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Way-out to the gravitino problem in intersecting D-brane Pati-Salam models

机译:相交D轴帕蒂·萨拉姆(Pati-Salam)模型中引力问题的出路

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We discuss the gravitino problem in the context of the exotic see-saw mechanism for neutrinos and leptogenesis, UV completed by intersecting D-branes Pati-Salam models. In the exotic see-saw model, supersymmetry is broken at high scales MSUSY >10(9) GeV and this seems in contradiction with gravitino bounds from inflation and baryogenesis. However, if gravitino is the lightest stable supersymmetric particle, it will not decay into other SUSY particles, avoiding the gravitino problem and providing a good cold dark matter (CDM). Gravitini are super heavy dark particles and they can be produced by non-adiabatic expansion during inflation. Intriguingly, from bounds on the correct abundance of dark matter (DM), we also constrain the neutrino sector. We set a limit on the exotic instantonic coupling of <10(-2)-10(-3). This also sets constrains on the Calabi-Yau compactifications and on the string scale. This model strongly motivates very high energy DM indirect detection of neutrini and photons of 10(11)-10(13) GeV: gravitini can decay on them in a cosmological time because of soft R-parity breaking effective operators.
机译:我们讨论中微子和瘦素的异域跷跷板机制的上下文中的gravitino问题,通过相交D轴Pati-Salam模型完成的UV。在异乎寻常的跷跷板模型中,超对称在MSUSY> 10(9)GeV的高比例下被打破,这似乎与通货膨胀和重生作用产生的引力线边界相矛盾。但是,如果gravitino是最轻的稳定超对称粒子,则不会衰减成其他SUSY粒子,从而避免了gravitino问题并提供了良好的冷暗物质(CDM)。 Gravitini是超重的深色颗粒,可以在充气过程中通过非绝热膨胀产生。有趣的是,从正确的暗物质丰度(DM)的界限出发,我们还限制了中微子区域。我们对<10(-2)-10(-3)的奇异瞬时耦合进行了限制。这也限制了Calabi-Yau压实和细绳规模。该模型强烈激发了非常高能量的DM间接检测10(11)-10(13)GeV的中微子和光子:由于软R奇偶性破坏了有效算子,因此引力子可以在宇宙学时间内衰减它们。

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