| 000 | 02981nlm1a2200373 4500 | ||
|---|---|---|---|
| 001 | 660181 | ||
| 005 | 20231030041656.0 | ||
| 035 | _a(RuTPU)RU\TPU\network\29165 | ||
| 090 | _a660181 | ||
| 100 | _a20190506a2018 k y0engy50 ba | ||
| 101 | 0 |
_aeng _deng |
|
| 135 | _adrcn ---uucaa | ||
| 181 | 0 | _ai | |
| 182 | 0 | _ab | |
| 200 | 1 |
_aGravitino and Polonyi production in supergravity _fA. Addazi, S. V. Ketov, M. Yu. Khlopov |
|
| 203 |
_aText _celectronic |
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| 300 | _aTitle screen | ||
| 320 | _a[References: 71 tit.] | ||
| 330 | _aWe study production of gravitino and Polonyi particles in the minimal Starobinsky-Polonyi N=1N=1 supergravity with inflaton belonging to a massive vector supermultiplet. Our model has only one free parameter given by the scale of spontaneous SUSY breaking triggered by Polonyi chiral superfield. The vector supermultiplet generically enters the action non-minimally, via an arbitrary real function. This function is chosen to generate the inflaton scalar potential of the Starobinsky model. Our supergravity model can be reformulated as an abelian supersymmetric gauge theory with the vector gauge superfield coupled to two (Higgs and Polonyi) chiral superfields interacting with supergravity, where the U(1) gauge symmetry is spontaneously broken. We find that Polonyi and gravitino particles are efficiently produced during inflation, and estimate their masses and the reheating temperature. After inflation, perturbative decay of inflaton also produces Polonyi particles that rapidly decay into gravitinos. As a result, a coherent picture of inflation and dark matter emerges, where the abundance of produced gravitinos after inflation fits the CMB constraints as a Super Heavy Dark Matter (SHDM) candidate. Our scenario avoids the notorous gravitino and Polonyi problems with the Big Bang Nucleosynthesis (BBN) and DM overproduction. | ||
| 461 |
_tThe European Physical Journal C _oScientific Journal |
||
| 463 |
_tVol. 78, iss. 8 _v[642, 40 р.,] _d2018 |
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| 610 | 1 | _aэлектронный ресурс | |
| 610 | 1 | _aтруды учёных ТПУ | |
| 610 | 1 | _aгравитирующие тела | |
| 610 | 1 | _aполоний | |
| 610 | 1 | _aсупергравитация | |
| 700 | 1 |
_aAddazi _bA. _gAndrea |
|
| 701 | 1 |
_aKetov _bS. V. _cphysicist _cChief Expert of Tomsk Polytechnic University, Candidate of physical and mathematical sciences _f1960- _gSergey Vladimirovich _2stltpush _3(RuTPU)RU\TPU\pers\36631 |
|
| 701 | 1 |
_aKhlopov _bM. Yu. _gMaksim Yurjevich |
|
| 712 | 0 | 2 |
_aНациональный исследовательский Томский политехнический университет _bИсследовательская школа физики высокоэнергетических процессов _c(2017- ) _h8118 _2stltpush _3(RuTPU)RU\TPU\col\23551 |
| 801 | 2 |
_aRU _b63413507 _c20200124 _gRCR |
|
| 856 | 4 | _uhttp://earchive.tpu.ru/handle/11683/57553 | |
| 856 | 4 | _uhttps://doi.org/10.1140/epjc/s10052-018-6111-7 | |
| 942 | _cCF | ||