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Development of a New Electro-thermal Simulation Tool for RF circuits

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12 2.1. Assumptions <strong>for</strong> analytical <strong>thermal</strong> model<br />

2. The image function method (e.g. [35]). In this approach the temperature<br />

solution is first determined by neglecting the boundary conditions at the<br />

lateral and bottom boundaries . This implies that in this approximation<br />

one treats the heat source as if it were in a semi-infinite domain. It has<br />

been shown that it is possible to finish a simple closed-<strong>for</strong>m solution <strong>for</strong><br />

rectangular heat sources (see section 2.3.1 and 2.3.2). The second step is to<br />

incorporate the effect <strong>of</strong> boundary conditions. This is done by introducing<br />

an infinite number <strong>of</strong> fictitious heat sources. As a result, the temperature<br />

solution is expressed as an infinite sum <strong>of</strong> terms, each accounting <strong>for</strong> a<br />

fictitious image source. Note that if the heat source-to-chip area ratio is<br />

small, so the effect <strong>of</strong> boundary conditions will be negligible in practice and<br />

a small number <strong>of</strong> terms (or even just one one term) need to be included.<br />

There<strong>for</strong>e this method is very efficient <strong>for</strong> small devices.<br />

In section 2.2, the problem <strong>of</strong> solution <strong>of</strong> the heat-flow equation will be described<br />

from the mathematical point <strong>of</strong> view, introducing possible approximations. The<br />

idea <strong>of</strong> <strong>thermal</strong> resistance and <strong>thermal</strong> impedance will be demonstrated.<br />

2.1.<br />

Assumptions <strong>for</strong> analytical <strong>thermal</strong> model<br />

The steady-state heat-flow equation is described as follows:<br />

▽ [k(T ) ▽ T ] + g(x, y, z) = 0 (2.1)<br />

where k(T ) is the <strong>thermal</strong> conductivity, T is the temperature and g(x, y, z) is the power<br />

density (which depends on a position) per unit volume [W/cm 3 ].<br />

To solve the heat-flow equation (Eq. 2.2) one needs to specify:<br />

➤ How the heat is exchanged with the environment (boundary conditions).<br />

➤ The generation <strong>of</strong> the heat (power density g function).<br />

Usually this problem is resolved by simplifying both:<br />

Power Density. The active area where the heat is generated, is assumed <strong>of</strong> a simple<br />

geometry (parallelepiped or rectangle), with a power density g function, that is<br />

(1) constant and uni<strong>for</strong>m in the heat source area (2) zero outside the heat source<br />

area.<br />

Boundary Conditions (B.C.). The boundary conditions are simplified as follows:

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