Nucleonics Matrix



Nuclear Stability

By Alain Lareau

Chapter 2 Page 1

Integrated Cause
Composite Effect


All Isobars to six
H-1


H-2


He-3


H-3


Li-4


He-4


H-4


Li-5


He-5


Be-6


Li-6


He-6


I tend to view all the neutrons and protons of an atomic nucleus, while they exist in and as the nucleus the same. That is I do not view them as charge specific nor quark composite specific. I view them as fluid to some degree. The quality that I do impart to them is they still must fill space, and so I tend to the use of the term "isobar" instead of isotope. While we use tools and techniques to determine the size and shape of atomic nuclei we certainly can imagine that we are interacting with a positron cloud. The Platonic and Archimedeian solids are omnipresent in nature representing equal division of a sphere. Can not a soap bubble oscillate somewhat, can we suppose atomic nuclei do something similar


 Isotope Relative
Atomic Mass 
 Isotopic
  Composition  
Standard
Atomic Weight 
  Notes 
1 H 1       1.007 825 032 1(4)   99.9885(70) 1.007 94(7) g,m,r,c,w
D   2     2.014 101 778 0(4)   0.0115(70)
T     3   3.016 049 2675(11)   

2 He 3       3.016 029 309 7(9)   0.000 137(3) 4.002 602(2) g,r,a
  4     4.002 603 2497(10)   99.999 863(3)

3 Li   6     6.015 122 3(5)   7.59(4) 6.941(2) g,m,r,b,d
    7   7.016 004 0(5)   92.41(4)

4 Be     9   9.012 182 1(4)   100 9.012 182(3)  

5 B   10     10.012 937 0(4)   19.9(7) 10.811(7) g,m,r
    11   11.009 305 5(5)   80.1(7)

6 C   12     12.000 000 0(0)   98.93(8) 12.0107(8) g,r
    13   13.003 354 8378(10)   1.07(8)
      14 14.003 241 988(4)   

7 N   14     14.003 074 005 2(9)   99.632(7) 14.0067(2) g,r,e
    15   15.000 108 898 4(9)   0.368(7)

8 O   16    15.994 914 6221(15)   99.757(16) 15.9994(3) g,r
    17   16.999 131 50(22)   0.038(1)
      18 17.999 160 4(9)   0.205(14)

9 F     19   18.998 403 20(7)   100 18.998 403 2(5)  

10 Ne   20     19.992 440 1759(20)   90.48(3) 20.1797(6) g,m,r,a
    21   20.993 846 74(4)   0.27(1)
      22 21.991 385 51(23)   9.25(3)

11 Na     23   22.989 769 67(23)   100 22.989 770(2)  


n =
p-1p p+1p+2 p+3p+4
H 1   n    
  H 2      
He 3   H 3     
  He 4      
        
  Li 6      
Be 7   Li 7     
        
   Be 9     
  B 10   Be 10   
   B 11     
  C 12      
   C 13     
  N 14   C 14   
   N 15     
  O 16      
   O 17     
     O 18   
   F 19     
  Ne 20      
   Ne 21     
     Ne 22   
   Na 23     
The Incremental Tables are available for your use as you see fit. There are at least three immediate paths of invetigation you may take to acquaint your self with what The Incremental Table format can do for you.
One path of investigation could be to flesh out a table by adding all the radionuclides row by row starting with the short tables.

Stable Isobars to (4)

n = p-1 n = p
001 99.985%

SUPER Stable

1.007825
 
  002 0.015%

Stable

2.0141017
003 0.000137%

Stable

3.0160293
 
  004 99.999863%

SUPER Stable

4.0026032
4c - - 6a
A different path could be to examine the pattern of all stable Nuclides in incrementing Isobar rows without labels.



A third path would be, as I suggest below, is to begin with elements
appraised as most abundant and add in the less plentiful
as they rank in abundance. The chart crust displays
the most abundant elements of the earth's crust in the left column, in the right column the elements are reoganized in order of atomic number.

See Crust --- --- Next