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Epigastric Hernia

An epigastric hernia is a primary midline defect through the linea alba between the xiphoid process and umbilicus.

Most are small and contain preperitoneal fat rather than bowel. Multiple small defects may coexist.

Pain can arise from incarceration of preperitoneal fat even when the external swelling is tiny.

Rectus diastasis frequently coexists but is not itself a true hernia because the linea alba remains intact.

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Richter Hernia

A Richter hernia occurs when only part of the circumference of the bowel wall, usually the antimesenteric border, becomes trapped within a small fascial defect.

Because the intestinal lumen is not completely occluded, the patient may continue passing stool and flatus despite progressive strangulation of the trapped bowel wall.

This makes Richter hernia particularly dangerous. Bowel necrosis or perforation can occur without classical complete bowel obstruction.

Common sites include femoral and inguinal defects and small laparoscopic port sites.