# Talks (non-conference)

 2022-08-2622:25 [PUBDB-2022-04586] Talk (non-conference) Lawrie, C. 4d SCFTs with $a = c$ 2022-08-2622:24 [PUBDB-2022-04585] Talk (non-conference) Lawrie, C. Infinitely-many 4d SCFTs with $a=c$ 2022-08-2622:22 [PUBDB-2022-04584] Talk (non-conference) Lawrie, C. 6d SCFTs and Their Compactifications 2022-08-1911:35 [PUBDB-2022-04511] Talk (non-conference) Vis, J. M. v. d. Baryogenesis and gravitational waves in the electroweak phase transition BCTP Seminar, Bonn UniversityBonn, Bonn University, Germany, 11 Jul 2022   When the temperature of the universe was about 100 GeV, the electroweak phase transition took place. In this process, the electroweak symmetry broke, and the particles of the Standard Model became massive. [...] Restricted: PDF PDF (PDFA); 2022-07-1812:39 [PUBDB-2022-03928] Talk (non-conference) (Invited) Köhler, M. ; Sachs, K. ; Thiele, R. Information Retrieval Summer Student Program, DESYHamburg, DESY, Germany, 19 Jul 2022 - 19 Jul 2022 [10.3204/PUBDB-2022-03928]   Introduction to information retrieval for summer students including a list of selected services of the DESY library OpenAccess: PDF PDF (PDFA) (additional files); 2022-07-0510:21 [PUBDB-2022-03257] Talk (non-conference) Vis, J. M. v. d. Gravitational waves from cosmological phase transitions: Using LISA to probe particle physics Nordita Astrophysics Seminar, NorditaStockholm, Nordita, Sweden, 11 May 2022   Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...] Restricted: PDF PDF (PDFA); 2022-07-0510:18 [PUBDB-2022-03255] Talk (non-conference) (Invited) Vis, J. M. v. d. Gravitational waves from cosmological phase transitions:Using LISA to probe particle physics S@INT Seminar, University of WashingtonSeattle, University of Washington, USA, 5 May 2022   In many extensions of the Standard Model, the electroweak phase transition is first order. Such a phase transition proceeds via the formation and collision of bubbles. [...] Restricted: PDF PDF (PDFA); 2022-07-0510:13 [PUBDB-2022-03253] Talk (non-conference) (Invited) Vis, J. M. v. d. Gravitational waves from cosmological phase transitions: Using LISA to probe particle physics Theory Seminar, University of SiegenSiegen, University of Siegen, Germany, 2 May 2022   In many extensions of the Standard Model, the electroweak phase transition is first order. Such a phase transition proceeds via the formation and collision of bubbles. [...] Restricted: PDF PDF (PDFA); 2022-07-0510:08 [PUBDB-2022-03252] Talk (non-conference) Vis, J. M. v. d. Constraining phase transitions with LISA: Prospects and degeneracies Theoretical Physics Seminar, Université Libre de BruxellesBrussels, Université Libre de Bruxelles, Belgium, 11 Mar 2022   Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...] Restricted: PDF PDF (PDFA); 2022-07-0510:03 [PUBDB-2022-03251] Talk (non-conference) (Invited) Vis, J. M. v. d. Constraining phase transitions with LISA: Prospects and degeneracies Cosmology lunch seminar, University of CambridgeCambridge, University of Cambridge, UK, 7 Feb 2022   Sound waves sourced by bubble collisions during a cosmological first order phase transition can constitute an observable gravitational wave signal. In the standard picture, the gravitational wave spectrum is described in terms of four parameters: the wall velocity and the strength, duration and temperature of the phase transition. [...] Restricted: PDF PDF (PDFA);