${\hbox{MgB}}_{2}$ for Application to RF Cavities for Accelerators

Abstract

Magnesium diboride (MgB <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sub> ) has a transition temperature of (T <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">c</sub> ) ~40 K, i.e., about 4 times as high as that of niobium (Nb). We have been evaluating MgB <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">2</sub> as a candidate material for radio-frequency (RF) cavities for future particle accelerators. Studies in the last 3 years have shown that it could have about one order of magnitude less RF surface resistance (R <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">s</sub> ) than Nb at 4 K. A power dependence test using a 6 GHz TE <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">011</sub> mode cavity has shown little power dependence up to ~12 mT (120 Oe), limited by available power, compared to other high- materials such as YBCO. A recent study showed, however, that the power dependence of R <sub xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">s</sub> is dependent on the coating method. A film made with on-axis pulsed laser deposition (PLD) has showed rapid increase in compared to the film deposited by reactive evaporation method. This paper shows these results as well as future plans.