Copyright - Karim A. Khaidarov, 2003. Updated August 1, 2003

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1998 Ω Λ 42 ( .) [1] Supernova Cosmology Project Calan/Tololo Supernova Survey.

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- :

hν = hνo e Ht ,

(1)

h - ,
      νo ,
      ν t,
      H ( ),
      t - .

:

z = λ / λ0 - 1 = ν0 / ν - 1 ,

(2)

λ ,
      λ0 ,
      ν ,
      ν0 .

(1) (2) t z

t = ln(z+1) / H ,

(3)

W = t2 2,512 M1 m x peak ,

t ,
      2,512 ,
      M1 , 1 ,
      m x peak .

[1] (1). Ia

M0 aver = M1 2,5 lg(108/3,263)2 = -18,5

1 (3) [1], 1.

z , 390 / 0,0013 .


.1 52 . ]
H = 72 / ( ).

(1) Ia 1973 2003 [2] , M0 0,8 . , , " ".

, 2 ( 2).


. 2. 433 [.]
H = 72 / ( ).

[1] , . M0 -0,182 .

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2,73 0K, , :

R = c ln(T/T0) / H ,

c ,
      T ,
      H , 72 [ / ( )]
      T0 2,73 0K.

, 6000 0K

R = 13,6 ln(6000/2,73) = 105 [. . ]

" ", 500 . [3]. , .. (1).

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"" . , 1961 .

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" ", - - " ". "" , 2,73 0K. , [4].

(1) , , .

:

  1. Measurements of Ω and Λ from 42 high-redshift supernovae. - S. Perlmutter et al., 1998
  2. , .. , .., .., .., 2003.
  3. A correlation of the cosmic microwave sky with large scale structure. S. Boughn & R. Crittenden, 2003
  4. . ., . ., . . , - : - . -, 1996. - 120 .

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, 1974 - 1980 . , , , , 360±30 /, - . , "Deutsche Physik", . FAQ .

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