Prone scintimammography with Tc-99m SestaMIBI has been proposed as a method
of detecting breast cancers in women with dense breasts. Clinical reports
have shown that this technique lacks sensitivity for cancer smaller than 1
cm. To overcome some limitations offered by Anger camera on breast imaging
was realized a new scintigraphic detector dedicated to SPEM (Single Photon
Emission Mammography). This novel small FOV device, shows high spatial reso
lution performances (<2 mm), but poorer energy resolution values, than Ange
r camera (17% vs. 10%, respectively). In this paper we examine the spatial
distribution of Compton-to-photopeak ratio in planar scintimammographic ima
ges in order to elucidate the causes of lack of scintimammography in visual
izing deep or posteriorly located cancers introduced by the scatter from th
e patient's body. Phantom and clinical studies with several instruments inc
luding a general purpose gamma camera, a dedicated camera and a non imaging
Germanium detector were performed. The results obtained suggest that scatt
er from extramammary sources plays an important role in breast imaging with
radiotracers. By using gentle breast compression in cranio-caudal view the
energy resolution attained with the dedicated camera is adequate to differ
entiate between photopeak and Compton counts; the Compton-to photopeak mean
ratio resulted 4.5 and 6.9 for mild portion and posterior breast respectiv
ely.