We present a generic framework, "baryomorphosis", which modifies the baryonasymmetry to be naturally of the order of a typical thermal relic WIMP density.We consider a simple scalar-based model to show how this is possible. Thismodel introduces a sector in which a large initial baryon asymmetry is injectedinto particles ("annihilons") phi_B, \bar{phi}_B of mass ~ 100 GeV - 1 TeV.phi_B-\bar{phi}_B annihilations convert the initial phi_B, \bar{phi}_Basymmetry to a final asymmetry with a thermal relic WIMP-like density. Thissubsequently decays to a conventional baryon asymmetry whose magnitude isnaturally related to the density of thermal relic WIMP dark matter. In this waythe two coincidences of baryons and dark matter i.e. why their densities aresimilar to each other and why they are both similar to a WIMP thermal relicdensity (the "WIMP miracle"), may be understood. The model may be tested by theproduction of annihilons at colliders.
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机译：我们提出了一个通用的框架“重态变态”，将重对称性自然地修改为典型的热文物WIMP密度的数量级。我们考虑一个基于标量的简单模型来说明这是可能的。此模型引入了一个扇区，在该扇区中，将大的初始重子不对称性注入到质量为100 GeV〜1 GeV的\ bar {phi} _B的粒子（“ \灭”）中phi_B- \ bar {phi} _B an灭会转换初始phi_B， \ bar {phi} _Basymmetry到最终不对称，且具有类似WIMP的热密度。因此，这会衰减为常规的重子不对称性，其大小自然与热文物WIMP暗物质的密度有关。以这种方式，可以理解重子和暗物质的两个巧合，即为什么它们的密度彼此相似，以及为什么它们都与WIMP热残余密度（“ WIMP奇迹”）相似。该模型可以通过在对撞机上产生无环数来进行测试。
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