Sixth Texas Symposium on relativistic astrophysics.
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The Texas symposium on relativistic astrophysics.
This is the written version of the summary talk given at the 20th Texas Symposium on Relativistic Astrophysics in Austin, Texas, on December 15, 2000. After a brief summary of some of the highlights at the conference, comments are offered on three special topics: theories with large additional spatial dimensions, the cosmological constant problems, and the analysis of fluctuations in the cosmic...
متن کامل20 th Texas Symposium on Relativistic Astrophysics
This is the written version of the summary talk given at the 20th Texas Symposium on Relativistic Astrophysics in Austin, Texas, on December 15, 2000. After a brief summary of some of the highlights at the conference, comments are offered on three special topics: theories with large additional spatial dimensions, the cosmological constant problems, and the analysis of fluctuations in the cosmic...
متن کاملar X iv : a st ro - p h / 01 04 48 2 v 3 4 M ay 2 00 1 UTTG - 05 - 01 Conference Summary 20 th Texas Symposium on Relativistic Astrophysics
This is the written version of the summary talk given at the 20th Texas Symposium on Relativistic Astrophysics in Austin, Texas, on December 15, 2000. After a brief summary of some of the highlights at the conference, comments are offered on three special topics: theories with large additional spatial dimensions, the cosmological constant problems, and the analysis of fluctuations in the cosmic...
متن کاملMagnetic Fields from Bubble Collisions — A Progress Report
Primordial magnetic fields may be created in collisions of expanding bubbles in a first-order cosmological phase transition and later serve as seed fields for galactic magnetic fields. Here I present results from numerical and analytical studies of U(1) bubble collisions done in collaboration with Ed Copeland and Paul Saffin. I also reveal preliminary results from analytical studies of SU(2)×U(...
متن کاملHalo Dark Clusters of Brown Dwarfs and Molecular Clouds
The observations of microlensing events in the Large Magellanic Cloud suggest that a sizable fraction (∼ 50%) of the galactic halo is in the form of MACHOs (Massive Astrophysical Compact Halo Objects) with an average mass ∼ 0.27M⊙, assuming a standard spherical halo model. We describe a scenario in which dark clusters of MACHOs and cold molecular clouds (mainly of H2) naturally form in the halo...
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عنوان ژورنال:
- Annals of the New York Academy of Sciences
دوره 224 شماره
صفحات -
تاریخ انتشار 1973