5,571 research outputs found

    Exploring Vacuum Structure around Identity-Based Solutions

    Full text link
    We explore the vacuum structure in bosonic open string field theory expanded around an identity-based solution parameterized by a(>=1/2)a(>=-1/2). Analyzing the expanded theory using level truncation approximation up to level 20, we find that the theory has the tachyon vacuum solution for a>1/2a>-1/2. We also find that, at a=1/2a=-1/2, there exists an unstable vacuum solution in the expanded theory and the solution is expected to be the perturbative open string vacuum. These results reasonably support the expectation that the identity-based solution is a trivial pure gauge configuration for a>1/2a>-1/2, but it can be regarded as the tachyon vacuum solution at a=1/2a=-1/2.Comment: 12 pages, 5 figures; new numerical data up to level (20,60) included; Contribution to the proceedings of "Second International Conference on String Field Theory and Related Aspects" (Steklov Mathematical Institute, Moscow, Russia, April 12-19, 2009

    Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics

    Full text link
    We present calculations showing that upcoming Cosmic Microwave Background (CMB) experiments will have the power to improve on current constraints on neutrino masses and provide new limits on neutrino degeneracy parameters. The latter could surpass those derived from Big Bang Nucleosynthesis (BBN) and the observationally-inferred primordial helium abundance. These conclusions derive from our Monte Carlo Markov Chain (MCMC) simulations which incorporate a full BBN nuclear reaction network. This provides a self-consistent treatment of the helium abundance, the baryon number, the three individual neutrino degeneracy parameters and other cosmological parameters. Our analysis focuses on the effects of gravitational lensing on CMB constraints on neutrino rest mass and degeneracy parameter. We find for the PLANCK experiment that total (summed) neutrino mass Mν>0.29M_{\nu} > 0.29 eV could be ruled out at 2σ2\sigma or better. Likewise neutrino degeneracy parameters ξνe>0.11\xi_{\nu_{e}} > 0.11 and ξνμ/τ>0.49| \xi_{\nu_{\mu/\tau}} | > 0.49 could be detected or ruled out at 2σ2\sigma confidence, or better. For POLARBEAR we find that the corresponding detectable values are Mν>0.75eVM_\nu > 0.75 {\rm eV}, ξνe>0.62\xi_{\nu_{e}} > 0.62, and ξνμ/τ>1.1| \xi_{\nu_{\mu/\tau}}| > 1.1, while for EPIC we obtain Mν>0.20eVM_\nu > 0.20 {\rm eV}, ξνe>0.045\xi_{\nu_{e}} > 0.045, and ξνμ/τ>0.29|\xi_{\nu_{\mu/\tau}}| > 0.29. Our forcast for EPIC demonstrates that CMB observations have the potential to set constraints on neutrino degeneracy parameters which are better than BBN-derived limits and an order of magnitude better than current WMAP-derived limits.Comment: 27 pages, 11 figures, matches published version in JCA

    Analytical Tachyonic Lump Solutions in Open Superstring Field Theory

    Full text link
    We construct a classical solution in the GSO(-) sector in the framework of a Wess-Zumino-Witten-like open superstring field theory on a non-BPS D-brane. We use an su(2) supercurrent, which is obtained by compactifying a direction to a circle with the critical radius, in order to get analytical tachyonic lump solutions to the equation of motion. By investigating the action expanded around a solution we find that it represents a deformation from a non-BPS D-brane to a D-brane-anti-D-brane system at the critical value of a parameter which is contained in classical solutions. Although such a process was discussed in terms of boundary conformal field theory before, our study is based on open superstring field theory including interaction terms.Comment: 17 pages, references adde
    corecore