We have recently pointed out [1] that the string swampland conjectures [2], if true, provide important constraints on dark energy models. The constraints apply to the field range of a scalar field Φ described by an e...We have recently pointed out [1] that the string swampland conjectures [2], if true, provide important constraints on dark energy models. The constraints apply to the field range of a scalar field Φ described by an effective field theory, and to the slope of the potential Ⅴ of such fields.展开更多
基金supported by the Funding from the European Research Council(ERC)under the European Unions Horizon 2020 Research and Innovation Program(Grant No.801781)the Swiss National Science Foundation(Grant No.1797400)+1 种基金an NSERC Discovery Grantthe Canada Research Chair Program
文摘We have recently pointed out [1] that the string swampland conjectures [2], if true, provide important constraints on dark energy models. The constraints apply to the field range of a scalar field Φ described by an effective field theory, and to the slope of the potential Ⅴ of such fields.
