dyooteeriym
| haaidrojan-2 | |
|---|---|
 Full table
|
|
| saamaanya | |
| naam, chinh | dyooteriym, 2H ya D |
| nyootraun | 1 |
| proton | 1 |
| nyooklaaid aankade | |
| praakrutik prachurata | 0.015% |
| ardhaayu | sthir |
| samasthaanik dravyamn | 2.014101779 u |
| spin | 1+ |
| atirikt oorja | 13,135.72±0.1 keV |
| baainding oorja | 2,224.52±0.2 keV |
dyooteeriym athva dyooteriym haaidrojan ka ek sthir samasthaanik hai. iski praakrutik upalabdhata pruthvi ke saagaraon mein haaidrojan ke lagbhag ek parmaanu prati 6,500 (~154 ppm) hai.
pratidyooteeriym
pratidyooteeriym, dyooteeriym ke naabhik pratikn hai jismein ek pratiproton tatha ek pratinyootraun hota hai. pratidyooteeriym ka sarvapratham nirmaan 1965 mein sarn sthit proton sinkotraun[1] tatha brookahaivan raashtreeya prayogashaala sthit altaraneting grediyent sinkotraun mein kiya gaya.[2] pojeetraun sahit ek poorn parmaanu ko pratidyooteeriym kaha jaata hai lekin 2013 tak iska nirmaan sambhav naheenho paaya. pratidyooteeriym ke liye prastaavit prateek chinh D hai jo angreji akshar D ke upar rekha lagaane par praapt hota hai.[3]
sandarbh
- ↑ Massam, T; Muller, Th.; Righini, B.; Schneegans, M.; Zichichi, A. (1965). "Experimental observation of antideuteron production". Il Nuovo Cimento 39: 10–14. Bibcode 1965NCimS..39...10M. doi:10.1007/BF02814251.
- ↑ Dorfan, D. E; Eades, J.; Lederman, L. M.; Lee, W.; Ting, C. C. (June 1965). "Observation of Antideuterons". Phys. Rev. Lett. 14 (24): 1003–1006. Bibcode 1965PhRvL..14.1003D. doi:10.1103/PhysRevLett.14.1003.
- ↑ Chardonnet, P; Orloff, Jean; Salati, Pierre (1997). "The production of anti-matter in our galaxy". Physics Letters B 409: 313. arXiv:astro-ph/9705110. Bibcode 1997PhLB..409..313C. doi:10.1016/S0370-2693(97)00870-8.
| halka: haaidrojan 1 |
dyooteeriym haaidrojan ka samasthaanik hai |
bhaari: haaidrojan 3 |
|
dekhein proton kshaya ka kshaya utpaad |
dyooteeriym ki kshaya shrunkhala |
sthir ke kshaya |