HIP NEWS November 9th 2015

HIP NEWS November 9th 2015
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DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 10 November 2015 at 10.15 in A315
David Salek (Amsterdam)
Dark matter (and dark mediators) at the LHC

Abstract: The LHC results on dark matter from Run-1 were mostly interpreted in the framework of effective field theories. Simplified models involve new mediators between the Standard Model and the Dark Sector and allow for richer phenomenology and more complex interpretations. Possible dark matter search strategies at the LHC in Run-2 will be discussed.

COSMO-Seminar
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Wednesday 11 November at 14:15 in A315
Matti Heikinheimo (Helsinki)
Dark Matter Self-Interactions via Collisionless Shocks in Cluster Mergers

Abstract: While dark matter self-interactions may solve several problems with structure formation, so far only the effects of two-body scattering of dark matter particles have been considered. I will discuss a scenario where a subdominant component of dark matter is charged under an unbroken U(1) gauge group. In this case collective plasma effects need to be taken into account to understand the dynamics of the interacting DM. Plasma instabilities can lead to collisionless dark matter shocks in galaxy cluster mergers. I will discuss the observations made in the Abell 3827 and 520 clusters in this context.

COSMOLOGY COLLOQUIUM
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Time and place: Thursday 12 November at 14:15 in E204 (note place)
Speaker: Lawrence Krauss (Arizona State University)
Title: Journey to the Beginning of Time: Gravitational Waves, Inflation and Fundamental Physics
Abstract: Gravitational Waves from Inflation may have been discovered, or may soon be discovered. If they are, this will push our empirical handle on the universe back in time by 49 orders of magnitude, and will allow us to explore issues ranging from supersymmetry to grand unification, the quantum theory of gravity, and even the possible existence of other universes.

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Thursday 12 November 2015 at 14.15 in E207 (note place)
Jaeyoung Park (Energy Matter Conversion Corporation, San Diego)
Polywell Fusion – Electric Fusion in a Magnetic Cusp

Abstract: Nuclear fusion power is considered the ultimate energy source because of its nearly inexhaustible supply of cheap fuels,
intrinsic safety, zero carbon emissions and lack of long-lived radioactive waste. In this talk, I will introduce the Polywell fusion concept that may offer a low cost and rapid development path to power the world economically and sustainably. As conceived by Dr. Robert Bussard at Energy Matter Conversion Corporation (EMC2) in 1985, the Polywell fusion concept combines electric fusion with magnetic cusp confinement. This allows the Polywell reactor to be small, stable, and highly efficient. Recently, EMC2 carried out an experiment that demonstrated dramatically improved high-energy electron confinement in a magnetic cusp system operating at beta (=plasma pressure/magnetic field pressure) near 1. This result has significant implications for cusp related schemes for producing controlled nuclear fusion power.

Fulbright-Technology Industries of Finland Grant
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More information about Fulbright-Technology Industries of Finland Grants (in Finnish): www.fulbright.fi/fi/stipendit-tohtorintutkinnon-jalkeiseen-tutkimukseen-ja-luennointiin/fulbright-technology-industries.
Application deadline is December 14, 2015, 10:00 a.m.

Update your information in Tuhat
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Permanently employed teaching and research staff are requested to update their information in the Tuhat database by 11 January 2016.
https://flamma.helsinki.fi/en/notifications/update-your-information-in-tuhat

Fortcoming training for employees
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Prepare for your doctoral defence 20.11.2015 at 12:30-16:00
Those with dissertation in the near future.
Last sign-up date: 9.11.2015
Sign up in http://www.helsinki.fi/trainingcalendar ( Staff Training Calendar HENKKA)

The Strategic Research Council (SRC) at the Academy of Finland : Apply for strategic research funding
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The SRC’s call will be implemented in two stages. The first stage, for letters of intent, will be open in the Academy of Finland’s online services between 5 November and 9 December 2015.
In addition, the SRC will open a supplementary call within the 2015 programme A Climate-Neutral and Resource-Scarce Finland. https://flamma.helsinki.fi/en/notifications/apply-for-strategic-research-funding

Visitors
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K.C. Chan 29.11. – 6.12. (FM)
J. Ghiglieri 23.11. – 27.11. (AV)
G. Itsios 16.11. – 23.11. (NJ)
J. Park 12.11. – 13.11. (TL)

HIP NEWS November 2nd 2015

HIP NEWS November 2nd 2015
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HIP Staff News
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Dr. Jaakko Härkönen has been appointed by the Xiangtan University
(PR China) as a honorary professor for the period 2015-2017.

HIP Detector Laboratory informs
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20 doctoral students from Nordic countries will visit HIP Detector Laboratory for research training course in detector technology for particle physics during 2-6.11.2015.

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 3 November 2015 at 10.15 in A315
Lene Bryngemark (Lund)
Search for physics beyong the Standard Model using dijet distributions in ATLAS

Abstract: The LHC gives us access to the highest collider energies, at the highest intensities, providing a unique opportunity to thoroughly examine the constituents of matter and their interactions at ever smaller distances and higher mass scales. Produced in the strong — or a new, previously unseen — interaction, jets probe the very energy frontier. With the recent increase in LHC beam energy, ATLAS makes use of this sensitivity to make its first statements of what physics looks like in a new energy regime. In this presentation I show the results from both the 8 and the more recent 13 TeV analysis of dijet mass and angular distributions.

COSMO-Seminar
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Wednesday 4 November at 14:15 in A315
Michael Joyce (UPMC, Paris)
Non-linear structure formation in scale free cosmological models

Abstract: Calculation of the clustering of matter in the universe in different cosmological models, even in the approximation that all but gravitational forces are neglected, relies essentially on numerical simulations which use the N body method. The physics of this non-linear clustering remains poorly understood, and there are also open questions about the resolution/precision of simulations. After a brief overview of these issues, I will discuss them in the framework of a particularly simple class of “scale-free” cosmological models, which have the interest of providing a very simple diagnostic for determining resolution, and also some simple analytical predictions for clustering. We explore using these models, in both one and three dimensions, two questions which turn out to be intimately linked to the issue of numerical resolution: the relevance of the stable clustering approximation in the strongly non-linear regime, and the dependence of halo profiles on cosmology and initial conditions.

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Thursday 5 November 2015 at 10.15 in A315
David Daverio (Geneva)
Large scale structure formation within a general relativistic framework

Abstract: One century after the conception of General Relativity (GR), there is still a large pool of predictions we still have difficulties to get. Indeed, to give only one example, large scale structure formation is still simulated within a Newtonian framework. This framework, even well suited for cosmology as it can be understood as a week field quasi static approximation of GR, does not take into account the propagating degree of freedom of GR and is not well suited to include relativistic sources such as neutrinos. Recently, the first code aiming to simulate large scale structure within a general relativistic framework has been developed. This code, gevolution, solves GR in the weak field limit using the approximation scheme proposed in Adamek et al. 2014 and is constructed on top of the framework LATfield2 which manages the particles and provides a scalable parallelisation allowing to run with lattice of 4096^3 cells with one particle per cell on 16k processes. In this talk we will discuss the method used to develop this code and first results of cold dark matter simulation will be presented.

Visitors
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D. Daverio 25.10. – 6.11. (KR)
M. Joyce 3.11. – 5.11. (ML)

HIP NEWS October 26th 2015

HIP NEWS October 26th 2015
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DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 27 October 2015 at 10.15 in A315
Alexander Merle (MPI, Munich)
Sterile Neutrino Dark Matter: From Particle to Astrophysics and back

Abstract: In the absence of a clear WIMP signal, we should think about alternative candidates for Dark Matter. A very well motivated example is a (up to now hypothetical) sterile neutrino with a mass of a few keV. In this talk, I will give an overview over the topic of keV sterile neutrino Dark Matter, thereby exploring all corners from Dark Matter production in the early Universe over astrophysical bounds and neutrino phenomenology to particle physics model building aspects. While WIMPs are not dead yet, they have to learn how to live in the neighbourhood of serious competitors.

COSMO-Seminar
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Wednesday 28 October 2015 at 14:15 in A315
Tommi Tenkanen (Helsinki)
Cosmic Inflation and Dark Matter

Abstract: We show that dark matter abundance and inflationary scale could be intimately related. Standard Model extensions with Higgs mediated couplings to new physics typically contain extra scalars whose excursions at the end of inflation can be very large. If their coupling to the Standard Model is weak, they will not thermalize and may easily constitute too much dark matter. As an example we consider Standard Model extended by a real singlet scalar and a singlet fermion. We discuss the field dynamics during inflation together with the post-inflationary dark matter production mechanisms and derive stringent constraints on viable mass scales and coupling values.

H2020 Marie Sklodowska-Curie ITN info session for the 2016 call applicants
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Time: 29.10.2015 at 13-15
https://flamma.helsinki.fi/en/researchers/infosession-msca-itn-2016-call-applicants
Registration: https://elomake.helsinki.fi/lomakkeet/64310/lomake.html
Further information on MSCA is available on https://flamma.helsinki.fi/en/EUframeworkprogrammes/HY309934

Particle Physics Day 2015
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Friday 30 October 2015 at 10:15 – 15:00 in Exactum CK112
http://www.helsinki.fi/~hitu_www/hituday_2015.html

Fortcoming training for employees
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Finnish Working Culture 6.11.2015 at 9:00 – 16:00
The course is targeted for all new international employees of the University of Helsinki.
Last sign-up date: 26.10.2015
Sign up in http://www.helsinki.fi/trainingcalendar ( Staff Training Calendar HENKKA)

Visitors
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A. Cabo 2.10. – 27.10. (AT)
D. Daverio 25.10. – 6.11. (KR)
A. Merle 26.10. – 28.10. (TT)
Y. Zhu 28.10. – 30.10. (AV)

HIP NEWS October 19th 2015

HIP NEWS October 19th 2015
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HIP Staff News
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Dr. Mikko Voutilainen has been appointed
as assistant professor (tenure-track)
in experimental particle physics at
the University of Helsinki starting
Nov. 1st, 2015.

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 20 October 2015 at 10.15 in A315
Timo Alho (Reykjavik)
Geometric Algebra: a coordinate free formalism for inner product spaces

Abstract: Geometric Algebra (GA) is a mathematical system defined by
imbuing the vectors of an inner product space directly with the
Clifford algebra generated by the inner product, without considering a
separate representation of the algebra operating on the vectors. This
simple change in point of view gives a system which generalizes
exterior algebra, quaternions, spinors, and many other algebras used in
theoretical physics, while simplifying both concepts and calculations.
This talk will open a brief course on the algebra and its extension to
geometric calculus. During the talk we will primarily give elementary
details of the formalism, with more advanced topics to be handled later
during the course. Some applications are pointed out for motivation.

COSMO-Seminar
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Wednesday 21 October 2015 at 14:15 in A315
Hannu Nyrhinen (Helsinki)
Story of bimetric variational formalism
Abstract: Bimetric variational formalism was introduced a while ago to construct
novel bimetric gravity models. In these models an affine connection is generated
by an additional tensor field which is independent of the physical metric.
In this talk I will describe the ideas behind the bimetric variational formalism
and some results preceding our work (in JCAP05(2015)021). Namely, we addressed
the issue of ghosts plaguing many bimetric models. Previous work had hinted of a
possibility of removing such unstable degrees of freedom from these theories.
I will show how using the ADM decomposition it is possible to study these models
and the behaviour of their degrees of freedom.

H2020 Marie Sklodowska-Curie ITN info session for the 2016 call applicants
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Time: 29.10.2015 at 13-15
https://flamma.helsinki.fi/en/researchers/infosession-msca-itn-2016-call-applicants
Registration: https://elomake.helsinki.fi/lomakkeet/64310/lomake.html
Further information on MSCA is available on
[1]https://flamma.helsinki.fi/en/EUframeworkprogrammes/HY309934

Visitors
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A. Cabo 2.10. – 27.10. (AT)

HIP NEWS October 12th 2015

HIP NEWS October 12th 2015
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DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 13 October 2015 at 10.15 in A315
Alejandro Cabo (La Habana, Cuba)
Is a generalized NJL model the effective action of massless QCD?

Abstract: A local and gauge invariant alternative version of QCD for massive fermions introduced in previous works, is considered here to
propose a model which includes Nambu-Jona-Lasinio (NJL) terms in the action. The Lagrangian includes new vertices which at first sight look as breaking power counting renormalizability. However, these terms also modify the quark propagators, to become more convergent at large momenta, thus indicating that the theory is renormalizable. Therefore, it follows the surprising conclusion that the added NJL four fermion terms do not break renormalizability. The approach can also be interpreted as a slightly generalized renormalization procedure for massless QCD, which seems able to incorporate the mass generating properties for the quarks of the NJL model, in a renormalizable way. It also seems to have opportunity to implement Fritzsch’s Democratic Symmetry description of the quark mass hierarchy.

Thursday 15 October 2015 at 10.15 in A315
Tommi Alanne (CP3-Origins, Odense)
Elementary Goldstone Higgs and raising the fundamental scale

Abstract: We study an extension of the scalar sector of the Standard Model (SM) where the observed Higgs is a pseudo-Goldstone boson (pGB) associated with the global symmetry breaking pattern SU(4) to Sp(4). This particular breaking pattern is interesting, because depending on the embedding of the electroweak (EW) symmetry, the breaking of the global symmetry can either leave the full EW sector intact, break the EW completely to electromagnetism, or more interestingly lead to something between these two extreme cases. In the unbroken case, the entire Higgs doublet can be identified with four of the five Goldstone bosons of the global symmetry breaking.

All of the different alignments of the EW symmetry are equivalent at the tree-level, but since the gauging of the electroweak sector and introducing Yukawa terms for the SM fermions break the global symmetry of the scalar sector, quantum effects determine a preferred vacuum alignment.

In this talk, I will present the main results of our study and show that very slightly broken EW symmetry is preferred. Therefore, the observed Higgs boson is dominantly a pGB, and interestingly the electroweak scale emerges due to the alignment of the EW sector in the global symmetry, whereas the fundamental scale of the spontaneous symmetry breaking is significantly higher.

Visitors
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A. Cabo 2.10. – 27.10. (AT)

HIP NEWS October 5th 2015

HIP NEWS October 5th 2015
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HIP Staff News
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Professor Paula Eerola has been appointed
as the Director of HIP for the 5-year period
starting 1.1.2016.

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 6 October 2015 at 10.15 in A315
Jarno Rantaharju (Odense)
Lattice Four-Fermion Interactions for Beyond Standard Model Physics

Abstract: We present a study of a lattice model of chirally symmetric four-fermion interactions, the Nambu Jona-Lasinio model, with Wilson fermions. Four fermion operators are a necessary part of many models of beyond Standard Model physics. In particular we are interested in technicolor models, where effective four-fermion operators are used to generate the standard model fermion masses. In the ideal walking scenario, the same interaction is responsible for breaking the chiral symmetry in an otherwise conformal model. As a first step, we study the restoration and spontaneous breaking of chiral symmetry in the lattice NJL model before adding a gauge interaction. We map the phase structure of the model and establish chiral symmetry breaking.

Seminar: The Brilliance of Science – the Role of Women in International Science
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Time: Tuesday 6 October, 2015 at 17:00 – 19:30 (note the changed start time)
Organizers:
Finnish Academy of Science and Letters
Embassy of Italy in Helsinki
Istituto Italiano di Cultura
Place: Kumpula Campus, Exactum, Lars Ahlfors Auditorium
Gustaf Hällströmin katu 2 B, 1st floor, Helsinki
Program: http://www.acadsci.fi/tilaisuudet/brilliance.htm

TEDxCERN@University of Helsinki, Friday 9 October webcast at Kumpula
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The webcast is shown in Physicum E207 from 15 to 21. For more information on the event and the speakers, visit: tedxcern.web.cern.ch/speakers.

OPEN POSITIONS:
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A tenure-track faculty opening in Theoretical Particle-Astrophysics at the Department of Physics at Washington University in St. Louis, by Dec. 1st, 2015.
http://www.physics.wustl.edu/faculty_openings

Visitors
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A. Cabo 2.10. – 27.10. (AT)
J. Rantaharju 5.10. – 9.10. (KR)

HIP NEWS September 28th 2015

HIP NEWS September 28th 2015
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DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 29 September 2015 at 10.15 in A315
Jose Miguel No (Sussex)
Probing the Electroweak Phase Transition at LHC and Beyond

Abstract: Uncovering the nature of the electroweak (EW) phase transition in the early Universe would be key to shed light on the possible origin of the cosmic matter-antimatter asymmetry. We discuss various ways in which searches for new physics beyond the Standard model (SM) at LHC can be used to probe the nature of the EW phase transition, and their implications for the generation of the baryon asymmetry of the Universe at the EW scale.

Väisälä Foundation grants
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are open for applications until Sep. 28th., see www.acadsci.fi/scholarships.htm

OPEN POSITIONS:
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A tenure-track faculty opening in Theoretical Particle-Astrophysics at the Department of Physics at Washington University in St. Louis, by Dec. 1st, 2015.
http://www.physics.wustl.edu/faculty_openings

Visitors
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A. Cabo 2.10. – 27.10. (AT)
J.M. No 29.9. – 1.10. (VK)

HIP NEWS September 21st 2015

HIP NEWS September 21st 2015
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COSMO-Seminar
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Wednesday 23 September at 14:15 in A315
András Kovacs (Barcelona)
Cold imprint of supervoids in SDSS, Pan-STARRS1, and DES

Abstract: Large-scale structures at low redshift leave their mark on the Cosmic Microwave Background radiation via the Integrated Sachs-Wolfe and Rees-Sciama effects, providing direct probes of the late time cosmic acceleration and the physics of Dark Energy. In practice, however, these imprints are small enough to be measurable sufficiently with currently available galaxy catalogues. Yet, striking correlations have been observed between cosmic super-structures in SDSS and the CMB, and there is evidence for a supervoid at redshift z~0.2 aligned with the Cold Spot suggesting a causal relationship. Accounting for these anomalies, N-body simulations and theoretical studies suggest that the signal can only arise from a different physical mechanism or is a statistical fluke. I will discuss an important piece of the puzzle that remains out of place: the effect of photometric redshift uncertainties. I will present the recent characterization of the three-dimensional properties of the SDSS super-structures using BOSS spectroscopy, details about the density mapping of the Cold Spot region, and specific void finding strategies designed for the Dark Energy Survey.

Väisälä Foundation grants
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are open for applications until Sep. 28th., see www.acadsci.fi/scholarships.htm

OPEN POSITIONS:
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A tenure-track faculty opening in Theoretical Particle-Astrophysics at the Department of Physics at Washington University in St. Louis, by Dec. 1st, 2015.
http://www.physics.wustl.edu/faculty_openings

Fortcoming training for employees
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Tervetuloa yliopistoon 07.10.2015 klo 08:30 – 14:00
Kohderyhmä: Yliopiston uudet työntekijät. Last sign-up date: 25.9.2015

Sign up in http://www.helsinki.fi/trainingcalendar ( Staff Training Calendar HENKKA)

Visitors
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A. Kovacs 22.9. – 25.9. (SR)

HIP NEWS September 14th 2015

HIP NEWS September 14th 2015
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COSMO-Seminar
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Wednesday 16 September 2015 at14:15 in A315
Seshadri Nadathur (Helsinki)
The nature of voids: simulations, theory, and use in cosmology

Abstract: Cosmic voids are an exciting tool which can potentially be used to test a number of different cosmological scenarios, including structure formation, dark energy and modified gravity. Yet voids are not well understood. I will discuss the general properties of voids in simulations show that they do not match the predictions of the standard theoretical model of voids based on the excursion set formalism. I will discuss the reasons for this discrepancy and argue that it points to the need for simulation-based calibration of void properties for comparison with observation. I discuss the dependence of void properties on those of the galaxies in which they are found, and identify some universal properties which are independent of these details. In particular I will focus on how voids trace maxima of the gravitational potential field, and the implications of this for lensing and ISW studies.

Fortcoming training for employees
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Welcome to the University 30.09.2015 at 08:45 – 14:00
The course is targeted for all new international employees of the University of Helsinki.
Last sign-up date: 20.9.2015

Sign up in http://www.helsinki.fi/trainingcalendar ( Staff Training Calendar HENKKA)

Väisälä Foundation grants
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are open for applications until Sep. 28th., see www.acadsci.fi/scholarships.htm

Visitors
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Y.C. Ong 7.9. – 14.9. (MC)

HIP NEWS September 7th 2015

HIP NEWS September 7th 2015
===========================

DEPARTMENT OF PHYSICS / HIP JOINT COLLOQUIA / SEMINARS
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Tuesday 8 September 2015 at 10.15 in A315
Robert Fleischer (Nikhef, Amsterdam)
In Pursuit of New Physics with B Decays: Theoretical Status and Prospects

Abstract: The exploration of B-meson decays has reached an unprecedented level of sophistication, with a phase of even much higher precision ahead of us thanks to the next run of the LHC and the future era of Belle II and the LHCb upgrade. For many processes, the theoretical challenge in the quest to reveal possible footprints of physics beyond the Standard Model will be the control of uncertainties from strong interactions. After a brief discussion of the global picture emerging from the LHC data, I will focus on the theoretical prospects and challenges for benchmark B decays to search for new sources of CP violation, and highlight future opportunities to probe the Standard Model with strongly suppressed rare B decays.

Thursday 10 September 2015 at 10.15 in A315
Aleksi Kurkela (CERN)
Hydrodynamisation in high energy nuclear collisions from QCD Lagrangian?

Abstract: Thermalisation, isotropisation and hydrodynamisation in high energy collisions of large nuclei has been studied in numerous models. I present a computation which is as close as possible to a first principle one starting from the QCD Lagrangian.

Thursday 10 September 2015 at 14.15 in E206. Note place and time!
Yen Chin Ong (Nordita, Stockholm)
Hawking evaporation time scale of black holes in Anti-de Sitter spacetime

Abstract: If an absorbing boundary condition is imposed at infinity, an asymptotically Anti-de Sitter Schwarzschild black hole with a spherical horizon takes only a finite amount of time to evaporate away even if its initial mass is arbitrarily large. In fact this is a rather generic property for an asymptotically locally AdS spacetime: regardless of their horizon topologies, neutral AdS black holes in general relativity take about the same amount of time to evaporate down to the same size. We explain this surprising property in this talk.

Visitors
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R. Fleischer 6.9. – 9.9. (KK, AV)
P. Lehmann 8.9. – 11.9. (IK)