The idea of the quantum state of the Universe described by some density matrix, i.e mixture of at least two vacua, the trivial symmetric and the nontrivial one with spontaneously broken symmetry is discussed. Nonzero cosmological constant necessarily arises for such a state and has the observable value if one takes the axion mass for the vacuum expectation value. The Higgs model, Nambu's model and discrete symmetry breaking are considered. Human observers can observe only the world on the nonsymmetric vacuum, the world on the other vacuum is some dark matter. Gravity is due to action of two worlds. Tachyons nonobservable for visible matter can be present in the dark matter, leading to some effects of nonlocality in the space of the Universe
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
We show that non-Abelian gauge fields in a higher-dimensional theory compactified on small extra dim...
AbstractIn N=1 supergravity the scalar potential of the hidden sector may have degenerate supersymme...
We address the question how to adapt cosmological constant Λ for description of a vacuum dark energy...
Recently, a new framework for describing the multiverse has been proposed which is based on the pri...
In quantum field theory, many phenomena are characterized by a condensed structure of their vacua. S...
In quantum field theory, many phenomena are characterized by a condensed structure of their vacua. S...
We study the behavior of the vacuum condensates characterizing many physical phenomena. We show that...
Contemporary physics faces three great riddles that lie at the intersection of quantum theory, parti...
A key challenge for many quantum gravity approaches is to construct states that describe smooth geom...
The nonminimal coupling of a massive self-interacting scalar field with a gravitational field is stu...
AbstractWe argue that in the context of string theory a large number N of connected degenerate super...
We argue that quantum theory should proceed not from a spacetime background but from a Lie algebra, ...
Non commutative geometry is creating new possibilities for physics. Quantum spacetime geometry and p...
Cosmological constant corresponds to the maximally symmetric cosmological term with the equation of ...
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
We show that non-Abelian gauge fields in a higher-dimensional theory compactified on small extra dim...
AbstractIn N=1 supergravity the scalar potential of the hidden sector may have degenerate supersymme...
We address the question how to adapt cosmological constant Λ for description of a vacuum dark energy...
Recently, a new framework for describing the multiverse has been proposed which is based on the pri...
In quantum field theory, many phenomena are characterized by a condensed structure of their vacua. S...
In quantum field theory, many phenomena are characterized by a condensed structure of their vacua. S...
We study the behavior of the vacuum condensates characterizing many physical phenomena. We show that...
Contemporary physics faces three great riddles that lie at the intersection of quantum theory, parti...
A key challenge for many quantum gravity approaches is to construct states that describe smooth geom...
The nonminimal coupling of a massive self-interacting scalar field with a gravitational field is stu...
AbstractWe argue that in the context of string theory a large number N of connected degenerate super...
We argue that quantum theory should proceed not from a spacetime background but from a Lie algebra, ...
Non commutative geometry is creating new possibilities for physics. Quantum spacetime geometry and p...
Cosmological constant corresponds to the maximally symmetric cosmological term with the equation of ...
In the present work, it is shown that the problem of the cosmological constant (CC) is practically t...
We show that non-Abelian gauge fields in a higher-dimensional theory compactified on small extra dim...
AbstractIn N=1 supergravity the scalar potential of the hidden sector may have degenerate supersymme...