Model calculations for laser action in He
i are carried out, when helium plasma is rapidly cooled by expansion. Results are presented for four transitions, two of which, 3
1
S
2
1
P
0 (

7281) and 3
1
D
2
1
P
0 (

6678), show strong population inversion. Available observational evidence for possible laser action in these two lines in Wolf-Rayet and emission-line stars is summarized and discussed.