The impact of axion-like particles on late stellar evolution - From intermediate-mass stars to core-collapse supernova progenitors

Open Access

Table 1.

Impact of ALPs on the minimum mass for off-center C ignition.

g₁₀	g₁₃	$M_{COWD}^{\max}$ $M^{\mathrm{max}}_{\mathrm{COWD}}$	M_CO	Age	X_C
0.0	0.0	7.5	1.064	43.5	0.203
0.0	1.5	8.0	1.089	37.9	0.216

0.2	0.0	8.0	1.101	37.9	0.216
0.2	1.5	8.2	1.104	36.0	0.227

0.4	0.0	8.2	1.099	35.9	0.225
0.4	1.5	8.4	1.104	34.1	0.241

0.6	0.0	8.4	1.095	33.9	0.235
0.6	1.5	8.5	1.104	33.1	0.241

0.6	4.0	9.2	1.155	28.2	0.239

Notes. Columns: ALP-photon coupling strength, ALP-electron coupling strength, $M_{COWD}^{\max}$ $M^{\mathrm{max}}_{\mathrm{COWD}}$ , and the corresponding CO core mass, total lifetime and central C mass fraction after the core-He burning (from left to right). Masses are in given in M_⊙, ages in Myr.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.