Published April 27, 1992
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Constraints on the nuclear matter equation of state from pulsar glitches
Description
We study the post-glitch response of four pulsars to obtain lower limits on the total moment of inertia of the inner crust superfluid. In contrast to previous work, our constraints are independent of the form of the crust-superfluid coupling. We conclude that the superfluid must comprise approx-gt 0.8% of the total moment of inertia of the star. This constraint rules out the softest equations of state
Availability note (English)
MF available from INIS under the Report Number; OSTI as DE92015142; NTIS; INIS; US Govt. Printing Office Dep.
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Additional details
Publishing Information
- Imprint Pagination
- 9 p.
- Report number
- LA-UR--92-1610
Conference
- Title
- Physics of isolated pulsars workshop.
- Dates
- 23-28 Feb 1992.
- Place
- Taos, NM (United States).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 23072604
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- EQUATIONS OF STATE; MOMENT OF INERTIA; NEUTRON STARS; NUCLEAR MATTER; PULSARS; SUPERFLUIDITY
- Descriptors DEC
- COSMIC RADIO SOURCES; EQUATIONS; MATTER; STARS
Optional Information
- Contract/Grant/Project number
- Contract W-7405-ENG-36
- Funding organization
- USDOE, Washington, DC (United States).
- Secondary number(s)
- CONF-9202117--2.