<blockquote><font class="small">In reply to:</font><hr /><p><b>Cold Fusion (Low Temperature Physics): A Correlation to Some Star Births</b><br /> <br />Like I said a 1000-times already: I am working on the affects of velocity: Increased Mass -(m <sub>i</sub>); Time Dilation; -(t <sub>d</sub>); Length Contraction -(L <sub>c</sub>); however, this analysis is going to be utilized in real world working simulations too. Therefore, fission and/or fusion is critical to my theories success. I am not so much concerned with the whole shebang, so to speak, as much as I am concerned with the lighter elements, i.e. Helium (He), Hydrogen (H), ..., Oxygen (O <sub>2</sub>), ..., etc. I would prefer to work with (He), but containment might not be possible, so I may be required to move down to (H). The fact of the matter is: I am not sure yet, and that is why I opened this Fusion versus Fission thread. <br /> <br />With respect to (He), (He) breaks down to various sub-elements, and at the moment I am only interested in Helium-3 and 4, as in (<sub>3</sub>He and <sub>4</sub>He), and as a result, I am more inclined to lean towards fusion for my experiments, if I ever get the opportunity to try my experiments that is. You see, charged particles travel faster that the speed-of-light -(c) within a medium, (fusion and fission), and we are currently utilizing various mediums comprised of liquid(s) that projecting varying degrees of temperatures. The fusion reactors with lithium mediums are nice, but they are far less efficient than Helium (He) reactors; plus they are hotter than hell. If I am going to go through the pain staking work of inventing cold reactors, then I will prefer to work with (He), if you all get my drift.<br /><br /><b>So, without further ado; I present to my audience Cold Fusion (Low Temperature Physics):</b><br /><br />Temperature physics is a science concerned with the production and maintenance of extreme temperatures that are far below and above normal, and we are primarily c</p></blockquote>