Two broad scenarios for extended linear Lorentz transformations (ELTs) are modeled in Section 2 for mixing subluminal and superluminal sectors resulting in standard or deformed energy-momentum dispersions. The first scenario is elucidated in the context of four diverse realizations of a continuous function <svg style="vertical-align:-3.56265pt;width:30.1625px;" id="M1" height="16.6625" version="1.1" viewBox="0 0 30.1625 16.6625" width="30.1625" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"> <g transform="matrix(.017,-0,0,-.017,.062,12.162)"><path id="x1D453" d="M619 670q0 -13 -9 -26t-18 -19q-13 -10 -25 2q-36 38 -66 38q-31 0 -54.5 -50t-45.5 -185h120l-20 -31l-107 -12q-23 -138 -57 -293q-27 -122 -55 -184.5t-75 -109.5q-60 -61 -114 -61q-25 0 -47.5 15t-22.5 31q0 17 31 44q11 8 20 -1q10 -11 31 -19t35 -8q26 0 47 19
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What goes in the making of the ELT in this scenario is not the boost speed <svg style="vertical-align:-0.1638pt;width:7.4875002px;" id="M4" height="7.9124999" version="1.1" viewBox="0 0 7.4875002 7.9124999" width="7.4875002" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"> <g transform="matrix(.017,-0,0,-.017,.062,7.638)"><use xlink:href="#x1D463"/></g> </svg>, as ascertained by two inertial observers in uniform relative motion (URM), but <svg style="vertical-align:-3.56265pt;width:55.049999px;" id="M5" height="16.6625" version="1.1" viewBox="0 0 55.049999 16.6625" width="55.049999" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"> <g transform="matrix(.017,-0,0,-.017,.062,12.162)"><use xlink:href="#x1D463"/></g><g transform="matrix(.017,-0,0,-.017,11.197,12.162)"><path id="xD7" d="M528 54l-36 -38l-198 201l-198 -201l-36 38l197 200l-197 201l36 38l198 -202l198 202l36 -38l-197 -201z" /></g><g transform="matrix(.017,-0,0,-.017,24.949,12.162)"><use xlink:href="#x1D453"/></g><g transform="matrix(.017,-0,0,-.017,35.862,12.162)"><use xlink:href="#x28"/></g><g transform="matrix(.017,-0,0,-.017,41.743,12.162)"><use xlink:href="#x1D463"/></g><g transform="matrix(.017,-0,0,-.017,49.104,12.162)"><use xlink:href="#x29"/></g> </svg>. The second scenario infers the preexistence of two rest-mass-dependent superluminal speeds whereby the ELTs are finite at the light speed <svg style="vertical-align:-0.1638pt;width:7.0250001px;" id="M6" height="7.9499998" version="1.1" viewBox="0 0 7.0250001 7.9499998" width="7.0250001" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"> <g transform="matrix(.017,-0,0,-.017,.062,7.675)"><use xlink:href="#x1D450"/></g> </svg>. Particle energies are evaluated in this scenario at <svg style="vertical-align:-0.1638pt;width:7.0250001px;" id="M7" height="7.9499998" version="1.1" viewBox="0 0 7.0250001 7.9499998" width="7.0250001" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns="http://www.w3.org/2000/svg"> <g transform="matrix(.017,-0,0,-.017,.062,7.675)"><use xlink:href="#x1D450"/></g> </svg> for several particles, including the neutrinos, and are auspiciously found to be below the GKZ energy cutoff and in compliance with a host of worldwide ultrahigh energy cosmic ray data. Section 3 presents two broad scenarios involving a number of novel nonlinear LTs (NLTs) featuring small Lorentz invariance violations (LIVs), as well as resurrecting the notion of simultaneity for limited spacetime events as perceived by two observers in URM. These inquiries corroborate that NLTs could be potent tools for investigating LIVs past the customary LTs.
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