3.7.1. Multi-field theories
While much of early investigation of inflation featured potentials such as the massive field discussed above, such models are widely regarded by inflation model builders as unsatisfactory. The reason is that current thinking in particle physics is dominated by supersymmetry, implying that in a cosmological context we should be operating within the framework of supergravity. Once supergravity is brought into play, the numerical value of the scalar field acquires a well-defined meaning, and it is believed that its value must be less than the (reduced) Planck mass mPl / (8 ) if the potential is not to be vulnerable to large nonrenormalizable corrections, which typically will destroy slow-roll and anyway will render theoretical calculations unreliable. As we have just seen, one cannot obtain sufficient inflation (or indeed any at all) with the polynomial potential under this restriction, and this conclusion is fairly generic for models where there is only a single scalar field.
An attractive way of circumventing this problem is the hybrid inflation model [10], where a second field provides an additional energy density which dominates over that from the inflaton itself. A typical potential takes the form
where g2 is the coupling constant governing the
interaction between
the two fields. This is shown in Fig. 1. For large
inflaton values the coupling stabilizes
at zero, where it
contributes a potential energy
M4 / 4 but
otherwise does not
participate in the dynamics, so that the inflaton sees a potential
The interesting case is where the constant term dominates, as it
provides extra friction to the
equation of motion which makes
it roll much more slowly, enabling sufficient inflation without
violating the condition
<< mPl /
(8
). Inflation
ends when the field drops below a
critical value, destabilizing
the field and allowing the system
to rapidly evolve into its
true minimum at = 0,
= ±M.
Figure 1. The potential for the hybrid
inflation model. The field rolls down the channel at
= 0 until
it reaches the critical value,
then falls off the side to the
true minimum at = 0 and
= ±M.
The original models
[10]
assumed that the inflaton potential
V() was just that of a
massive field, but unfortunately this
choice is vulnerable to large loop corrections which dominate over the
mass term. However many other possible models have been derived within
the hybrid framework; for an extensive discussion of this and other
model-building issues see the review of Lyth and Riotto
[11].