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hamers / mse

Multiple Stellar Evolution -- A Population Synthesis Code for Multiple-Star Systems
GNU General Public License v3.0
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Segmentation fault #5 #34

Closed pavanvyn closed 3 years ago

pavanvyn commented 3 years ago

Version 7ec7a30659cbf87c09cd8ccc3fffedf1e529d1f4

N_bodies = 4
masses = [35.48451711269334, 3.754291259792952, 1.5698448495850958, 2.458995707154814]
metallicities = [0.02856425149565036, 0.02856425149565036, 0.02856425149565036, 0.02856425149565036]
semimajor_axes = [13.3262155657255, 3.4979312630635655, 6609.517083248268]
eccentricities = [0.23737870375549824, 0.23197438121205205, 0.49232074675514736]
inclinations = [1.6635484797295157, 0.6920134796825302, 1.4541731092472017]
arguments_of_pericentre = [1.6311984421749086, 5.668718789942289, 3.0727957388875455]
longitudes_of_ascending_node = [0.8760625104853672, 3.237978932106665, 0.8929969114254929]
tend = 1.400000E+10
N_steps = 1000
stellar_types = [1, 1, 1, 1]
object_types = [1, 1, 1, 1]

Error: U not finite Segmentation fault

hamers commented 3 years ago

I suspect this is because of a problem with MSTAR; I have asked Antti to look into it.

hamers commented 3 years ago

The issue was related to a time stepping problem in MSTAR that has now been resolved (ad9e7cf).