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ORIGINS annual Science Meeting
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Europe/Berlin
Description
The Excellence Cluster ORIGINS hosts their annual Science Week this year at beautiful Kloster Seeon in Upper Bavaria.
The agenda will include overview and science highlight talks from our research units, connectors and infrastructures, our annual General Assembly, PhD Awards talks and Laudations, Seed Money posters and a new election of cluster coordinators as well as ORIGINS 2 planning sessions.
Scientific Organization Committee: Dieter Braun, Andreas Burkert, Barbara Ercolano, Laura Fabbietti, Stephan Paul, Petra Schwille and Jochen Weller
Science Manager
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12:00 PM
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1:30 PM
Arrivals and Lunch 1h 30m
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1:30 PM
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1:40 PM
Opening and Welcome 10mSpeakers: Andreas Burkert (LMU), Stephan Paul (TUM)
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1:40 PM
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3:25 PM
6 Recent Cluster Highlights / 15 min each
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1:40 PM
Antihelium nuclei as messengers from the depths of the galaxy 15mSpeaker: Stephan Koenigstorfer (TUM)
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1:55 PM
Complete RNA replication cycles in a Hadean microcompartment system 15mSpeaker: Annalena Salditt (LMU)
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2:10 PM
The search for supersymmetry with ATLAS 15mSpeaker: Jonas Wuerzinger (TUM, ODSL)
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2:25 PM
Long-term presence of liquid water on the surface of exomoons orbiting free-floating planets 15mSpeaker: Giulia Roccetti (LMU/ESO)
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2:40 PM
How could we probe the angular dependence of dark matter self-interactions? 15mSpeaker: Moritz Fischer (USM/LMU)
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2:55 PM
Advanced numerical models of the thermal and non-thermal properties of the turbulent star forming interstellar medium 15mSpeaker: Thorsten Naab (Max-Planck-Institute for Astrophysics)
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3:10 PM
Simulation of non perturbative quantum field theory phenomena 15mSpeaker: Anthony Hartin (LMU)
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1:40 PM
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3:25 PM
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3:55 PM
Coffee & Tea & Posters & XR Demos for ORIGINS physics education 30m
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3:55 PM
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4:35 PM
PhD Awards 2022 - I
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3:55 PM
Laudatio to PhD Award Winner Riccardo Arcodia (MPE) 10mSpeaker: Peter Predehl (MPE)
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4:05 PM
PhD Award Thesis: Accretion onto black holes across the mass scale 30m
Riccardo's thesis focused on accretion of matter onto black holes of different masses. It studied one of the most known, yet still unexplained, observational relations in active super-massive black holes and compared it with observations of their stellar-mass relative. It made use of the newly-launched eROSITA X-ray telescope to study a new class of transient accretion events around black holes of intermediate masses.
Speaker: Riccardo Arcodia (MPE)
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3:55 PM
- 4:35 PM → 5:00 PM
- 5:00 PM → 5:30 PM
- 5:30 PM → 5:45 PM
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5:45 PM
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6:30 PM
Seed Money Poster Session ; XR Demos for ORIGINS physics education
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6:30 PM
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8:30 PM
Dinner 2h
- 8:30 PM → 9:10 PM
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12:00 PM
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1:30 PM
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9:00 AM
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9:50 AM
RU-D "Galaxies, Stars and Planets"
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9:00 AM
RU-D "Galaxies, Stars and Planets" Milestone Progress Summary 25mSpeaker: Eric Emsellem (ESO)
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9:25 AM
RU-D Highlight Talk: Combining simulations, observations and instrumentation to understand star and planet formation. 25mSpeaker: Amelia Bayo (ESO)
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9:00 AM
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9:50 AM
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10:45 AM
CN-2 "Planets and other Habitats"
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9:50 AM
CN-2 "Planets and the Habitats" Milestone Summary 25mSpeaker: Barbara Ercolano
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10:15 AM
Twinkle: A Mission to Deliver Large, Structured Extrasolar and Solar System Surveys 30m
The Twinkle Space Mission is a space-based observatory that has been conceived to measure the composition of solar system objects, exoplanets, protoplanetary disks and stars. The satellite is based on a high-heritage platform and will carry a 0.45 m telescope with a visible and infrared spectrograph providing simultaneous wavelength coverage from 0.5 - 4.5 μm. The spacecraft will be launched into a Sun-synchronous low-Earth polar orbit and will operate in this highly stable thermal environment for a baseline lifetime of seven years.
This talk will provide an overview of Twinkle’s capabilities and discuss the broad range of targets the mission could observe, demonstrating the huge scientific potential of the spacecraft. Additionally, the work of the Founding Members will be highlighted, showing the initial interest of the survey members
Speaker: Jonathan Tennyson (UCL)
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9:50 AM
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10:45 AM
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11:15 AM
Coffee, Tea and VR 30m
- 11:15 AM → 11:45 AM
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11:45 AM
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12:30 PM
Geoscience LMU 45mSpeakers: Don Dingwell (LMU), Yan Lavallee (LMU Munich)
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12:30 PM
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2:15 PM
Lunch 1h 45m
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2:15 PM
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2:55 PM
PhD Awards II
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2:15 PM
Laudatio to PhD Award Winner Alan Ianeselli 10mSpeaker: Hermann Gaub (LMU)
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2:25 PM
PhD Awards Thesis: Hadean water-dew cycles drive the evolution of DNA and protocells 30m
Liquid water plays an active role in shaping molecular evolution during the Origin of Life. Water cycles under a Hadean CO2 atmosphere create fluctuations in the salinity, pH and temperature that drive the replication and evolution of long DNA sequences. The water cycles at the millimeter-scale also affect the assembly, division and selection of coacervate protocells.
Speaker: Alan Ianeselli (LMU)
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2:15 PM
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2:55 PM
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3:45 PM
RU-E "Prebiotic Molecules and Life"
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2:55 PM
RU-E Milestone Progress Summary 20mSpeaker: Dieter Braun (LMU Munich)
- 3:15 PM
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3:30 PM
The Time Complexity of Self-Assembly 15mSpeaker: Erwin Frey (LMU)
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2:55 PM
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3:45 PM
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4:10 PM
Coffee, Tea and VR 25m
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4:10 PM
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4:50 PM
CN-8 "Emergence of Structure"
- 4:10 PM
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4:35 PM
CN-8 Highlight Talk : Self-organization across spatial scales 15mSpeaker: Steffen Rulands (LMU)
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4:50 PM
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6:30 PM
ORIGINS 2 Steering Committee Talk and Open-End Brainstorming
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6:30 PM
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8:30 PM
Dinner 2h
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8:30 PM
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10:30 PM
Gaming "Aeon" emergence of life board game or Bowling in Ratskeller
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9:00 AM
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9:50 AM
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9:00 AM
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9:55 AM
RU-A "Fundamental Particles and Forces"
- 9:00 AM
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9:25 AM
Exploring the properties of Quark-Gluon Plasma with heavy-ion collisions 30m
An important ongoing program in high-energy nuclear physics is the exploration of the phase diagram of quantum chromodynamics (QCD) at large values of temperature and/or densities. In that regime, QCD predicts the existence of a quark-gluon plasma (QGP) state, in which quarks are deconfined and can move freely over distances comparable with the size of hadrons. Results from heavy-ion collision data at LHC are consistent with the scenario in which QGP
undergoes collective expansion, dominated by its hydrodynamic response to the anisotropies in the initial state geometry — a phenomenon known as anisotropic
flow. Properties of QGP are typically portrayed by specifying its
transport properties (e.g. shear or bulk viscosities), or its equation of state.In this talk, anisotropic flow results obtained from multi-particle
correlation techniques are presented. Special focus is given to recently developed new flow observables (symmetric and asymmetric cumulants of multi-harmonic flow correlations, symmetry plane correlations) [1,2], each of which by
design extract new and independent information about QGP properties. By using Bayesian parameter estimation methods, it is demonstrated how the temperature-dependent
specific shear and bulk viscosity of QGP can be constrained from experimental data [3,4].Speaker: Ante Bilandzic (Technical University of Munich)
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9:55 AM
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10:45 AM
CN-3 "Properties of Dark Matter"
- 9:55 AM
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10:20 AM
Learning about particle physics with the large-scale structures of the Universe 25mSpeaker: Henrique Rubira (TUM)
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10:45 AM
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11:15 AM
Coffee, Tea & VR 30m
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11:15 AM
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12:00 PM
RU-B "Particles and the Cosmos"
- 11:15 AM
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11:40 AM
RU-B Highlight Talk: Latest results from KATRIN on the neutrino mass and beyond 20mSpeaker: Christoph Wiesinger (MPP, TUM)
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12:00 PM
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12:30 PM
CN-6 "Cosmic Accelerators"
- 12:00 PM
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12:15 PM
Evidence for neutrino emission from the nearby active galaxy NGC 1068 15mSpeaker: Chiara Bellenghi (TUM)
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12:30 PM
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2:15 PM
Lunch 1h 45m
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2:15 PM
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3:15 PM
Astrochemistry
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2:15 PM
Astrochemistry in Solar System precursors: new results on complex carbon chains 20mSpeaker: Eleonora Bianchi (Excellence Cluster ORIGINS)
- 2:35 PM
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2:55 PM
Exoplanet astrochemistry questions that we did not have before JWST 20mSpeaker: Karan Molaverdikhani (USM/LMU)
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2:15 PM
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3:15 PM
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6:00 PM
Annual General Assembly of all Cluster Members and Infrastructure Summaries
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3:15 PM
ORIGINS Summary (Andreas Burkert/Stephan Paul) 15mSpeakers: Andreas Burkert (LMU), Stephan Paul (TUM)
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3:30 PM
Administration Summary 45mSpeakers: Ina Haneburger (Cluster of Excellence ORIGINS), Alice Smith-Gicklhorn (Excellence Cluster ORIGINS), Odele Straub, Stefan Waldenmaier (Excellence Cluster ORIGINS)
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4:15 PM
Coffee, Tea and VR 30m
- 4:45 PM
- 5:00 PM
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5:15 PM
LRSM Summary 15mSpeaker: Martin Losekamm (Technische Universität München)
- 5:30 PM
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5:45 PM
MIAPbP Summary 15mSpeaker: Andreas Weiler (TUM)
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3:15 PM
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6:00 PM
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6:30 PM
Group Photo
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6:30 PM
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8:30 PM
Dinner 2h
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9:00 AM
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9:55 AM
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9:00 AM
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9:55 AM
RU-C "Large Scale Structure"
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9:00 AM
RU-C Milestone Update 25mSpeaker: Jochen Weller (LMU)
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9:25 AM
Computer Vision for high-redshift astrophysics and cosmology 30mSpeaker: Dr Caroline Heneka (Institute of Theoretical Physics, University of Heidelberg)
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9:00 AM
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9:55 AM
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10:35 AM
CN-4: "Dark Energy"
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9:55 AM
CN-4 "Dark Energy" Milestone Summary 20mSpeaker: Ariel Sanchez (MPE)
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10:15 AM
New Secondary CMB Anisotropies, Radio Galaxies and Non-thermal SZ 20mSpeaker: Subhabrata Majumdar (Tata Institute for Fundamental Research (TIFR), Mumbai, ORIGINS Guest)
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9:55 AM
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10:35 AM
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11:15 AM
Coffee & Tea 40m
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11:15 AM
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12:00 PM
CN-1 "Black Holes"
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11:15 AM
CN-1 "Black Holes" Milestone Progress Summary 30mSpeaker: Dieter Luest (LMU-Munich)
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11:45 AM
CN-1 Highlight Talk: AGN results from eROSITA 15mSpeaker: Johannes Buchner (MPE)
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11:15 AM
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12:00 PM
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1:30 PM
Lunch 1h 30m
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1:30 PM
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2:10 PM
CN-5 "Turbulence"
- 1:30 PM
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1:55 PM
A spectral Cosmic Ray Model for Cosmological Simulations 15mSpeaker: Ludwig Boess (USM/LMU)
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2:10 PM
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3:00 PM
CN-7 "Matter under Extreme Conditions"
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2:10 PM
CN-7 Milestone Progress Summary 25mSpeaker: Laura Fabbietti (TUM)
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2:35 PM
Collective neutrino oscillations in core-collapse supernovae and neutron star mergers 25mSpeaker: Sajad Abbar (MPP)
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2:10 PM
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3:00 PM
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3:30 PM
Invited Talk: CMOS Technology for sensor applications 30mSpeaker: Magnus Mager (CERN)
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3:30 PM
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4:00 PM
Coffee & Tea 30m
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4:00 PM
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4:30 PM
Final Remarks & Discussion 30m
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4:35 PM
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4:36 PM
Buses leaves for Munich 1m
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9:00 AM
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9:55 AM
