27
Dr Martin Hendry University of Glasgow

Dr Martin Hendry University of Glasgow

  • Upload
    mateja

  • View
    29

  • Download
    5

Embed Size (px)

DESCRIPTION

Why are we here?. Dr Martin Hendry University of Glasgow. Why are we here?…. The period of inflation in the very early Universe was invoked to explain some apparent ‘fine tuning’ problems. If the Universe is now inflating, this presents a new set of ‘fine tuning’ problems. Atoms. - PowerPoint PPT Presentation

Citation preview

Page 1: Dr Martin Hendry University of Glasgow

Dr Martin HendryUniversity of Glasgow

Page 2: Dr Martin Hendry University of Glasgow

Why are we here?….

The period of inflation in the very early Universe was invoked to explain some apparent ‘fine tuning’ problems.

If the Universe is now inflating, this presents a new set of ‘fine tuning’ problems

Page 3: Dr Martin Hendry University of Glasgow

Dark Energy

Cold Dark Matter

Ato

ms

State of the Universe – Nov 2003

Page 4: Dr Martin Hendry University of Glasgow

Dark Energy

Cold Dark Matter

Ato

ms

State of the Universe – Nov 2003

Why does 96% of the Universe consist of ‘strange’ matter and energy?

Page 5: Dr Martin Hendry University of Glasgow

CDM

From Lineweaver (1998)

Page 6: Dr Martin Hendry University of Glasgow

General Relativity:-

Geometry matter / energy

“Spacetime tells matter how to move and matter tells spacetime how to curve”

Einstein’s Field Equations

TGRgRG 82

1

Einstein tensor Ricci tensor Metric tensorCurvature scalar Energy-momentum tensor

of gravitating mass-energy

Page 7: Dr Martin Hendry University of Glasgow

General Relativity:-

Geometry matter / energy

“Spacetime tells matter how to move and matter tells spacetime how to curve”

Einstein’s Field Equations

Treating the Universe as a perfect fluid, can solve equations to determine the pressure and density, and how they evolve

Page 8: Dr Martin Hendry University of Glasgow

Einstein originally sought static solution but this isn’t possible, for ‘normal’ pressure and density

He added a ‘cosmological constant’ to the field equations

Can tune to give static Universe, but unstable

(and Hubble expansion made idea redundant anyway!)

Page 9: Dr Martin Hendry University of Glasgow

Einstein’s greatest blunder?

Page 10: Dr Martin Hendry University of Glasgow

But what is ?…

Particle physics motivates as energy density of the vacuum but scaling arguments suggest:-

So historically it was easier to believe

12010theory)(

obs)(

0

Page 11: Dr Martin Hendry University of Glasgow

Re-expressing Friedmann’s Equations

At any time

1 km

Dimensionless matter density

Dimensionless vacuum energy density

Dimensionless curvature density

Page 12: Dr Martin Hendry University of Glasgow

Re-expressing Friedmann’s Equations

At any time

If the Universe is flat then

1 km

Dimensionless matter density

Dimensionless vacuum energy density

Dimensionless curvature density

0k

Page 13: Dr Martin Hendry University of Glasgow

Dark Energy

Cold Dark Matter

Ato

ms

State of the Universe – Nov 2003

Page 14: Dr Martin Hendry University of Glasgow

State of the Universe – Nov 2003

m

Page 15: Dr Martin Hendry University of Glasgow

CDM

From Lineweaver (1998)

Page 16: Dr Martin Hendry University of Glasgow

m

Value of

Present-day 0/ RR

If the Concordance Model is right, we live at a special epoch. Why?…

Page 17: Dr Martin Hendry University of Glasgow

Hydrogen fusion – fuelling a star’s nuclear furnace

E = mc 2

Page 18: Dr Martin Hendry University of Glasgow

P-P chain, converting hydrogen to helium

Page 19: Dr Martin Hendry University of Glasgow

This has led to more general Dark Energy or Quintessence models:

Evolving scalar field which ‘tracks’ the matter density

Convenient parametrisation: ‘Equation of State’

Can we measure w(z) ?

wP Matter 0Radiation 1/3Curvature -1/3‘Lambda’ -1Quintessence w(z)

iw

Pressure

Density

Page 20: Dr Martin Hendry University of Glasgow

SNIa at z = 0.5

Adapted from Schmidt (2002)

mq2

10

At low redshift, SN1a essentially measure the deceleration parameter

Page 21: Dr Martin Hendry University of Glasgow

SNIa at z = 1.0

Adapted from Schmidt (2002)

At low redshift, SN1a essentially measure the deceleration parameter

mq2

10

Page 22: Dr Martin Hendry University of Glasgow

SNIa at 0.5<z<1.0

Adapted from Schmidt (2002)

At low redshift, SN1a essentially measure the deceleration parameter

mq2

10

Page 23: Dr Martin Hendry University of Glasgow

Tegmark et al (1998)

SNIa measure:-

CMBR measures:-

Together, can constrain:-

mq2

10

mk 1

,m

Page 24: Dr Martin Hendry University of Glasgow

Can we distinguish a constant term from quintessence?…

Not from current ground-based SN observations (combined with e.g. LSS)

Adapted from Schmidt (2002)

Page 25: Dr Martin Hendry University of Glasgow

Can we distinguish a constant term from quintessence?…

Not from current ground-based SN observations (combined with e.g. LSS)…

…or from future ground-based observations (even with LSS + CMBR)

Adapted from Schmidt (2002)

Page 26: Dr Martin Hendry University of Glasgow

Can we distinguish a constant term from quintessence?…

Not from current ground-based SN observations (combined with e.g. LSS)…

…or from future ground-based observations (even with LSS + CMBR)

Adapted from Schmidt (2002)

Page 27: Dr Martin Hendry University of Glasgow

Can we distinguish a constant term from quintessence?…

Not from current ground-based SN observations (combined with e.g. LSS)…

…or from future ground-based observations (even with LSS + CMBR)

Main goal of the SNAP satellite(launch ~2010?)

Adapted from Schmidt (2002)