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Postadress Box 192, 221 00 Lund Besöksadress LUX (Hus B), Helgonavägen 3 E-post carita.lundmark@kansliht.lu.se Kansl i HT Car i ta Lundmark, u tb i ldn ings ledare Agnes Malmgren, u tb i ldn ings ledare Kvalitetssäkring och kvalitetsutveckling av utbildning på grundnivå, avancerad nivå och forskarnivå 2024 Denna rapport beskriver Humanistiska och teologiska fakulteternas (HT) kvalitetssäkring och
C:/Report_050125/REPORT.dvi Department of Mechanical Engineering Solid Mechanics ISRN LUTFD2/TFHF–05/5111–SE(1–156) EVALUATING THE 3DM MODEL - AN EXPERIMENTAL AND FINITE ELEMENT STUDY Master’s Dissertation by Oscar Elison and Lars Hansson Supervisors Johan Tryding, Tetra Pak Magnus Just, Tetra Pak Anders Harrysson, Div. of Solid Mechanics Matti Ristinmaa, Div. of Solid Mechanics Copyright c© 2005
https://www.solid.lth.se/fileadmin/hallfasthetslara/utbildning/examensarbete/TFHF5111.pdf - 2026-05-25
6 Vocabularies of Reason 2025 Pufendorf Lectures Lund University Lecture II Logic and the Structure of Reasons I. Three Versions of a Basic Discursive Bipolarity In my first lecture I introduced the concept of reason relations of implication and incompatibility, motivated by Harman’s argument for the need to distinguish such rational relations from inferential practices. I showed that such consequ
https://www.fil.lu.se/fileadmin/user_upload/pufendorf/Files/Lecture_2.pdf - 2026-05-26
1 23 Biosemiotics ISSN 1875-1342 Volume 7 Number 3 Biosemiotics (2014) 7:405-427 DOI 10.1007/s12304-014-9200-5 The Role of Image Schemas and Superior Psychic Faculties in Zoosemiosis José Manuel Ureña Gómez-Moreno JoséManuel Nota Anunciado en: http://www.springerlink.com/openurl.asp?genre=article&id=doi:10.1007/s12304-014-9200-5 1 23 Your article is protected by copyright and all rights are held e
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Framsida Sthlm copy WPSS WORKING PAPERS IN SCANDINAVIAN SYNTAX June 2018 Issue 100 Working Papers in Scandinavian Syntax is an electronic publication for current articles relating to the study of Scandinavian syntax. The articles appearing herein are previously unpublished reports of ongoing research activities and may subsequently appear, revised or unrevised, in other publications. The WPSS home
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Guidelines for degree projects in the first and second cycles Decision by the Working Committee of the Faculty Board on 22 June 2022 Date of entry into force: 1 September 2022 Reg. no STYR 2021/1863 Postal address Box 192, 22100 LUND Visiting address LUX Helgonavägen 3, LUND Homepage http://www.ht.lu.se Contents Introduction .........................................................................
Ninth International Conference on Hunting and Gathering Societies 1 In Defense of the Nature/Culture Distinction: Why Environmental Anthropology Can Neither Dispense With, Nor be Reduced to, Semiotics Alf Hornborg Human Ecology Division, Lund University, Finngatan 16, 223 62 Lund, Sweden Phone 46-46-2223113, Fax 46-46-2223695, Email alf.hornborg@humecol.lu.se Abstract This paper argues against the
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Postadress Box 192, 221 00 Lund Besöksadress LUX (Hus B), Helgonavägen 3 E-post carita.lundmark@kansliht.lu.se Uppföljning av HT-fakulteternas kvalitetsdialoger på grundnivå och avancerad nivå 2023 I mars månad varje år genomför HT-fakulteterna kvalitetsdialoger1 med institutionerna och Språk- och litteraturcentrums (SOL) sektioner,2 samt med HT- biblioteken.3 Dialogerna har en tematisk inriktning
We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration less than or similar to 1 s over the frequency ba
We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009, and October 20, 2010. We searched for signals from binaries with total mass between 2 and 25M(circle dot); this includes binary neutron stars, binary black holes, and binaries consisting of a black hole and neutron star. The detectors were sensitive to systems up t
Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational-wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model selection are crucial analysis steps for any detection candidate events. Detailed models of the anticipated waveforms enable inference on several param
This paper presents results of an all-sky search for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative range of similar to[-20, 1.1] x 10(-10) Hz s(-1) for the fifth LIGO science run (S5). The search uses a noncoherent Hough-transform method to combine the information from coherent searches on time scales of about one day. Because these searches are ve
A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical origin. This background is a target for the current generation of ground-based detectors. In this article we present the first joint search for a stochastic background using data from the LIGO and Virgo interferometers.
We present the results of a weakly modeled burst search for gravitational waves from mergers of nonspinning intermediate mass black holes in the total mass range 100-450 M-circle dot and with the component mass ratios between 1: and 4:1. The search was conducted on data collected by the LIGO and Virgo detectors between November of 2005 and October of 2007. No plausible signals were observed by the
Between 2007 and 2010 Virgo collected data in coincidence with the LIGO and GEO gravitational-wave (GW) detectors. These data have been searched for GWs emitted by cataclysmic phenomena in the universe, by non-axisymmetric rotating neutron stars or from a stochastic background in the frequency band of the detectors. The sensitivity of GW searches is limited by noise produced by the detector or its
Infinite Lotteries, Uniform Probability, and Expected Utility (February 27, 1997) Standard Decision Theory Corrected: Assessing Options When Probability is Infinitely and Uniformly Spread* Peter Vallentyne Department of Philosophy, University of Missouri-Columbia Originally published in Synthese 122 (2000): 261-290. © 2000 Kluwer Academic Publishers. Reprinted (with two small corrections) with per
https://www.fil.lu.se/hommageawlodek/site/papper/VallentynePeter.pdf - 2026-05-26
1 El estado de derecho Guía para políticos 2 Copyright © El Instituto Raoul Wallenberg de Derechos Humanos y Derecho Internacional Humanitario y el Instituto de La Haya para la Internacionalización de la Ley 2012 ISBN: 978-91-86910-89-1 Cualquier forma de reproducción, distribución, comunicación pública o trans- formación de esta obra sólo puede ser realizada con la autorización previa de sus titu
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Guidelines and management rules for the establishment, revision and discontinuation of degree programmes in the first and second cycles Decision by the faculty board’s working committee on 21 October 2020 Valid from 18 January 2021 Reg. no STYR 2020/666 Postal address Box 192, 22100 LUND Visiting address LUX Helgonavägen 3, LUND Email http://www.ht.lu.se/person/LisaHetherington/ Homepage http://ww
ANALYTICITY, MODALITY, AND GENERAL TERMS Kathrin Glüer Department of Philosophy Stockholm University kathrin.gluer@philosophy.su.se Peter Pagin Department of Philosophy Stockholm University peter.pagin@philosophy.su.se ABSTRACT: In his recent paper ‘Analyticity: An Unfinished Business in Possible-World Semantics’ (Rabinowicz 2006), Wlodek Rabinowicz takes on the task of providing a satisfactory de
https://www.fil.lu.se/hommageawlodek/site/papper/Gluer&Pagin.pdf - 2026-05-26
We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20, 20)M-circle dot coalescence was 300 Mpc. No gravitational wave signals w
