Development of a New Electro-thermal Simulation Tool for RF circuits
Development of a New Electro-thermal Simulation Tool for RF circuits
Development of a New Electro-thermal Simulation Tool for RF circuits
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28 2.4. Compact Thermal Model<br />
the creation <strong>of</strong> a 3D <strong>thermal</strong> model, based on the detailed physical structure is a<br />
cumbersome task.<br />
Ideal CTM should be (1) accurate, (2) able to manage multiple heat sources and cooling<br />
surfaces, (3) taking nonlinear material properties into account, and (4) Boundary<br />
Condition Independent (BCI). Nevertheless, CTM structure has to remain simple, and<br />
easy to extract. Existing methodologies usually focus on a few <strong>of</strong> abovementioned<br />
qualities; otherwise, the resulting CTM would become too complex. Several methods<br />
have been already developed to provide accurate CTMs. One <strong>of</strong> them is the Delphi<br />
method [43, 44], which is able to give accurate static BCI CTMs <strong>for</strong> single-chip<br />
electronic devices and systems. An important drawback <strong>of</strong> Delphi, is the amount <strong>of</strong><br />
3D simulations [41]. In addition, dynamic models are difficult to extract. Delphi CTMs<br />
with more than two heat sources result in a very dense and excessively complex resistor<br />
network, where the number <strong>of</strong> 3D simulations or measurements becomes exorbitant.<br />
On the other hand, [45, 46] describe "traditional" CTM generation methods, with the<br />
way to make the <strong>thermal</strong> coupling between heat sources in static and dynamic modes.<br />
However in these methodologies, the CTMs are BCI only <strong>for</strong> systems with one cooling<br />
surface.<br />
Beside that, the device manufacturers may not wish to publish the confidential data<br />
about the dimensions, materials and technology. However from the customer point<br />
<strong>of</strong> view, the knowledge <strong>of</strong> a <strong>thermal</strong> behaviour might be necessary. This problem<br />
has been noticed by the semiconductor industry [39, 40, 41, 42]. As the result, the<br />
standard equivalent <strong>thermal</strong> networks libraries have been developed, which are in use<br />
with standard CAD s<strong>of</strong>tware. However, the drawback <strong>of</strong> this approach is the amount <strong>of</strong><br />
3D numerical simulations to be per<strong>for</strong>med, in order to produce the CTM parameters.<br />
A new CTM methodology will be demonstrated, which <strong>of</strong>fers reduced amount <strong>of</strong><br />
3D simulations. The model has been under investigation during the PhD stage in<br />
LAAS-CNRS laboratory, Toulouse, France. Based on existing methods, the approach<br />
gives innovative solutions, in order to improve known CTM generation procedures.<br />
Firstly, a BCI CTM extraction method <strong>for</strong> systems with multiple cooling surfaces will<br />
be demonstrated. The CTM is an evolution <strong>of</strong> the star <strong>thermal</strong> network. Secondly,<br />
a new method conceived especially <strong>for</strong> multi-chip devices, i.e., multiple coupled heat<br />
sources [47, 48] will be presented. The <strong>thermal</strong> coupling is based on a definition <strong>of</strong> an<br />
Optimal Thermal Coupling Point (OTCP) between heat sources [49].<br />
2.4.2. Methodology <strong>for</strong> Multi-Cooling Surface Structures<br />
The star <strong>thermal</strong> network is a simple representation, which allows dealing easily as<br />
well with static as dynamic multiple cooling surface problems. In typical configuration<br />
the model (Fig. 2.17) has three cooling surfaces. Each one is represented with <strong>thermal</strong><br />
resistance: Rth_top, Rth_bottom and Rth_side. The main drawback <strong>of</strong> the star model is with<br />
boundary conditions (Rh_top, Rh_bottom and Rh_side) change, the model becomes not<br />
valid. . The presented methodology is an extension <strong>of</strong> the star model representation,<br />
modified in order to deal with changing boundary conditions (BCI). The detailed