159 citations · 726 across the 47 of their papers we have counts for
39 papers · 1 filter
Proposal for Compositeness of String out of Objects -- Fake Scattering, Finite String Field Theory Formulation
Holger Bech Nielsen, Masao Ninomiya
We review a bit our earlier novel string field theory\cite{self2,self8} stressing the interesting property, that it becomes expressed in terms of particle like objects called by us…
Instructive Review of Novel SFT with Non-interacting consituents "objects", and attempt Generalization to p-adic theory
Holger Bech Nielsen, Masao Ninomiya
We have constructed a new formalism for describing a situation with {\color{red} several (dual) strings} present at a time, a {\color{red} string field theory}, by means of a const…
Novel String Field Theory with also Negative Energy Constituents/Objects gives Veneziano Amplitude
Holger Bech Nielsen, Masao Ninomiya
We have proposed a new type of string field theory. The main point of the present article is to cure some technical troubles: missing two out three terms in veneziano amplitude. Ou…
Bosons being their own antiparticles in Dirac formulation
Holger B. Nielsen, Masao Ninomiya
Using our earlier formalism of extending the idea of the Dirac sea (negative energy states) to also for Bosons, we construct a formalism for Bosons which are their own antiparticle…
A state description of pair production from Dirac sea in gravitational field --physical interpretation of Weyl anomaly--
Yoshinobu Habara, Holger B. Nielsen, Masao Ninomiya
We present the method that the pair production of particles is described as a Fock space state vector, where the pair production stems from receiving energy from, as an example, gr…
A new mechanism of realizing inflationary universe with recourse to backreaction of quantized free fields -- Inflation without inflaton --
Yoshinobu Habara, Hikaru Kawai, Masao Ninomiya
It is shown that the inflationary era in early universe is realized due to the effect of backreaction of quantized matter fields. In fact we start by quantizing a free scalar field…