Lecture 5

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Special  &  General  Relativity

HW  1  due  Thursday  at   start  of  class.  

  Questions?  

  Nicholas  Erickson:    MW  10-­‐11  am,  E122  

  Jeremy  Darling:    TR  11-­‐noon,  C323B  

Read  Thorne  Chapter  2

Equivalence  of   mass  and  energy

Newton

Mass  and  energy  are  entirely  different  things:

•  Mass  

  -­‐  inertial  mass  

  -­‐  gravitational  mass  

•  Energy  

  -­‐  related  to  independent  properties  of    

    the  object  (how  hot  it  is  –  “thermal  

    energy”,  how  fast  moving  –  “kinetic  

    energy”  etc)

Einstein

Consequence  of  special  relativity:  energy  and   mass  are  equivalent

Energy  is  proportional  to  the  mass,  with  the     scaling  factor  being  speed  of  light  squared:

E = mc 2

Even  less  obvious  when  we  work  out  numbers!  

E

=

1 kg

×

(

×

10 8 m s -1

)

2

= 9 × 10 16 Joules

How  big  is  a  Joule?  

A  power  of  one  Watt  is  one  Joule  per  second  

Total  US  electrical  production  per  day  is  about  

4  x  10 16  Joules  

E = 1 kg ×

(

× 10 8 m s -1

2

)

=

9

×

10 16 Joules this  energy  is  equivalent  to  ~0.5  kg  of  matter  

Efficiency  of

E = mc 2

Fusion  

Fission  

Black  Holes  

Annihilation

Efficiency  of  nuclear  reactions

In  the  Sun,  nuclear  fusion

4  x

protons  

(hydrogen  nuclei)

2  protons  +  2  neutrons  

(helium  nucleus)

Mass  of  a  helium  nucleus  is  0.7%   less   than   the  mass  of  4  protons:  reaction  releases  energy

4  x

1  kg  of     hydrogen

0.993  kg  of   helium energy  equivalent  of  

0.007  kg  =  6.3  x  10 14    

Joules

Enormous  energy:  600  million  tons  per  second  of     hydrogen  fusing  to  helium  provide  the  Sun’s   luminosity  (power)

Generally:  structure  of  nuclei   means  that  fusion  of  “light”   elements  toward  iron  releases   energy

Fission   (splitting)  of  heavy     elements  also  releases   energy,  but  less  as  a  fraction   of  the  mass  involved  

Fusion  reactions  are  hard…

+ + positive  charges   repel   deuterium

Requires  very  high  temperatures  (15  million   degrees  in  the  Sun)  to  force  protons  to  collide   and  fuse

Fission  reactions:

•  can  occur  spontaneously  for  some  heavy    

  elements  (e.g.  uranium)  

•  can  release  neutrons  that  trigger  additional  

  fission  reactions

Oklo  natural  nuclear  reactor

Efficiency  of  accretion

Gas  spiraling  toward  a  black  hole  also  releases   energy  as  it  falls  deeper  into  the  gravitational  field  

Active  ~1.7  billion   years  ago  in  Gabon

…important  test  that  constants  of  Nature  have  

  actually  been  constant  over  a  long  time!

Efficiency  of  accretion

1  kg  of  gas  at  large   distance  from  hole

Characterize  as  fraction   of  the  mass  falling  in:   about  10%   (depending   on  spin  of  black  hole) increases  mass  of   hole  by  0.9  kg   release  energy   equivalent  of  0.1  kg

Efficiencies

Nuclear  fusion :  0.7%  (hydrogen  to  helium)

Black  hole  accretion :  ~10%  (no  fusion  involved)

About  10-­‐20  times  more  efficient:  why     black  holes  are  important  in   astronomy

Annihilation

Paul  Dirac  predicted  that  the     electron  should  have  an     anti-­‐particle

Later  discovered:  the   positron  

(same  mass,  opposite  electric   charge)

Other  examples  of  anti-­‐matter:  proton  /  anti-­‐   proton,  hydrogen  /  anti-­‐hydrogen  (hard  to  make!)

Chris  Fragile

Annihilation

photons  (energy   equal  to  rest  mass   of  electron  +     positron,   plus  any     kinetic  energy)   matter:  particle   and  anti-­‐particle

Only  process  allowing  100%  efficient  conversion   of  mass  into  its  equivalent  energy

What  about  gravity?

e -­‐ e +

Gravitational  effect  doesn’t  care  if  it’s  matter     or  energy:  just  the  same  thing

General  Relativity

Special  relativity  (1905)

General  Relativity:  motivation

F =

GMm d 2

Newtonian  gravity  is   inversely  proportional     to   the  instantaneous   distance  squared

Relativity:  distances     and  simultaneity  are   not  universal

General  relativity  (1915)

General  Relativity:  motivation

Ellipse  of  Mercury’s  orbit   precesses,  mostly  because   of  perturbations  from     other  planets  

!

But   43  arcseconds  (1/3600   of  a  degree)  of  precession   per  century  is  unexplained   in  Newtonian  gravity

The  “happiest  thought  of  my  life”

If  a  person  falls  freely,  he  will     not  feel  his  own  weight.

Einstein,  1907

Principle  of  Equivalence

freely   falling   box box  moving     uniformly   through  space

Principle  of  Equivalence

stationary  in  a     gravitational     field accelerating   in  empty  space

Principle  of  Equivalence

Laws  of  physics  in  a   small  freely  falling     frame  are  indistinguishable  from  those   in  a  uniformly  moving  frame  in  a     gravity-­‐free  Universe   and

Laws  of  physics  in  a   small  accelerating   frame  are  indistinguishable  from  those   in  a  stationary  frame  in  a  gravitational   field

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