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1.
Proc Natl Acad Sci U S A ; 95(1): 82-4, 1998 Jan 06.
Article in English | MEDLINE | ID: mdl-9419329

ABSTRACT

Observations of microwave background fluctuations can yield information not only about the geometry of the universe but potentially about the topology of the universe. If the universe is negatively curved, then the characteristic scale for the topology of the universe is the curvature radius. Thus, if we are seeing the effects of the geometry of the universe, we can hope to soon see signatures of the topology of the universe. The cleanest signature of the topology of the universe is written on the microwave sky: There should be thousands of pairs of matched circles. These circles can be used to determine the precise topology and volume of the universe. Because we see hundreds of slices through the fundamental domain of the universe, we can use the microwave observations to reconstruct the initial conditions of the entire universe on the scale of a few megaparsecs.

2.
Proc Natl Acad Sci U S A ; 94(13): 6579-84, 1997 Jun 24.
Article in English | MEDLINE | ID: mdl-11607729
3.
Proc Natl Acad Sci U S A ; 94(7): 2783-4, 1997 Apr 01.
Article in English | MEDLINE | ID: mdl-11607725
4.
Science ; 237(4821): 1471-3, 1987 Sep 18.
Article in English | MEDLINE | ID: mdl-17816790

ABSTRACT

A simplified analytic model of a cooling hot neutron star, motivated by detailed computer calculations, describes well the neutrinos detected from the recent supernova in the Large Magellanic Cloud. The observations do not require explanations that invoke exotic physics or complicated astrophysics. The parameters in this simple model are not severely constrained: 6.1(-3.6)(+3.5) x 10(52) ergs emitted in electron antineutrinos, a peak temperature of 4.2(-0.8)(+1.2) megaelectron volts, a radius of 27(-15)(+17) kilometers, and a cooling time of 4.5(-2.0)(+1.7) seconds.

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