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ARUP; ISBN: 978-0-9562121-5-3 - CMBBE 2012 - Cardiff University

ARUP; ISBN: 978-0-9562121-5-3 - CMBBE 2012 - Cardiff University

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estimated the morphological modifications of the breast under gravity loading for<br />

plastic surgery. For that, they proposed that the effect of the gravity in prone position<br />

was compensated by applying the gravity force in the opposite direction. This<br />

approximation has been chosen in this work to study the influence of considering the<br />

prone gravity-loaded breast taken from a MRI as the reference state for the simulation<br />

of a mammographic compression.<br />

In this paper, an approximated of zero-strain state was performed by applying the<br />

gravity force in the opposite direction to the prone position as performed in [9], aimed<br />

to find a reference state to simulate X-ray mammographies. In this work, the<br />

compression force is used to compare two simulations of the X-ray compression, when<br />

gravity is ignored and prone gravity loaded (obtained from MRI) is used as reference<br />

state, and when gravity force is applied and the calculated zero-strain configuration is<br />

used as reference state.<br />

3. MATERIALS AND METHODS<br />

The following four models from literature were used to simulate the breast tissue<br />

biomechanical behavior:<br />

• Linear elastic model: proposed by Kellner et al. in [4] with the following<br />

Young’s modulus for the different tissues Eskin= 88000 Pa, Efat=1000 Pa, and<br />

Egland=10000 Pa and 0.49 for the Poisson's ratios.<br />

• Nonlinear hyperelastic models:<br />

o Neo-Hookean: this model is characterized by its strain energy density<br />

function which is given by Eq. 1:<br />

With the constants provided by Pérez del Palomar et al. in [9]:<br />

C1fat=3000 Pa and C1gland=12000 Pa.<br />

o Mooney-Rivlin: A Money-Rivlin five parameter model is characterized<br />

by its strain energy density function as Eq. 2 shows:<br />

With the constants provided by Tanner et al. in [3]:<br />

- Fat: C10= 46420, C01= -31770, C20= 37070, C11=1960, C02= 1510 Pa.<br />

- Glandular: C10= 42830, C01= -36540, C20=51830, C11=7330, C02=<br />

520 Pa.<br />

o Polynomial: A Polynomial second order model (N=2) is characterized by<br />

its strain energy density function as shown in Eq. 3:<br />

With the constants provided by Samani et al. in [10]:<br />

- Fat: C10= 310, C01= 300, C20=3800, C11=2250, C02= 4700 Pa.<br />

- Glandular: C10= 330, C01= 280, C20=7700, C11=4490, C02= 9400 Pa.<br />

(1)<br />

(2)<br />

(3)

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