and Their Categorical Semantics

As shown by Tsukada and Ong, simply-typed, normal and η-long resource terms correspond to plays in Hyland-Ong games, quotiented by Melliès' homotopy equivalence. Though inspiring, their proof is indirect, relying on the injectivity of the relational model {w.r.t.} both sides of the correspondence - in particular, the dynamics of the resource calculus is taken into account only via the compatibility of the relational model with the composition of normal terms defined by normalization. In the present paper, we revisit and extend these results. Our first contribution is to restate the correspondence by considering causal structures we call augmentations, which are canonical representatives of Hyland-Ong plays up to homotopy. This allows us to give a direct and explicit account of the connection with normal resource terms. As a second contribution, we extend this account to the reduction of resource terms: building on a notion of strategies as weighted sums of augmentations, we provide a denotational model of the resource calculus, invariant under reduction. A key step - and our third contribution - is a categorical model we call a resource category, which is to the resource calculus what differential categories are to the differential λ-calculus

Cosmology with the Laser Interferometer Space Antenna

This work is partly supported by: A.G. Leventis Foundation; Academy of Finland Grants 328958 and 345070; Alexander S. Onassis Foundation, Scholarship ID: FZO 059-1/2018-2019; Amaldi Research Center funded by the MIUR program “Dipartimento di Eccellenza” (CUP: B81I18001170001); ASI Grants No. 2016-24-H.0 and No. 2016-24-H.1-2018; Atracción de Talento Grant 2019-T1/TIC-15784; Atracción de Talento contract no. 2019-T1/TIC-13177 granted by the Comunidad de Madrid; Ayuda ‘Beatriz Galindo Senior’ by the Spanish ‘Ministerio de Universidades’, Grant BG20/00228; Basque Government Grant (IT-979-16); Belgian Francqui Foundation; Centre national d’Etudes spatiales; Ben Gurion University Kreitman Fellowship, and the Israel Academy of Sciences and Humanities (IASH) & Council for Higher Education (CHE) Excellence Fellowship Program for International Postdoctoral Researchers; Centro de Excelencia Severo Ochoa Program SEV-2016-0597; CERCA program of the Generalitat de Catalunya; Cluster of Excellence “Precision Physics, Fundamental Interactions, and Structure of Matter” (PRISMA+ EXC 2118/1); Comunidad de Madrid, Contrato de Atracción de Talento 2017-T1/TIC-5520; Czech Science Foundation GAČR, Grant No. 21-16583M; Delta ITP consortium; Department of Energy under Grant No. DE-SC0008541, DE-SC0009919 and DE-SC0019195; Deutsche Forschungsgemeinschaft (DFG), Project ID 438947057; Deutsche Forschungsgemeinschaft under Germany’s Excellence Strategy - EXC 2121 Quantum Universe - 390833306; European Structural and Investment Funds and the Czech Ministry of Education, Youth and Sports (Project CoGraDS - CZ.02.1.01/0.0/0.0/15 003/0000437); European Union’s H2020 ERC Consolidator Grant “GRavity from Astrophysical to Microscopic Scales” (Grant No. GRAMS-815673); European Union’s H2020 ERC, Starting Grant Agreement No. DarkGRA-757480; European Union’s Horizon 2020 programme under the Marie Sklodowska-Curie Grant Agreement 860881 (ITN HIDDeN); European Union’s Horizon 2020 Research and Innovation Programme Grant No. 796961, “AxiBAU” (K.S.); European Union’s Horizon 2020 Research Council grant 724659 MassiveCosmo ERC-2016-COG; FCT through national funds (PTDC/FIS-PAR/31938/2017) and through project “BEYLA – BEYond LAmbda” with Ref. Number PTDC/FIS-AST/0054/2021; FEDER-Fundo Europeu de Desenvolvimento Regional through COMPETE2020 - Programa Operacional Competitividade e Internacionalização (POCI-01-0145-FEDER-031938) and research Grants UIDB/04434/2020 and UIDP/04434/2020; Fondation CFM pour la Recherche in France; Foundation for Education and European Culture in Greece; French ANR project MMUniverse (ANR-19-CE31-0020); FRIA Grant No.1.E.070.19F of the Belgian Fund for Research, F.R.S.-FNRS Fundação para a Ciência e a Tecnologia (FCT) through Contract No. DL 57/2016/CP1364/CT0001; Fundação para a Ciência e a Tecnologia (FCT) through Grants UIDB/04434/2020, UIDP/04434/2020, PTDC/FIS-OUT/29048/2017, CERN/FIS-PAR/0037/2019 and “CosmoTests – Cosmological tests of gravity theories beyond General Relativity” CEECIND/00017/2018; Generalitat Valenciana Grant PROMETEO/2021/083; Grant No. 758792, project GEODESI; Government of Canada through the Department of Innovation, Science and Economic Development and Province of Ontario through the Ministry of Colleges and Universities; Grants-in-Aid for JSPS Overseas Research Fellow (No. 201960698); I+D Grant PID2020-118159GB-C41 of the Spanish Ministry of Science and Innovation; INFN iniziativa specifica TEONGRAV; Israel Science Foundation (Grant No. 2562/20); Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Nos. 20H01899 and 20H05853; IFT Centro de Excelencia Severo Ochoa Grant SEV-2; Kavli Foundation and its founder Fred Kavli; Minerva Foundation; Ministerio de Ciencia e Innovacion Grant PID2020-113644GB-I00; NASA Grant 80NSSC19K0318; NASA Hubble Fellowship grants No. HST-HF2-51452.001-A awarded by the Space Telescope Science Institute with NASA contract NAS5-26555; Netherlands Organisation for Science and Research (NWO) Grant Number 680-91-119; new faculty seed start-up grant of the Indian Institute of Science, Bangalore, the Core Research Grant CRG/2018/002200 of the Science and Engineering; NSF Grants PHY-1820675, PHY-2006645 and PHY-2011997; Polish National Science Center Grant 2018/31/D/ST2/02048; Polish National Agency for Academic Exchange within the Polish Returns Programme under Agreement PPN/PPO/2020/1/00013/U/00001; Pró-Reitoria de Pesquisa of Universidade Federal de Minas Gerais (UFMG) under Grant No. 28359; Ramón y Cajal Fellowship contract RYC-2017-23493; Research Project PGC2018-094773-B-C32 [MINECO-FEDER]; Research Project PGC2018-094773-B-C32 [MINECO-FEDER]; ROMFORSK Grant Project. No. 302640; Royal Society Grant URF/R1/180009 and ERC StG 949572: SHADE; Shota Rustaveli National Science Foundation (SRNSF) of Georgia (Grant FR/18-1462); Simons Foundation/SFARI 560536; SNSF Ambizione grant; SNSF professorship Grant (No. 170547); Spanish MINECO’s “Centro de Excelencia Severo Ochoa” Programme Grants SEV-2016-0597 and PID2019-110058GB-C22; Spanish Ministry MCIU/AEI/FEDER Grant (PGC2018-094626-B-C21); Spanish Ministry of Science and Innovation (PID2020-115845GB-I00/AEI/10.13039/501100011033); Spanish Proyectos de I+D via Grant PGC2018-096646-A-I00; STFC Consolidated Grant ST/T000732/1; STFC Consolidated Grants ST/P000762/1 and ST/T000791/1; STFC Grant ST/S000550/1; STFC Grant ST/T000813/1; STFC Grants ST/P000762/1 and ST/T000791/1; STFC under the research Grant ST/P000258/1; Swiss National Science Foundation (SNSF), project The Non-Gaussian Universe and Cosmological Symmetries, Project Number: 200020-178787; Swiss National Science Foundation Professorship Grants No. 170547 and No. 191957; SwissMap National Center for Competence in Research; “The Dark Universe: A Synergic Multi-messenger Approach” Number 2017X7X85K under the MIUR program PRIN 2017; UK Space Agency; UKSA Flagship Project, Euclid.The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.Atracción de Talento 2019-T1/TIC-13177Centro de Excelencia Severo Ochoa Program EXC 2118/1, SEV-2016-0597Contrato de Atracción de Talento 2017-T1/TIC-5520European Union’s H2020 ERC GRAMS-815673European Union’s Horizon 2020 Research Council 724659 MassiveCosmo ERC-2016-COGEuropean Union’s Horizon 2020 programme 860881, ITN HIDDeNIFT Centro de Excelencia Severo OchoaSpanish Ministry MCIU PGC2018-094626-B-C21, PGC2018-096646-A-I00, PID2020-115845GB-I00/AEI/10.13039/501100011033Horizon 2020 Framework Programme 796961 H2020Comunidad de MadridEusko Jaurlaritza IT-979-16Ministerio de Economía y Competitividad 302640 MINECOGeneralitat Valenciana 758792, PROMETEO/2021/083 GVAMinisterio de Ciencia e Innovación PID2020-113644GB-I00 MICINNMinisterio de Universidades BG20/00228 MIUEuropean Union’s H2020 ERC, DarkGRA-75748

Cosmic string bursts in LISA

Cosmic string cusps are sources of short-lived, linearly polarised gravitational wave bursts which can be searched for in gravitational wave detectors. We assess the capability of LISA to detect these bursts using the latest LISA configuration and operational assumptions. For such short bursts, we verify that LISA can be considered as ``frozen", namely that one can neglect LISA's orbital motion. We consider two models for the network of cosmic string loops, and estimate that LISA should be able to detect 1-3 bursts per year assuming a string tension $G\mu \approx 10^{-11} - 10^{-10.5}$ and detection threshold $\rm{SNR} \ge 20$. Non-detection of these bursts would constrain the string tension to $G\mu\lesssim 10^{-11}$ for both models.Comment: 6 page

Transitions - Note 2

Note complète ; Résumé ; Capsule 2 : L'accès inégal des influence des « EPG » à l'éducation postsecondair

Thermal tides in neutrally stratified atmospheres: Revisiting the Earth's Precambrian rotational equilibrium

Rotational dynamics of the Earth, over geological timescales, have profoundly affected local and global climatic evolution, probably contributing to the evolution of life. To better retrieve the Earth's rotational history, and motivated by the published hypothesis of a stabilized length of day during the Precambrian, we examine the effect of thermal tides on the evolution of planetary rotational motion. The hypothesized scenario is contingent upon encountering a resonance in atmospheric Lamb waves, whereby an amplified thermotidal torque cancels the opposing torque of the oceans and solid interior, driving the Earth into a rotational equilibrium. With this scenario in mind, we construct an ab initio model of thermal tides on rocky planets describing a neutrally stratified atmosphere. The model takes into account dissipative processes with Newtonian cooling and diffusive processes in the planetary boundary layer. We retrieve from this model a closed-form solution for the frequency-dependent tidal torque which captures the main spectral features previously computed using 3D general circulation models. In particular, under longwave heating, diffusive processes near the surface and the delayed thermal response of the ground prove to be responsible for attenuating, and possibly annihilating, the accelerating effect of the thermotidal torque at the resonance. When applied to the Earth, our model prediction suggests the occurrence of the Lamb resonance in the Phanerozoic, but with an amplitude that is insufficient for the rotational equilibrium. Interestingly, though our study was motivated by the Earth's history, the generic tidal solution can be straightforwardly and efficiently applied in exoplanetary settings.Comment: 20 pages (+14 for appendices), 6 figure

Can one hear supercontinents in the tides of ocean planets?

Recent observations and theoretical progress made about the history of the Earth-Moon system suggest that tidal dissipation in oceans primarily drives the long term evolution of orbital systems hosting ocean planets. Particularly, they emphasise the key role played by the geometry of land-ocean distributions in this mechanism. However, the complex way continents affect oceanic tides still remains to be elucidated. In the present study, we investigate the impact of a single supercontinent on the tidal response of an ocean planet and the induced tidally dissipated energy. The adopted approach is based on the linear tidal theory. By simplifying the continent to a spherical cap of given angular radius and position on the globe, we proceed to a harmonic analysis of the whole planet's tidal response including the coupling with the solid part due to ocean loading and self-attraction variations. In this framework, tidal flows are formulated analytically in terms of explicitly defined oceanic eigenmodes, as well as the resulting tidal Love numbers, dissipated power, and torque. The analysis highlights the symmetry breaking effect of the continent, which makes the dependence of tidal quantities on the tidal frequency become highly irregular. The metric introduced to quantify this continentality effect reveals abrupt transitions between polar and non-polar configurations, and between small-sized and medium-sized continents. Additionally, it predicts that a continent similar to South America or smaller (30{\deg}-angular radius) does not alter qualitatively the tidal response of a global ocean whatever its position on the planet.Comment: 35 pages, 13 figures, 5 tables. Accepted for publication in Astronomy & Astrophysic

Transitions Note 2 : Les étudiants de première génération : un concept prometteur? /

Note complète ; Résumé ; Capsule ; Full text