Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/5/84; site prometheus.UUCP Path: utzoo!linus!philabs!cmcl2!seismo!umcp-cs!prometheus!pmk From: pmk@prometheus.UUCP (Paul M Koloc) Newsgroups: net.physics Subject: Re: Color of Neutron Stars. Message-ID: <139@prometheus.UUCP> Date: Sun, 7-Apr-85 23:27:05 EST Article-I.D.: promethe.139 Posted: Sun Apr 7 23:27:05 1985 Date-Received: Tue, 9-Apr-85 03:37:04 EST References: <1523@decwrl.UUCP> Organization: Prometheus II Ltd., College Park, MD Lines: 23 > It would > be expected that the "typical" neutron star would have a > very intense magnetic field, a result of compression of the > "ancestral" stars ordinary magnetic field. > It's probably true that most neutron stars have very intense magnetic field densities, but probably NOT the result of compression of the "ancestral" star state. In fact, that ancestral field is swept away by the outward snow plow action of the outer plasma mantle of the star as the mantle is driven by the release of energy arising from the "gravitational collapse of the inner core of the star. It is sort of an inverse inverse pinch. The field of the collapsed star probably has its origin from unified field related processes which are not yet known, or well understood, but may well be mass density, star body spin and precession related. I like crimson. -- +-------------------------------------------------------+--------+ | pmk@prometheus: (301) 445-1075 | FUSION | | Prometheus II Ltd., College Park, MD 20740-0222 | this | | ..!{umcp-cs,seismo}!prometh!pmk | decade | +-------------------------------------------------------+--------+