AIMS

1. To consolidate development efforts that have taken place so far

2. To set a roadmap for future development priorities

3. To grow the user community, and especially to encourage sideways interaction between users

We will set aside several hours of the workshop each day as a hackfest, to collaboratively implement new features and tests

PROGRAM

Monday 19 Feb 2018
9.00 – 9.30 Registration
9.30 – 10.30

Joe Monaghan

: Introduction to SPH Part I (Video)
10.30 – 11.00 Coffee Break
11.00 – 12.00

Joe Monaghan

: Introduction to SPH Part II (Video)
12.00 – 13.00 CAVE2 Visualisation Tour
13.00 – 14.00 Lunch
14.00 – 17.00 Advanced Fortran 90 Programming + Version Control with git (notes: Part I, Part II)
17.00 – 19.00 Wine and Cheese Evening
Tuesday 20 Feb 2018
9.00 – 10.00

Daniel Price

: Dust and Gas in SPH
10.00 – 10.30

Terrence Tricco

: Magnetic Fields in SPH (Notes)
10.30 – 11.00 Coffee Break
11.00 – 11.30

James Wurster

: Non-Ideal MHD (slides)
11.30 – 12.30

Christophe Pinte

: Monte Carlo Radiative Transfer (slides)
12.30 – 13.00

Christopher Russell

: Introduction to 360-degree videos (get your goggles out!)
13.00 – 14.00 Lunch
14.00 – 17.00 Phantom Workshop/Hackathon – visualisation focus (YouTube playlist)
Wednesday 21 Feb 2018
9.00 – 9.40

Daniel Price

: Phantom - design overview and recent applications (slides)
9.40 – 10.10

Conrad Chan

: MPI in Phantom
10.10 – 12.30 Presentations (20min Talk + 5min Questions)
10.10 Orsola De Marco (slides) Common envelope binary interaction simulations with PHANTOM
10.35 Thomas Reichardt Common Envelope Simulations in Phantom
11.00 Coffee Break
11.40 Maya Petkova (slides) Ionising stellar feedback with Phantom and CMacIonize
12.05 Christopher Russell Our galaxy's central parsec: hydrodynamic modelling
12.30 – 14.00 Lunch
14.00 – 17.00 Phantom Workshop/Hackathon
17.00 – late Dinner in the City
Thursday 22 Feb 2018
9.45 – 12.30 Presentations (20min Talk + 5min Questions)
9.45 Jean-Fran├žois Gonzalez (slides) Self-induced dust traps: overcoming planet formation barriers
10.10 Joe Monaghan Drag in SPH dust/gas simulations
10.35 Kieran Hirsh Cavities in circumbinary discs
11.00 Coffee Break
11.40 Daniel Mentiplay Super-Earths in the TW Hya disc
12.05 Christophe Pinte Radiation in protoplanetary discs (slides)
12.30 – 14.00 Lunch
14.00 – 17.00 Phantom Workshop/Hackathon
Friday 23 Feb 2018
9.30 – 11.50 Presentations (20min Talk + 5min Questions)
9.30 David Liptai General Relativistic SPH
9.55 James Wurster The effect of partial ionisation in star formation
10.20 Coffee Break
11.00 Terrence Tricco The Kelvin-Helmholtz Instability in SPH
11.25 Sergei Biriukov Anisotropic diffusion in SPH
11.50 – 13.00 Discussion: Phantom's Prospects
13.00 – 14.00 Lunch
14.00 – 15.30 CAVE2 Session

REGISTER

Click here to register. Be quick! Early bird closes 31/1/17 and numbers are limited.
If you do not wish to give a talk or poster, just enter "none" for the title and abstract.

LOCAL INFORMATION

The conference will be held in: Room 110 (first floor)
School of Physics and Astronomy
10 College Walk
Monash University Clayton Campus
Clayton, Victoria, Australia.

The cheapest way to get here is to take the Skybus from the airport to Southern Cross Station, jump on a train to Huntingdale (Pakenham/Cranbourne line) and then catch the 601 shuttle bus from Huntingdale station to the campus. Total cost around $25. Check the ptv website for details.

The fastest way to get here is in a taxi, but it will cost you around $120.

Our recommmended accommodation option is Mannix college. Otherwise you can check hotels close to campus. Staying somewhere in South Yarra is another option which is on the train line to Monash (30 mins to campus) but in a lively area closer to the centre of Melbourne.

Contact

daniel.price@monash.edu

Local organising committee

Daniel Price

Daniel Mentiplay

David Liptai

Sergei Biriukov

Hayley Macpherson

Christophe Pinte

Scientific organising committee

Daniel Price

James Wurster

Terrence Tricco

Christophe Pinte