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According to stellar classification [See Link] the proportion of Stars in category O,B those massive enough to be categorised as possible candidates for a black hole, number less than 0.13% while candidates for white dwarfs, category G,K, comprise about 20% of all known stars.

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This is because white dwarf stars are caused by the sides of a star pulling inward. However, a black hole is caused when a massive star completely collapses inward upon itself, creating a void of sorts, where instead of giving off light and power, it is blank and gives off nothing(black holes do NOT suck as many people believe). As massive stars are less likely to occur than medium and small- sized stars because of the amount of matter needed to make them, therefore we have many more white dwarf stars than we have black holes.

I have already answered this question but apperantly someone has deleted it so o.k. it is because most stars are medium sized, extremely condensed, or just plain small, while black holes need stars that are super-sized, or have a few medium stars in close proximaty(is someone could just correct those mistakes i would but i need to watch what i put down ty)
More stars have a longer main sequence (low mass stars), which don't swell up to supergiants, they only swell to giants. Low mass stars are more common, and they end up as white dwarfs.

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