Doktorat na TCfA
Warning: This info may be incomplete and partly out of date!
administrative steps
- getting documents to Dziekanat + http://irk.umk.pl : deadline often two possible deadlines, sometimes one in early July, and usually one around late August/early September
- interview (rozmowy): date a few days after each deadline
formal documents
Mostly in Polish:
conditions
- stipends:
- ,,UMK Szkoły Doktoranckiej (SzD)" - administrative structure being built April-October 2018 - themes for candidates + foreign extra supervisor need to be ready in April
- stipend only lasts for one year; new competition for stipends each year of doctorate, depending on chance and a supposedly meritocratic points system
- grants can be applied for in the national grant system (NCN), partly written in English, partly written in Polish
- most likely out-of-date: as of 2005: normal stipends are only for Polish citizens (EU rules should, in principle, allow other EU citizens, but this may not yet be implemented in national law nor in UMK rules)
- in addition to research, the doctorant must do coursework + teaching:
- the "przewod doktorski" (declaration of intent to submit a thesis) must be "opened" by the second year at latest
practical life
visits by scientists from Central/Eastern Europe
- Mianowski Fund: 1-12 months research visit, if you already have a position and a degree (master's maybe enough?) in your home country
- mianowski waw pl/programme.htm
Ewentualny Tematy
Non-perturbative N-body/GR simulations
N-body simulations (e.g.
AstroPh:0411043,
ArXiv:1105.1082,
AstroPh:0111367) used for the modelling of 0.1 to 5 Gpc scale structure formation assume a rigid Friedmann-Lemaitre-Robertson-Walker (FLRW) background against which perturbations grow according to Newtonian gravity, while the FLRW background itself evolves assuming that structure formation do
not form. An UMK-Lyon project is underway to develop relativistic methods of correcting N-body simulations for this contradiction, by using scalar averaging (
AstroPh:9912347,
ArXiv:0707.2153,
ArXiv:0803.1401,
ArXiv:1203.6263,
ArXiv:1303.6193). The main result of the full project (
ArXiv:1706.06179) is that more accurate simulations help show that "dark energy" is a misinterpretation of the virialisation epoch, during which much of the most massive galaxies and galaxy clusters formed. The student's contribution would be in checking caveats of this calculational method and/or proposing extensions.
http://cosmo.torun.pl/Cosmo/DoktoratTematy
Measuring metric inhomogeneity with BAO
The Universe is not homogeneous, but the Concordance Model starts with a spatially-homogeneous solution to the Einstein field equations and afterwards applies perturbations. The scalar averaging approach (
AstroPh:9912347,
ArXiv:0707.2153,
ArXiv:0803.1401,
ArXiv:1203.6263,
ArXiv:1303.6193) proposes a relativistically more realistic approach to cosmological modelling. The initial measurement of a shift of about 6% in the baryonic acoustic oscillation (BAO) peak location (
ArXiv:1410.1687) in overdense regions provides the first tentative evidence of metric inhomogeneity. The calculations using the presently available software are cpu-intensive. A student would help develop algorithmic speedups, tests of the different software modules, and possibly GPGPU modules under
OpenCL.
http://cosmo.torun.pl/Cosmo/DoktoratTematy