Articles
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05/14/2012--
05/14/2012
Three-port beam splitter for slow neutrons using holographic nanoparticle-polymer composite diffraction gratings
Diffraction of slow neutrons by nanoparticle-polymer composite gratings has
been observed. By carefully choosing grating parameters such as grating
thickness and spacing, a three-port beam splitter operation for cold neutrons -
splitting the incident neutron intensity equally into the plus-minus first and
zeroth diffraction orders - was realized. As a possible application, a Zernike
three-path interferometer is briefly discussed.
J. Klepp
Y. Tomita
C. Pruner
J. Kohlbrecher
M. Fally
11/13/2020--
11/13/2020
Tackling the phase problem of diffraction for retrieval of photonic structures formed in nanocomposite materials
We experimentally demonstrate how to solve the phase problem of diffraction
using multi-wave interference with standard diffraction experimental setups
without the need for taking any auxiliary data. In particular, we show that the
phases of the Fourier components of a periodic structure can be fully recovered
by deliberately choosing a probe wavelength of the diffracting radiation much
smaller than the lattice constant. In the course of the demonstration, we
accurately determine the refractive index profile of nanocomposite phase
gratings by light and neutron diffraction measurements.
M. Fally
Y. Tomita
A. Fimia
R. F. Madrigal
J. Guo
J. Kohlbrecher
J. Klepp
04/28/1999--
07/08/1998
Optical and CO Radio Observations of Poor Cluster Zwicky 1615.8+3505
The cluster Zwicky 1615.8+3505 is considered to be a dynamically young poor
cluster. To investigate the morphology and star-formation activity of galaxies
under the environment of a dynamically young poor cluster, we have performed V,
R, and I surface photometry, optical low-resolution spectroscopy, and 12CO
(J=1-0) line observations for member galaxies. Our data show that more than 90%
of the observed galaxies show regular morphologies and no star-formation
activities, indicating that the environment does not affect these galaxy
properties. Among sixteen galaxies observed, only NGC 6104 shows a significant
star-formation activity, and shows a distorted morphology, indicating a tidal
interaction. This galaxy contains double knots, and only one knot possesses
Seyfert activity, though the sizes and luminosities are similar to each other;
we also discuss this feature.
A. Tomita
H. Maehara
T. T. Takeuchi
K. Nakanishi
M. Honma
Y. Tutui
Y. Sofue
08/12/2016--
08/12/2016
$σ$-Ideals and outer measures on the real line
A {\it weak selection} on $\mathbb{R}$ is a function $f: [\mathbb{R}]^2 \to
\mathbb{R}$ such that $f(\{x,y\}) \in \{x,y\}$ for each $\{x,y\} \in
[\mathbb{R}]^2$. In this article, we continue with the study (which was
initiated in \cite{ag}) of the outer measures $\lambda_f$ on the real line
$\mathbb{R}$ defined by weak selections $f$. One of the main results is to show
that $CH$ is equivalent to the existence of a weak selection $f$ for which: \[
\mathcal \lambda_f(A)= \begin{cases} 0 & \text{if $|A| \leq \omega$,}\\ \infty
& \text{otherwise.} \end{cases} \] Some conditions are given for a
$\sigma$-ideal of $\mathbb{R}$ in order to be exactly the family
$\mathcal{N}_f$ of $\lambda_f$-null subsets for some weak selection $f$. It is
shown that there are $2^\mathfrak{c}$ pairwise distinct ideals on $\mathbb{R}$
of the form $\mathcal{N}_f$, where $f$ is a weak selection. Also we prove that
Martin Axiom implies the existence of a weak selection $f$ such that
$\mathcal{N}_f$ is exactly the $\sigma$-ideal of meager subsets of
$\mathbb{R}$. Finally, we shall study pairs of weak selections which are
"almost equal" but they have different families of $\lambda_f$-measurable sets.
S. García-Ferreira
A. H. Tomita
Y. F. Ortiz-Castillo
10/20/2022--
10/20/2022
Collective Thomson scattering in non-equilibrium laser produced two-stream plasmas
We investigate collective Thomson scattering (CTS) in two-stream
non-equilibrium plasmas analytically, numerically and experimentally. In
laboratory astrophysics, CTS is a unique tool to obtain local plasma
diagnostics. While the standard CTS theory assumes plasmas to be linear,
stationary, isotropic and equilibrium, it is often nonlinear, non-stationary,
anisotropic, and non-equilibrium in high energy phenomena relevant to
laboratory astrophysics. We theoretically calculate and numerically simulate
the CTS spectra in two-stream plasmas as a typical example of non-equilibrium
system in space and astrophysical plasmas. The simulation results show the
feasibility to diagnose two-stream instability directly via CTS measurements.
In order to confirm the non-equilibrium CTS analysis, we have been developing
experimental system with high repetition rate table top laser for laboratory
astrophysics.
K. Sakai
S. Isayama
N. Bolouki
M. S. Habibi
Y. L. Liu
Y. H. Hsieh
H. H. Chu
J. Wang
S. H. Chen
T. Morita
K. Tomita
R. Yamazaki
Y. Sakawa
S. Matsukiyo
Y. Kuramitsu
10/19/2023--
10/19/2023
A family of Mordell curves with the rank of at least three
We constructed a parametrized family of Mordell curves with the rank of at
least three.
Seiji Tomita
01/15/2024--
01/15/2024
On the diophantine equation $X^6-Y^6 = W^n-Z^n, n=2,3,4$
In this paper, we proved that there are infinitely many integer solutions of
$X^6 - Y^6 = W^n - Z^n,\ n=2,3,4$.
Seiji Tomita
05/06/1999--
05/06/1999
Central Rotation Curves of Spiral Galaxies
We present high-resolution central-to-outer rotation curves for Sb, SBb, Sc,
and SBc galaxies. We discuss their general characteristics, particularly their
central behavior, as well as dependencies on morphological types, activity, and
peculiarity. The rotation curves generally show a steep nuclear rise, and
high-velocity central rotation, followed by a broad maximum in the disk and
then by a flat rotation due to the massive halo. Since the central high
velocity and steep rise are common to all massive galaxies, it cannot be due to
non-circular motions. Disk rotation curves of barred galaxies show larger
dispersion than those of normal galaxies which is probably due to non-circular
motions. Interacting galaxies show often perturbed outer rotation curves, while
their central rotation shows no particular peculiarity. Also, central
activities, such as starbursts and AGN, appear to show no particular
correlation with the property of rotation curves. This would suggest that the
central activities are triggered by a more local effect than the global
dynamical property.
Y. Sofue
Y. Tutui
M. Honma
A. Tomita
T. Takamiya
J. Koda
Y. Takeda
03/05/2008--
03/05/2008
Cross-talk suppressed multi-anode MCP-PMT
We have developed a 4-channel multi-anode MCP-PMT, SL10, which exhibits a
performance of sigma_TTS ~ 30 ps for single photons with G ~ 10^6 and QE=20%
under a magnetic field of B <= 1.5 T. The cross-talk among anodes has been
extensively studied. We have taken two measures to suppress it: one is to
configure the SL10 to an effectively independent 4 small pieces of MCP-PMT's by
segmenting an electrode of the second MCP-layer; the other is to use a constant
fractional discriminator. Remarkable improvement has been achieved.
K. Inami
T. Mori
T. Matsumura
K. Kurimoto
S. Hasegawa
Y. Suzuki
T. Murase
Y. Yurikusa
M. Akatsu
Y. Enari
T. Hokuue
A. Tomita
N. Kishimoto
T. Ohshima
T. Ihara
H. Nishizawa
03/18/2011--
03/18/2011
Field test of quantum key distribution in the Tokyo QKD Network
A novel secure communication network with quantum key distribution in a
metropolitan area is reported. Different QKD schemes are integrated to
demonstrate secure TV conferencing over a distance of 45km, stable long-term
operation, and application to secure mobile phones.
M. Sasaki
M. Fujiwara
H. Ishizuka
W. Klaus
K. Wakui
M. Takeoka
A. Tanaka
K. Yoshino
Y. Nambu
S. Takahashi
A. Tajima
A. Tomita
T. Domeki
T. Hasegawa
Y. Sakai
H. Kobayashi
T. Asai
K. Shimizu
T. Tokura
T. Tsurumaru
M. Matsui
T. Honjo
K. Tamaki
H. Takesue
Y. Tokura
J. F. Dynes
A. R. Dixon
A. W. Sharpe
Z. L. Yuan
A. J. Shields
S. Uchikoga
M. Legre
S. Robyr
P. Trinkler
L. Monat
J. -B. Page
G. Ribordy
A. Poppe
A. Allacher
O. Maurhart
T. Langer
M. Peev
A. Zeilinger
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