Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Isotopes of boron

From Wikipedia, the free encyclopedia

icon
This articleneeds additional citations forverification. Please helpimprove this article byadding citations to reliable sources. Unsourced material may be challenged and removed.
Find sources: "Isotopes of boron" – news ·newspapers ·books ·scholar ·JSTOR
(May 2018) (Learn how and when to remove this message)
Isotopes ofboron (5B)
Main isotopes[1]Decay
Isotopeabun­dancehalf-life(t1/2)modepro­duct
8Bsynth771.9 msβ+8Be
10B[18.9%, 20.4%]stable
11B[79.6%, 81.1%]stable
Standard atomic weightAr°(B)

Boron (5B) naturally occurs asisotopes10
B
and11
B
, the latter of which makes up about 80% of natural boron. There are 13radioisotopes that have been discovered, with mass numbers from 7 to 21, all with shorthalf-lives, the longest being that of8
B
, with a half-life of only771.9(9) ms and12
B
with a half-life of20.20(2) ms. All other isotopes have half-lives shorter than17.35 ms. Those isotopes with mass below 10 decay intohelium (via short-livedisotopes of beryllium for7
B
and9
B
) while those with mass above 11 mostly becomecarbon.

List of isotopes

[edit]
Nuclide
[n 1]
ZNIsotopic mass(Da)[4]
[n 2][n 3]
Half-life[1]

[resonance width]
Decay
mode
[1]
[n 4]
Daughter
isotope

[n 5]
Spin and
parity[1]
[n 6][n 7]
Natural abundance(mole fraction)
Excitation energyNormal proportion[1]Range of variation
7
B
527.029712(27)570(14) ys
[801(20) keV]
p6
Be
[n 8]
(3/2−)
8
B
[n 9][n 10]
538.0246073(11)771.9(9) msβ+α4
He
2+
8m
B
10624(8) keV0+
9
B
549.0133296(10)800(300) zsp8
Be
[n 11]
3/2−
10
B
[n 12]
5510.012936862(16)Stable3+[0.189,0.204][5]
11
B
5611.009305167(13)Stable3/2−[0.796,0.811][5]
11m
B
12560(9) keV1/2+, (3/2+)
12
B
5712.0143526(14)20.20(2) msβ (99.40(2)%)12
C
1+
βα (0.60(2)%)8
Be
[n 13]
13
B
5813.0177800(11)17.16(18) msβ (99.734(36)%)13
C
3/2−
βn (0.266(36)%)12
C
14
B
5914.025404(23)12.36(29) msβ (93.96(23)%)14
C
2−
βn (6.04(23)%)13
C
β2n ?[n 14]12
C
 ?
14m
B
17065(29) keV4.15(1.90) zsIT ?[n 14]0+
15
B
51015.031087(23)10.18(35) msβn (98.7(1.0)%)14
C
3/2−
β (<1.3%)15
C
β2n (<1.5%)13
C
16
B
51116.039841(26)>4.6 zsn ?[n 14]15
B
 ?
0−
17
B
[n 15]
51217.04693(22)5.08(5) msβn (63(1)%)16
C
(3/2−)
β (21.1(2.4)%)17
C
β2n (12(2)%)15
C
β3n (3.5(7)%)14
C
β4n (0.4(3)%)13
C
18
B
51318.05560(22)<26 nsn17
B
(2−)
19
B
[n 16]
51419.06417(56)2.92(13) msβn (71(9)%)18
C
(3/2−)
β2n (17(5)%)17
C
β3n (<9.1%)16
C
β (>2.9%)19
C
20
B
[6]
51520.07451(59)>912.4 ysn19
B
(1−, 2−)
21
B
[6]
51621.08415(60)>760 ys2n19
B
(3/2−)
This table header & footer:
  1. ^mB – Excitednuclear isomer.
  2. ^( ) – Uncertainty (1σ) is given in concise form in parentheses after the corresponding last digits.
  3. ^# – Atomic mass marked #: value and uncertainty derived not from purely experimental data, but at least partly from trends from the Mass Surface (TMS).
  4. ^Modes of decay:
    n:Neutron emission
    p:Proton emission
  5. ^Bold symbol as daughter – Daughter product is stable.
  6. ^( ) spin value – Indicates spin with weak assignment arguments.
  7. ^# – Values marked # are not purely derived from experimental data, but at least partly from trends of neighboring nuclides (TNN).
  8. ^Subsequently decays by double proton emission to4
    He
    for a net reaction of7
    B
    4
    He
    + 3 1
    H
  9. ^Has 1halo proton
  10. ^Intermediate product ofa branch of proton–proton chain in stellar nucleosynthesis as part of the process converting hydrogen to helium
  11. ^Immediately decays into two α particles, for a net reaction of9
    B
    → 2 4
    He
    +1
    H
  12. ^One of the few stableodd-odd nuclei
  13. ^Immediately decays into two α particles, for a net reaction of12
    B
    → 3 4
    He
    +e
  14. ^abcDecay mode shown is energetically allowed, but has not been experimentally observed to occur in this nuclide.
  15. ^Has 2 halo neutrons
  16. ^Has 4 halo neutrons

Boron-8

[edit]

Boron-8 is an isotope of boron that undergoes β+ decay toberyllium-8 with a half-life of771.9(9) ms. It is the strongest candidate for ahalo nucleus with a loosely-bound proton, in contrast to neutron halo nuclei such aslithium-11.[7]

Although boron-8 beta decayneutrinos from the Sun make up only about 80 ppm of the totalsolar neutrino flux, they have a higher energy centered around 10 MeV,[8] and are an important background to dark matterdirect detection experiments.[9] They are the first component of the neutrino floor that dark matter direct detection experiments are expected to eventually encounter.

Applications

[edit]

Boron-10

[edit]

Boron-10 is used inboron neutron capture therapy as an experimental treatment of some brain cancers.

See also

[edit]

Daughter products other than boron

References

[edit]
  1. ^abcdeKondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S.; Audi, G. (2021)."The NUBASE2020 evaluation of nuclear properties"(PDF).Chinese Physics C.45 (3) 030001.doi:10.1088/1674-1137/abddae.
  2. ^"Standard Atomic Weights: Boron".CIAAW. 2009.
  3. ^Prohaska, Thomas; Irrgeher, Johanna; Benefield, Jacqueline; Böhlke, John K.; Chesson, Lesley A.; Coplen, Tyler B.; Ding, Tiping; Dunn, Philip J. H.; Gröning, Manfred; Holden, Norman E.; Meijer, Harro A. J. (2022-05-04)."Standard atomic weights of the elements 2021 (IUPAC Technical Report)".Pure and Applied Chemistry.doi:10.1515/pac-2019-0603.ISSN 1365-3075.
  4. ^Wang, Meng; Huang, W.J.; Kondev, F.G.; Audi, G.; Naimi, S. (2021). "The AME 2020 atomic mass evaluation (II). Tables, graphs and references*".Chinese Physics C.45 (3) 030003.doi:10.1088/1674-1137/abddaf.
  5. ^ab"Atomic Weight of Boron".CIAAW.
  6. ^abLeblond, S.; et al. (2018). "First observation of20B and21B".Physical Review Letters.121 (26): 262502–1–262502–6.arXiv:1901.00455.doi:10.1103/PhysRevLett.121.262502.PMID 30636115.S2CID 58602601.
  7. ^Maaß, Bernhard; Müller, Peter; Nörtershäuser, Wilfried; Clark, Jason; Gorges, Christian; Kaufmann, Simon; König, Kristian; Krämer, Jörg; Levand, Anthony; Orford, Rodney; Sánchez, Rodolfo; Savard, Guy; Sommer, Felix (November 2017). "Towards laser spectroscopy of the proton-halo candidate boron-8".Hyperfine Interactions.238 (1): 25.Bibcode:2017HyInt.238...25M.doi:10.1007/s10751-017-1399-5.S2CID 254551036.
  8. ^Bellerive, A. (2004). "Review of solar neutrino experiments".International Journal of Modern Physics A.19 (8):1167–1179.arXiv:hep-ex/0312045.Bibcode:2004IJMPA..19.1167B.doi:10.1142/S0217751X04019093.S2CID 16980300.
  9. ^Cerdeno, David G.; Fairbairn, Malcolm; Jubb, Thomas; Machado, Pedro; Vincent, Aaron C.; Boehm, Celine (2016). "Physics from solar neutrinos in dark matter direct detection experiments".JHEP.2016 (5): 118.arXiv:1604.01025.Bibcode:2016JHEP...05..118C.doi:10.1007/JHEP05(2016)118.S2CID 55112052.
Group12 3456789101112131415161718
PeriodHydrogen and
alkali metals
Alkaline
earth metals
Pnicto­gensChal­co­gensHalo­gensNoble gases
12
345678910
1112131415161718
192021222324252627282930313233343536
373839404142434445464748495051525354
55561 asterisk71727374757677787980818283848586
87881 asterisk103104105106107108109110111112113114115116117118
119120
1 asterisk5758596061626364656667686970 
1 asterisk8990919293949596979899100101102
International
National
Other


https://borates.today/isotopes-a-comprehensive-guide/#:~:text=Boron%20isotope%20elements%20with%20masses,11%20mostly%20decay%20into%20carbon.

Retrieved from "https://en.wikipedia.org/w/index.php?title=Isotopes_of_boron&oldid=1326780251"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp