1.  Field
Embodiments of the present mention generally relate to data storage systems, and more particularly, to write heads for thermally assisted recording. 
2.  Description of the Related Art
Higher storage bit densities in magnetic media used in disk drives have reduced the size (volume) of magnetic bits to the point where the magnetic bit dimensions are limited by the grain size of the magnetic material.  Although grain size can be reduced further, the data stored within the magnetic bits may not be thermally stable.  That is, random thermal fluctuations at ambient temperatures may be sufficient to erase data.  This state is described as the superparamagnetic limit, which determines the maximum theoretical storage density for a given magnetic media.  This limit may be raised by increasing the coercivity of the magnetic media or by lowering the temperature.  Lowering the temperature may not always be practical when designing hard disk drives for commercial and consumer use.  Raising the coercivity, on the other hand, requires write heads that incorporate higher magnetic moment materials, or techniques such as perpendicular recording (or both). 
One additional solution has been proposed, which uses heat to lower the effective coercivity of a localized region on the magnetic media surface and writes data within this heated region.  The data state becomes “fixed” once the media cools to ambient temperatures.  This technique is broadly referred to as “thermally assisted (magnetic) recording” (TAR or TAMR), “energy assisted magnetic recording” (EAMR), or “heat-assisted magnetic recording” (HAMR) which are used interchangeably herein.  It can be applied to longitudinal and perpendicular recording systems as well as “bit patterned media”.  Heating of the media surface has been accomplished by a number of techniques such as focused laser beams or near-field optical sources. 
While the laser beam or the near-field optical source is positioned to induce heating in the magnetic media, a certain percentage of heat will also be generated in the magnetic head.  This heating can affect the shape of the head at the air bearing surface (ABS), and therefore impact the fly height.  Heating of the head can also impact the reliability and performance of the head because high temperatures can accelerate thermal migration of various films and structures, causing inter-diffusion and dimensional smearing. 
The primary areas of the HAMR head that get hot are the antenna and the magnetic lip.  The antenna material is comprised of noble metals with low melting point and hence can show morphological changes with heating.  The magnetic lip material is comprised of alloy of (Co, Fe, Co, Ni, Cr) and with increase in temperature under operational conditions can degrade due to severe oxidation.  Thus, an efficient heat transfer path is needed from both the near field transducer (NFT) and the magnetic lip to the heat sink(s).  A critical component to ensure efficient heat transfer is elimination of thermal impedance at the interfaces formed during integration of different materials to fabricate the NFT, magnetic lip and the heat sink(s).  The interfaces generated during the fabrication process get exposed to atmosphere and are oxidized thus leading to high interface thermal impedance.  Therefore, there is a need in the art for an improved recording head for HARM.