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Ecole doctorale de Physique de la région Parisienne (ED107)

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E(t) / E 0<br />

1.15<br />

1.1<br />

1.05<br />

1<br />

4.4 Test and calibration of the co<strong>de</strong> 123<br />

Time evolution of energy with reaction force<br />

0 20 40 60<br />

t Ω<br />

Without correction<br />

With correction<br />

Figure 4.6 – Time evolution of the ratio between energy and initial energy in an inviscid<br />

and incompressible rigidly rotating fluid with an RR force corresponding to what should<br />

exist in a NS with M = 1.4M⊙, R = 10 km and Ω (2π) 500 Hz. The first curve<br />

corresponds to the basic co<strong>de</strong> and the second one to the co<strong>de</strong> with improved conservation<br />

of energy. The expected final value is about 1.057. The difference between this analytical<br />

calcu<strong>la</strong>tion and the corrected numerical result is less than 10 −3 .<br />

happen with physical values. As expected, there is an axial mo<strong>de</strong> (no radial velocity)<br />

driven to instability with exactly the frequency (w = 4Ω)<br />

and coefficients (l = 2) of the<br />

3<br />

r-mo<strong>de</strong>. Moreover, a single look at the Figure 4.9 shows that even when the velocity is<br />

mainly noisy, the tensor that p<strong>la</strong>ys the key-role in the instability is quite smooth. In this<br />

figure, we also drew a zoom corresponding to tΩ < 50 and the associated power spectrum.<br />

It shows two frequencies in this component of the tensor. One of them is the unstable<br />

r-mo<strong>de</strong> with 3w/Ω = 4 and the other (with 3w/Ω ∼ 2.70) disappears with a longer run, as<br />

the scale is adapted to the growing mo<strong>de</strong>. Yet, even in the spectrum of the full evolution,<br />

a trace of it can still be seen. We achieved exactly the same features with others noisy<br />

initial conditions, for instance a Dirac kick into the NS1 . We also did the same calcu<strong>la</strong>tions<br />

with other spatial <strong>la</strong>ttices (up to 64 × 48 × 4), and this result did not change at all.<br />

4.4.3 Test of the ane<strong>la</strong>stic approximation<br />

The <strong>la</strong>st calcu<strong>la</strong>tions we did in a rigid and Newtonian background were to test the<br />

effect of the ane<strong>la</strong>stic approximation. The i<strong>de</strong>a was to compare the previous results obtained<br />

with the divergence-free approximation and a rigid crust BC with results coming<br />

from the same initial conditions but with the ane<strong>la</strong>stic approximation and the free surface<br />

1 We mean an initial velocity equal to 0 anywhere except in an arbitrary point.

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