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
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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:
——————————
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
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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
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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)