The　Schwarzschild　singularity＇s　resolution　has　key　values　in　cracking　the　key　mysteries　related　with　black　holes,　the　origin　of　their　horizon　entropy　and　the　information　missing　puzzle　involved　in　their　evaporations.　We　provide　in　this　work　the　general　dynamic　inner　metric　of　collapsing　stars　with　horizons　and　with　non-trivial　radial　mass　distributions.　We　find　that　static　central　singularities　are　not　the　final　state　of　the　system.　Instead,　the　final　state　of　the　system　is　a　periodically　zero-cross　breathing　ball.　Through　3+1　decomposed　general　relativity　and　its　quantum　formulation,　we　establish　a　functional　Schrdinger　equation　controlling　the　micro-state　of　this　breathing　ball　and　show　that,　the　system　configuration　with　all　the　matter　concentrating　on　the　central　point　is　not　the　unique　eigen-energy-density　solution.　Using　a　BohrSommerfield　like　＂orbital＂　quantisation　assumption,　we　show　that　for　each　black　hole　of　horizon　radius　r(h),　there　are　about　e(r2h/l2pl)　allowable　eigen-energy-density　profiles.　This　naturally　leads　to　physic　interpretations　for　the　micro-origin　of　horizon　entropy,　as　well　as　solutions　to　the　information　missing　puzzle　involved　in　Hawking　radiations.　(C)　2017　The　Author(s).　Published　by　Elsevier　B.V.　This　is　an　open　access　article　under　the　CC　BY　license