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Sci
ence
astronomy particle physics
astroparticle physicsparticle astrophysics
IHEFStan Bentvelsen
IAPRalph Wijers
ITFAErik Verlinde
theoretical physics
-large: astronomy (ESO & ESA)
Electromagnetic: radio–infrared-optical-Xray-ray
IAP
-large: where do we stand?today
nucleosynthesis
cosmicmicrowavebackground
(CMB)radiation
cosmicbackgroundgravitational
waves
Theoretical physics0
s
10
43 s
14 miljard jaarna de Oerknal1
03
5 s
10
12 s nu:
Universum koelt af
Oerk
nal
?
??
ITFA
quantum field theory
(1950)
stringtheory
?
special relativity(Einstein, 1905)
general relativity(Einstein, 1915)
cspeed of light
quantum mechanics
(1920)
h Planck’sconstant
gravity(Newton, 1685)
classical mechanics
(Newton, 1685) GN
Newton’sconstant
Astroparticle physicswhen -small meets -large
FNWI speerpunten, 14 december 2007, Amsterdam
IHEF: Stan BentvelsenITFA: Erik VerlindeIAP: Ralph Wijers
FrankLinde
Composition of the UniverseEvolution of the Universe
The extreme Universe
Opportunities
AUGER – LOFAR – (SKA) ANTARES – (KM3NeT)
HESS – (CTA)VIRGO – (LISA)
UvA: pulsartimingarrays
(gravity)
UvA: dark
matter
GRBs
1. Cosmic rays LOFAR, AUGER
2. Neutrino’s ANTARES, KM3NeT
3. Gravitational waves VIRGO, LISA,
Ast
ropart
icle
physi
cs:
NL
appr
oved
subm
itted
Ast
ropart
icle
physi
cs:
UvA
IHEF IAP
ITFA
cosmologydark matter
(dark energy)
dark mater?cosmic rays?
GRBs?
LHC datadark matter?
extra dimensions?
Interpretaton:CMB data
Primordial GW datadark energy?
Astroparticle physics - strong points New field @ astronomy/particle physics interface Cutting edge infrastructures built & forthcoming High risk - high impact International activity Appeals to students & general public NL: funding starting to flow (FOM, NOVA, )
UvA/Amsterdam: World-renowned theoretical physics group Excellent astronomy & particle physics groups (Nikhef) Excellent (grid) computing infrastructure Create more synergy between IAP-IHEF-ITFA