supernovae explosions and the accelerating universe...

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Bodo Ziegler VERA seminar Wien 27.10.2011 2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe Bodo Ziegler Nobel Prize for Physics 2011 Institute for Astronomy University of Vienna Supernovae explosions and the Accelerating Universe Since 09/2010: oUniProf University of Vienna 12/2008-08/10: Staff member European Southern Observatory 2008: Prof. University of Bonn 2002-2007: Volkswagen Foundation Young Research Group Göttingen Before: Heidelberg, Los Angeles, Munich, Durham (UK)

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Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Bodo Ziegler

Nobel Prize for Physics 2011

Institute for AstronomyUniversity of Vienna

Supernovae explosions and the Accelerating Universe

● Since 09/2010: oUniProf University of Vienna

● 12/2008-08/10: Staff member European Southern Observatory

● 2008: Prof. University of Bonn

● 2002-2007: Volkswagen Foundation Young Research Group Göttingen

● Before: Heidelberg, Los Angeles, Munich, Durham (UK)

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

FORS Deep Field Velocity FieldRotation Curve

Morphology

Cluster MS0451z=0.5

Bodo Ziegler:Main research fields:Galaxy formation & evolution

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

For the discovery of the accelerating expansion of the Universe through observations of distant supernovae.

Saul Perlmutter Brian Schmidt Adam Riess

Nobel Prize for Physics 2011

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Overview

● Basic Cosmology

● Stellar Evolution & Supernovae Ia

The accelerating Universe

Current & future research

Material:nobelprize.org (Royal Swedish Academy of Sciences); my own lecture notes;Riess et al. 1998 AJ 116, 1009; Perlmutter et al. 1999 ApJ 517, 565Dr. A Böhm (Innsbruck), Dr. M. Kenn (Vienna), Dr. B. Leibundgut (ESO)

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Big Bang

Evidence:

● Hubble expansion

● Primordial Nucleosynthesis

● Cosmic background radiation

● Structure formation

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Cosmic Microwave Background

Nobel Prize 2006 (Mather & Smoot) using COBE data:

CMB uniform blackbody with variations � T/T~10-5!

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Structure Formation

Early fl uctuations enable galaxy assembly (but: Dark Matter needed!)

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Expanding Universe

Hubble: brightness & size decrease with increasing redshift

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Redshift & Look-back time

S&W

Defi nition Redshift z :

for v << c: z = v/c

5 Gyr

8 Gyr

13.5 Gyr

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Expanding Universe

Hubble 1929:

Velocity - Distance Relation:

vrad

= H0 D [H

0]=km/s/Mpc

Sandage 1986:

at high z relativistic corrections needed

and dependance on matter content

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Dynamics of Universe

Einstein's General Relativity

Rij Ricci-Tensor, T

ij Energy-momentum tensor, g

ij Metric, � cosmological constant

Cosmological Principle: Universe is homogenous and isotropic

Robertson-Walker metric:

Friedmann equations:

R: scale radius� : energy densityp: pressurek: curvature

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Observable quantities

normalized densities

3H2/8G critical densityof 10-30 g/cm

If cosm. constant form of vacuum energy: �� = � / 8� G (energy density)

with equation-of-state: p� = w

� �

� .

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Standard Candles

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Elliptical Galaxies as Standard Candles

Ziegler&Bender 1997 Bender et al. 1998

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae at high z

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae at high z

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae at high z

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae Type Ia

Hamuy et al. 1996: SN Ia: standard candles with absolute magnitude MB=-19.1±0.3m

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae Type Ia

Hamuy et al. 1996: SN Ia: standard candles with absolute magnitude MB=-19.1±0.3m

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae Type Ia

Evolution binary star system with differing masses:● more massive star evolves faster becoming White Dwarf

● WD exhaust of H, He etc., no nuclear fusion > degenerate core

● Secondary star evolves to Red Giant phase exceeding Roche lobe

● WD extracts mass from RG, accumulates via accretion disk

● WD's mass exceeds Chandrasekhar limit of 1.4M0

● WD explodes completely as supernova

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Stellar Evolution

H→He

pp

M<1.2-1.5 M

radiative

convective

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Stellar Evolution

L~R2 T4eff

100 R

1 R

0.01 R

Hertzsprung – Russel diagram

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Stellar Evolution

Red Giant phase

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Stellar Evolution

Assymptotic Giant Branch phase:degenerate CO core

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Supernovae Type Ia

Wikipedia

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Calculation Distance Modulus

Dependance on cosmo. distance(distance luminosity)analytic expression for fl at Universewith deceleration parameter q

0 (Mattig 1958)

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Effects on Distance Modulus

+ kX + Ag + Ai + ke

K-correction(trafo to rest-frame)

Intrinsic absorption(dust in observed galaxy)

Galactic extinction(dust in Milky Way)

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Effects on Distance Modulus

+ kX + Ag + Ai + ke

K-correction(trafo to rest-frame)

Intrinsic absorption(dust in observed galaxy)

Galactic extinction(dust in Milky Way)

Evolutionary effects

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

SCP's Hubble diagram

Distant SNe are dimmer than expected in fl at or closed Universe!

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Accelerating Universe

SCP HZT

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Concordance Cosmology

Cosmic MicrowaveBackground

Supernovae

BaryonicAcousticOscillations

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Accelerating Universe

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Slide by B. Leibundgut, ESO

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Slide by B. Leibundgut, ESO

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Constraining Dark Energy: CLASH

Observes 25 massive galaxy clusters with HST (WFC3, ACS) in 15 fi lters.

Among primary goal: detect SNe Ia out to z~2 to test constancy of DE.

CLASH-VLT: spectroscopic follow-up using ESO's telescopes on Paranal.

PhD project U. Kuchner utilizes CLASH VIMOS spectra

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Synergy ground-based / space-based measurements

Bodo Ziegler VERA seminar Wien 27.10.2011

2011 Nobel Prize in Physics: Supernovae explosions and the Accelerating Universe

Cosmic History