| 000 | 02140nlm1a2200409 4500 | ||
|---|---|---|---|
| 001 | 669489 | ||
| 005 | 20231030042224.0 | ||
| 035 | _a(RuTPU)RU\TPU\network\40729 | ||
| 035 | _aRU\TPU\network\37744 | ||
| 090 | _a669489 | ||
| 100 | _a20230518a2022 k y0engy50 ba | ||
| 101 | 0 | _aeng | |
| 135 | _aarcn ---uucaa | ||
| 181 | 0 | _ai | |
| 182 | 0 | _ab | |
| 200 | 1 |
_aConstraints on the appearance of a maximum in astrophysical S-factor _fV. V. Sargsyan, G. G. Adamyan, N. V. Antonenko, H. Lenske |
|
| 203 |
_aText _celectronic |
||
| 300 | _aTitle screen | ||
| 320 | _a[References.: 38 tit.] | ||
| 330 | _aFor fusion reactions of astrophysical interest, the existence of a maximum of S-factor is revealed within the extended quantum diffusion approach. The available experimental data are well described. The reason and consequences of the existence of the S-factor maximum are explained. An universal formula for the position of the maximum is proposed. | ||
| 461 | _tPhysics Letters B | ||
| 463 |
_tVol. 824 _v[136792, 5 p.] _d2022 |
||
| 610 | 1 | _aэлектронный ресурс | |
| 610 | 1 | _aтруды учёных ТПУ | |
| 610 | 1 | _aastrophysical S-factor | |
| 610 | 1 | _adeep sub-barrier fusion (capture) | |
| 610 | 1 | _adissipative dynamics | |
| 610 | 1 | _aастрофизический S-фактор | |
| 610 | 1 | _aдиссипативная динамика | |
| 701 | 1 |
_aSargsyan _bV. V. _gVazgen Valerikovich |
|
| 701 | 1 |
_aAdamyan _bG. G. _gGurgen Grigorjevich |
|
| 701 | 1 |
_aAntonenko _bN. V. _cphysicist _cProfessor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences _f1964- _gNikolay Viktorovich _2stltpush _3(RuTPU)RU\TPU\pers\35905 |
|
| 701 | 1 |
_aLenske _bH. _gHorst |
|
| 712 | 0 | 2 |
_aНациональный исследовательский Томский политехнический университет _bШкола базовой инженерной подготовки _bОтделение математики и информатики _h8031 _2stltpush _3(RuTPU)RU\TPU\col\23555 |
| 801 | 2 |
_aRU _b63413507 _c20230518 _gRCR |
|
| 856 | 4 | _uhttps://doi.org/10.1016/j.physletb.2021.136792 | |
| 942 | _cCF | ||