BARYOGENESIS WITHOUT BARYON NUMBER VIOLATION

1990 ◽  
Vol 05 (21) ◽  
pp. 1623-1628 ◽  
Author(s):  
SCOTT DODELSON ◽  
LAWRENCE M. WIDROW

We review a new paradigm for baryogenesis in which the fundamental Lagrangian is baryon conserving [invariant under U (1) B ]. At high temperatures, U (1)B is spontaneously broken and an excess of quarks over antiquarks of 10−10s (s≡entropy density) is produced. Today, U(1)B is restored. A fundamental consequence of our assumptions is that the baryon number of the Universe is constant. If initially zero, it will be zero today. The excess baryon number produced in the quark fields is exactly compensated by antibaryon number in a weakly interacting scalar particle. We suggest that this scalar provides the mass density necessary to close the Universe.

1991 ◽  
Vol 06 (09) ◽  
pp. 769-773
Author(s):  
A.M. MATHESON

In some cosmic string models the strings may give rise to baryon number violation. Constraints are derived on theories of this kind, from the measured limits on proton decay and the timing residual of the millisecond pulsar, by requiring that strings should not wash out the observed baryon-to-entropy ratio of the universe.


1987 ◽  
Vol 194 (2) ◽  
pp. 241-246 ◽  
Author(s):  
John Ellis ◽  
R.A. Flores ◽  
S. Rudaz ◽  
D. Seckel

1983 ◽  
Vol 28 (9) ◽  
pp. 2248-2257 ◽  
Author(s):  
Paul Langacker ◽  
Deshdeep Sahdev

Sign in / Sign up

Export Citation Format

Share Document