<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Gover, A.</author>
             <author>Emma, C.</author>
             <author>Friedman, A.</author>
             <author>Ianconescu, R.</author>
             <author>Musumeci, P.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Conceptual Theory of Spontaneous and Taper-Enhanced Superradiance and Stimulated Superradiance
          </title>
       </titles>
       <pages>WEP085</pages>
       <keywords>
          <keyword>radiation</keyword>
          <keyword>electron</keyword>
          <keyword>wiggler</keyword>
          <keyword>FEL</keyword>
          <keyword>free-electron-laser</keyword>
       </keywords>
       <dates>
          <year>2015</year>
          <pub-dates>
             <date>2015-12</date>
          </pub-dates>
       </dates>
       <abstract>
          In the context of radiation emission from an electron beam Dicke's superradiance (SR) is the enhanced radiation emission from a pre-bunched beam. Stimulated Superradiance (ST-SR) is the further enhanced emission of the bunched beam in the presence of a phase-matched radiation wave. These processes were analyzed for Undulator radiation in the framework of radiation field mode-excitation theory[1]. In the nonlinear saturation regime the synchronism of the bunched beam and an injected radiation wave may be sustained by wiggler tapering [2]. Same processes are instrumental also in enhancing the radiative emission in the tapered wiggler section of seeded FEL[3]. In a long tapered wiggler the diffraction of the emitted radiation wave is not negligible even at Angstroms wavelengths (as in LCLS). A Fresnel diffraction model was provided in [4] for the SR process only. Here we outline the fundamental physical concepts of Spontaneous Superradiadce (SR), Stimulated Superradiance (ST-SR), Taper-Enhanced Superradiance (TES) and Taper-Enhanced Stimulated Superradiance Amplification (TESSA), and compare their Fourier and Phasor formulations in the radiation mode expansion and free-diffraction models. Detailed further analysis can provide better design concepts of high power FELs and improved tapering strategy for enhancing the power of seeded short wavelength FELs
       </abstract>
    </record>
  </records>
</xml>
