TY  -  
T1  - UV freeze-in in Starobinsky inflation 
SN  -  /  
UR  - http://hdl.handle.net/10138/335061 
T3  -  
A1  - Bernal, Nicolas; Rubio, Javier; Veermäe, Hardi 
A2  -  
PB  -  
Y1  - 2020 
LA  - eng 
AB  - In the Starobinsky model of inflation, the observed dark matter abundance can be produced from the direct decay of the inflaton field only in a very narrow spectrum of closeto-conformal scalar fields and spinors of mass similar to 10(7) GeV. This spectrum can be, however, significantly broadened in the presence of effective non-renormalizable interactions between the dark and the visible sectors. In particular, we show that UV freeze-in can efficiently generate the right dark matter abundance fo... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - dark matter theory; inflation; particle physics - cosmology connection; physics of the early universe; SCALAR-FIELD; DARK-MATTER; GRAVITY; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -