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Story of the Universe Story of the Universe

Story of the Universe - PowerPoint Presentation

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Story of the Universe - PPT Presentation

Atoms to Astronomy 2 Special theory of Relativity It is a basic property of Nature that Velocity of Light in vacuum is constant All inertial frames are identical so if two objects are moving with a constant velocity it is impossible to do any test which allows to measure the velocities in a ID: 542769

atoms astronomy stars universe astronomy atoms universe stars object objects velocity time theory gravity mass galaxies light 400 formation

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Slide1

Story of the UniverseSlide2

Atoms to Astronomy

2

Special theory of Relativity

It is a basic property of Nature that:

Velocity of Light in vacuum is constant.

All inertial frames are identical so if two objects are moving with a constant velocity, it is impossible to do any test which allows to measure the velocities in absolute manner.

This has significant consequences. Slide3

Atoms to Astronomy

3Slide4

Atoms to Astronomy

4

Consequences

Because velocity of light is constant:

space and time must contract.

Acceleration must increase not just the velocity of an object but also its inertia and hence objects become heavier as they approach the velocity of light

No object with finite mass can move at velocity of light and no object of zero mass can move at a slower velocity!Slide5

Atoms to Astronomy

5Slide6

Gravity - 1

Gravity is the attractive force that attracts two bodies of mass M and m with a force which is given by

where i is the unit vector in the line joining the centre of mass of the two objects.From this, one can derive Kepler’s 3 laws:Each planet goes around the sun in an elliptical orbit with the Sun at one focus of the ellipse. Planets cover equal area in equal times.

The square of the period of the revolution (T) of the planet is proportional to the cube of the semi-major access (a) of the

orbit.

 

6Slide7

Gravity - 2

It also defines Keplerian Velocity. In order for an object to remain in stable revolution around a star, it must have a velocity so that gravity and centrifugal force are balanced. The inverse square law implies that in general, the orbit of an object experiencing the gravitational attraction of another body will undergo motion best explained by conic curves (ellipse, parabola or hyperbola) defined by initial conditions. Also, the centre of mass of the two objects going around each other will be the stable point around which both the objects will revolve.

7Slide8

Lagrangian points

8The Lagrangian

points libration points are five positions between 2 gravitating bodies, where a small object affected only by gravity can theoretically be stationary relative to two larger objects (such as a satellite with respect to the Earth and Moon). The Lagrange points mark positions where the combined gravitational pull of the two large masses provides precisely the centripetal force required to rotate with them.Equipotential surfaces

Balanced potential point:

Object will be balanced

Mass transfer occurs from here

ROCHE LOBESlide9

Problems

However, this is not fully satisfactory and cannot explain precession of orbits etc. This led Einstein to expand it into a larger formulation called General Theory of Relativity.Newton’s laws are a special case of General Theory of relativity when the masses and speeds are small.Atoms to Astronomy

9Slide10

Atoms to Astronomy

10

General theory of Relativity

General Theory of relativity states that:

Influence of Gravity is identical to that of sitting in an accelerated frame.

Identifying the curvature of space-time with Gravity

It becomes important in the presence of Strong gravitational fields such as those existing near compact objects.Slide11

Atoms to Astronomy

11Slide12

Atoms to Astronomy

12

Super massive black hole in the galaxy NGC4258

MCG-6-30-16 - 400 ks long XMM observation

Iron line in compact objects

Quasi periodic oscillations of 0.01 to 500 Hz and direct evidence of BHSlide13

Atoms to Astronomy

13

Quantum Mechanics

When the measuring method is of the same order as what is being measured, there are some fundamental complications and the observer and the observed are intermixed!

Since energy and mass are equivalent, one can imagine mass as having energy and wavelength.

Inversely, light which is a packet of energy can be considered as if it was a solid object and can be traded only in fundamental units!

The wavelength of a matter object is in fact the probability of finding the object somewhere etc.

It also produces some interesting effects such as:

tunnelling

stable electron orbits.Slide14

Atoms to Astronomy

14Slide15

Atoms to Astronomy

15Slide16

Atoms to Astronomy

16

blue

yellow

red

blue

yellow

red

Doppler Shift

Light from stationary star

Light from star moving away from us (red shift)

Light from object moving towards us (blue shift)

red

blue

yellowSlide17

Atoms to Astronomy

17

Northern Sky

Southern SkySlide18

Atoms to Astronomy

18

Difference in brightness can arise because

The stars are at different distances

Stars are of different intrinsic brightnessSlide19

Atoms to Astronomy

19Slide20

Atoms to Astronomy

20

FOR NORMALISED AREASlide21

Atoms to Astronomy

21Slide22

Atoms to Astronomy

22

For stars at an angle, an additional cos(

) factor has to be consideredSlide23

Atoms to Astronomy

23

16 D

sunSlide24

Atoms to Astronomy

24

700 D

sun

1 AUSlide25
Slide26

Atoms to Astronomy

26

Measuring distances to galaxies involves using some selected objects

STANDARD CANDLES

These are objects of known intrinsic brightness. Hence a ratio of their apparent brightness to their intrinsic (absolute) brightness gives their distance.

For objects inside our galaxy an additional parameter comes from extinction where distance is measured by parallax and ism by extinction.Slide27

Atoms to Astronomy

27

Variable Stars as distance indicators

The period-luminosity relation for Cepheids

Constant luminosity

Note the logarithmic scale for the graph

(type 1)Slide28

Atoms to Astronomy

28Slide29

Atoms to Astronomy

29Slide30

30

Redshift (z) is defined as z =  / z = 1+[(c+vrec)/(c-vrec)]1/2

Depth of Universe Visible (a) is a = (1+ z)-1Slide31

Atoms to Astronomy

31Slide32

Atoms to Astronomy

32

Planck Value: 67.3 km/s/MpcSlide33

Atoms to Astronomy

33Slide34

Atoms to Astronomy

34Slide35

Atoms to Astronomy

35Slide36

Atoms to Astronomy

36Gamma raySlide37

37

WMAP

PlanckSlide38

38

3 min

380,000 yearsPresent

A conspiracy of Gravity and Nuclear forces

Time

EntropySlide39

Atoms to Astronomy

39Star formation through timeMadau plot (Cole et al. 2001)

Cosmic timeSlide40

Wonders of the Universe

40Slide41

Atoms to Astronomy

41Gravity dominatedExpansion dominatedSlide42

Atoms to Astronomy

42Slide43

Atoms to Astronomy

43

Inflation

It seems that the nascent universe passed through a phase of exponential expansion.

Inflation answers the following problems of the big bang cosmology:

Why does the universe appear flat, homogeneous and isotropic

Origin of the large-scale structure of the cosmos. Quantum fluctuations in the microscopic inflationary region, magnified to cosmic size, become the seeds for the growth of structure in the universe.Slide44

Atoms to Astronomy

44Slide45

Atoms to Astronomy

45Slide46

46

Dense clouds of gas collapse into the first (Pop III) massive stars and probably produce the first GRBs. GRBs can then precede the formation of the first galaxies, which in turn precede that of active galactic nuclei (AGN) powered by supermassive

black holes. Thus, GRBs could probe the first structures and galaxies to emerge after the 'dark ages' of the Universe. The narrow beaming of GRBs, best defined by GRB 080319B (not shown to scale), makes them the most luminous back-lights for mapping the far-distant visible Universe.Slide47

47

Inflation

10-35 sProton formation:1 sec

The earliest galaxies we have seen are at z ~

7.51

,

i.e. about

10.7

billion years since the birth of the Universe.

The earliest stars were born 200 million years after the Universe was born!Slide48

Atoms to Astronomy

48Slide49

Atoms to Astronomy

49Slide50

Atoms to Astronomy

50Slide51

51

Maxwell’s Electromagnetic Theory

Abdul Salam’s Electroweak TheoryStandard Model

String Theory?

Theory of Vacuum fluctuations???Slide52

Atoms to Astronomy

52Slide53

Atoms to Astronomy

53Slide54

Atoms to Astronomy

54Slide55

55

page 5 5 4 | N AT U R E | VO L 4 9 7 | 3 0 M AY 2 0 1 3 Slide56

Atoms to Astronomy

56This is an artist’s impression of the galaxy Z8-GND-5296. Image credit: V. Tilvi / S.L. Finkelstein / C. Papovich

/ the Hubble Heritage TeamZ8-GND-5296 is forming stars extremely rapidly – producing each year about 300 times the mass of our Sun. By comparison, our Milky Way Galaxy forms only 2 – 3 stars per year.Even galaxies observed at a time when the Universe had reached only 5% of its current age may already be chemically enriched with dust and heavy elements, which must have been produced by an earlier generation of stars.

Finkelstein, S. L. et al. Nature 502,

524–527 (2013

); see also

Riecher

24 October 2013, Nature, 502, 459

Slide57

57

Cosmic clockEvent

timeredshift

H and He formation

3 min.

10

9

Recombination

400,000 yr

1,500

The first stars

400

Myr

10

Reionization

400

Myr

9

The first galaxies

0.7

Gyr

6.5

Today

13.7 Gyr

0Slide58

Dark

Energy58Slide59

Atoms to Astronomy

59Slide60

Atoms to Astronomy

60Slide61

Atoms to Astronomy

61~ 2 billion years agoSlide62

Atoms to Astronomy

62MatterStrength of the repulsive force in the UniverseSlide63

Atoms to Astronomy

634%21 %

75%Slide64

Atoms to Astronomy

64Slide65

Origin of elements in the UniverseSlide66

Atoms to Astronomy

66Slide67

Atoms to Astronomy

67

Synthesis of elementsSlide68

Atoms to Astronomy

68

Limits to production of heavy elements in the Universe: The Binding energy curveSlide69

Atoms to Astronomy

69Slide70

Atoms to Astronomy

70Slide71

Atoms to Astronomy

71

Abundance of matter in the UniverseSlide72

How will the universe end?Slide73

Dark is more important than brightSlide74

Distance from Centre

Rotational velocity (km/s)Slide75
Slide76
Slide77
Slide78
Slide79
Slide80

Cosmic clock

Event

timeredshift

H and He formation

3 min.

10

9

Recombination

400,000 yr

1,500

The first stars

400 Myr

10

Reionization

500 Myr

9

The first galaxies

0.8 Gyr

6.5

Today

13.7 Gyr

0Slide81

Star formation through time

Madau plot (Cole et al. 2001)

Cosmic timeSlide82
Slide83
Slide84

~ 2 billion years agoSlide85

4%

26 %

60%Slide86
Slide87

I should have stopped long back

Atoms to Astronomy87Slide88

END