English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Tools annual

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

Within a supersymmetric (SUSY) type-I seesaw framework with flavor-blinduniversal boundary conditions, we study the consequences of requiring that theobserved baryon asymmetry of the Universe be explained by either thermal ornon-thermal leptogenesis. In the former case, we find that the parameter spaceis very constrained. In the bulk and stop-coannihilation regions of mSUGRAparameter space (that are consistent with the measured dark matter abundance),lepton flavor-violating (LFV) processes are accessible at MEG and futureexperiments. However, the very high reheat temperature of the Universe neededafter inflation (of about 10^{12} GeV) leads to a severe gravitino problem,which disfavors either thermal leptogenesis or neutralino dark matter.Non-thermal leptogenesis in the preheating phase from SUSY flat directionsrelaxes the gravitino problem by lowering the required reheat temperature. Thebaryon asymmetry can then be explained while preserving neutralino dark matter,and for the bulk or stop-coannihilation regions LFV processes should beobserved in current or future experiments.

Examining leptogenesis with lepton flavor violation and the dark matter abundance