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En este artículo, se estudia la posibilidad de que el bosón de Higgs del Modelo Estándar de Partículas Elementales pueda generar inflación primordial del tipo rodadura lenta, lo que resolvería los problemas clásicos de la cosmología estándar. El requisito crucial para hacer viable esta posibilidad, es que el campo escalar de Higgs presente un tipo particular de acoplamiento no mínimo a la gravedad. Se realiza una transformación conforme desde el marco de Jordan al marco de Einstein encontrándose una modificación al tradicional potencial de Higgs para valores muy grandes del campo, lo que permite una zona de alta planitud y, por ende, inflación primordial del tipo rodadura lenta. Se comparan los resultados asociados al índice espectral y a la razón tensor a escalar con las cotas observacionales más recientes, encontrándose que la generación de estructuras a gran escala en este escenario es satisfactoria.
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