Previous events - Page 259

Time and place: , CEES seminar room (3313/3315)

Late lunch talk by Robin Cristofari

Time and place: , AUD 3, Geology building, Sem Sælands vei 1

Welcome to the GeoHyd Lunch Seminar on Friday 24 October @12:15. Meet up in AUD 3 in the Geology building (OBS: different location than usual!!).

Time and place: , Auditorium 2, Farmasibygningen

M.Sc. Ingrid Augusta Aursnes Ingebrigtsen ved Farmasøytisk institutt vil forsvare sin avhandling for graden ph.d: Effect of lipid source and glutamate on growth, metabolism and muscle quality in Atlantic cod (Gadus morhua).

Time and place: , Rom 304 (Peisestua), Institutt for teoretisk astrofysikk

Pia Zacharias,Postdoctoral Fellow , ITA

Time and place: , Rom 3515

This week, we read a paper from Ecology Letters by Barnagaud et al. 2014.

Time and place: , Room 4212

This Friday we will discuss this review paper about the fascinating and numerous microsporidian parasites.

Time and place: , NHA bygget 9 etg B91

The Lattice Boltzmann Method and its application in modeling of physiological  flows

Time and place: , FØ467

Michael Kachelriess, NTNU [slides]

The IceCube Collaboration announced 2012 evidence for the first detection of extraterrestrial neutrinos. Meanwhile, the discovery of a extraterrestrial neutrino flux (of surprisingly large magnitude) has been established. After a review of the basic ideas of high-energy neutrino astrophysics, I discuss possible sources for these neutrinos and their signatures.  I  discuss the neutrino yield from collisions of cosmic ray nuclei with gas and the possibility that Galactic sources can explain the IceCube excess. I review also the cascade bound on extragalactic neutrinos and its consequences.

Time and place: , Holmen Fjordhotell

PROGRAM (pdf: This is an excerpt from the booklet that will be handed out at the conference)

Time and place: , Room 3315 (NB!)

Friday seminar by Charles Krebs

Time and place: , AUD I, Geology building, Sem Sælands vei 1

Welcome to the first GeoHyd Lunch Seminar this fall term Friday 17 October @12:15. Meet up in AUD I in the Geology building.

Time and place: , Rom 304 (Peisestua), Institutt for teoretisk astrofysikk

Kathleen M. Jennings, Fafo Institute for Labour and Social Research

Time and place: , Room 3513

This week we will read a paper on competition in bryozoans by Svensson and Marshall 2014: "Limiting resources in sessile systems: food enhances diversity and growth of suspension feeders despite available space".

Time and place: , NHA Hus, B71

Adam Sørensen (UiO) will give a talk with title: Almost commuting matrices

Abstract: Two matrices A,B are said to almost commute if AB is close to BA (in a suitable norm). A question of Halmos, answered by Lin, asks if two almost commuting self-adjoint matrices are always close to two exactly commuting self-adjoint matrices. We will survey what is known about this and similar questions, and report on recent work with Loring concerning how the questions change if we look at real rather than complex matrices.

 

Time and place: , FØ467

Jörn Kersten, Universitetet i Bergen [slides]

Despite the astonishing success of the standard LambdaCDM cosmological scenario, there is mounting evidence for a tension with observations. For example, some measurements indicate that a part of the dark matter is hot. In addition, the observed properties of relatively small galaxies do not quite agree with the predictions by simulations of structure formation.

I will discuss a simple particle physics model containing cold dark matter (DM) and sterile neutrinos. Both are charged under a new gauge interaction. The resulting DM self-interactions and DM-neutrino interactions resolve the problems with structure formation. The sterile neutrinos can account for both a small hot DM component and the neutrino anomalies found in short-baseline experiments.

Time and place: , Room 107, N.H.Abels House

Kristan Ranestad (Dept. of Math, UiO) gives a seminar in room 107, 1st floor N.H. Abels House at 14:15 Tuesday October 14th. Algebra og statistics: Phylogenetic models from an algebraic geometric viewpoint

 

Time and place: , Room 3315

We feel that it's time to find out about the Pairwise Sequential Markovian Coalescent and it derivations. How does it magically infer demography from single genomes? Why does the original author recommend other tools? Why do all these demography plots look the same? And can I use it for my data? Once more, we'll need more than one paper to find out. We'll focus on the first publication to present the PSMC, Li & Durbin (2011) in Nature, but we invite participants with a bit of extra time to check out and report on updates on the method, which were published by Schiffels & Durbin (2014) in Nature Genetics, and by Harris et al. (2014) on arXiv.

Time and place: , Seminar room (3313/3315)

A collection of recent CEES publications

Time and place: , University of Oslo
Time and place: , Rom 4512, Kristine Bonnevies hus

”Protist diversity across a marine - freshwater gradient with a special focus on the X-cell parasite”

Time and place: , Rom 304 (Peisestua), Institutt for teoretisk astrofysikk

Philip Bull,Postdoctoral Fellow , ITA

Time and place: , Rom 4512, Kristine Bonnevies hus

"Effekter av miljøgifter på torsk (Gadus morhua) fra indre Oslofjord"

Time and place: , Auditorium 1, the Geology building

Nele Kristin Meyer at the Department of Geosciences will be defending her dissertation: Debris flows - Initiation conditions and impact on functionality of Norwegian road network

Time and place: , Lille Fysiske Auditorium, room V232, the Physics building

Doctoral candidate Nele Kristin Meyer at the Department of Geosciences will give a trial lecture on the given topic: The challenges from global change for landslide hazard assessment

Time and place: , FØ467

Anders Kvellestad, UiO

Recently a few small (but intriguing) deviations from Standard Model predictions have been identified in the LHC data, one being an excess in the dilepton spectrum in a CMS search for so-called 'kinematic edges' -- a classic signal of physics models with heavy particles decaying through sequential two-body decays. We present an interpretation of this excess in terms of a supersymmetric model with squarks undergoing such sequential decays down to the lightest neutralino, which is a viable candidate for particle dark matter. The good-fit parameter space of the model is presented, along with predictions for squark production at the upcoming 13 TeV LHC run.

Further, using the above analysis as an example, we briefly comment on the main challenges of confronting complex models like Supersymmetry with experimental results, and present an ongoing effort to overcome some of these challenges.