SearcharxivSearch

arXiv subjects

K. Gutierrez

Publications and source records attributed to K. Gutierrez.

3 recordsLinked to original sources

Exact results for the infinite supersymmetric extensions of the infinite square well

One-dimensional potentials defined by $V^{(S)}(x) =S(S+1) \hbar^2 π^2 /[2ma^2\sin^2(πx/a)]$ (for integer $S$) arise in the repeated supersymmetrization of the infinite square well, here defined over the region $(0,a)$. We review the derivation of this hierarchy of potentials and then use the methods of supersymmetric quantum mechanics, as well as more familiar textbook techniques, to derive compact closed-form expressions for the normalized solutions, $ψ_n^{(S)}(x)$, for all $V^{(S)}(x)$ in terms of well-known special functions in a pedagogically accessible manner. We also note how the solutions can be obtained as a special case of a family of shape-invariant potentials, the trigonometric Pöschl-Teller potentials, which can be used to confirm our results. We then suggest additional avenues for research questions related to, and pedagogical applications of, these solutions, including the behavior of the corresponding momentum-space wave functions $ϕ_n^{(S)}(p)$ for large $|p|$ and general questions about the supersymmetric hierarchies of potentials which include an infinite barrier.

quant-ph

Multiwavelength Observations of 1ES 1959+650, One Year After the Strong Outburst of 2002

In April-May 2003, the blazar 1ES 1959+650 showed an increased level of X-ray activity. This prompted a multiwavelength observation campaign with the Whipple 10 m gamma-ray telescope, the Rossi X-ray Timing Explorer, the Bordeaux Optical Observatory, and the University of Michigan Radio Astrophysical Observatory. We present the multiwavelength data taken from May 2, 2003 to June 7, 2003 and compare the source characteristics with those measured during observations taken during the years 2000 and 2002. The X-ray observations gave a data set with high signal-to-noise light curves and energy spectra; however, the gamma-ray observations did not reveal a major TeV gamma-ray flare. Furthermore, we find that the radio and optical fluxes do not show statistically significant deviations from those measured during the 2002 flaring periods. While the X-ray flux and X-ray photon index appear correlated during subsequent observations, the apparent correlation evolved significantly between the years 2000, 2002, and 2003. We discuss the implications of this finding for the mechanism that causes the flaring activity.

astro-ph

The Off-Axis Galaxy Cluster Merger Abell 115

We have used a 50.4 ksec Chandra obsffervation to examine the galaxy cluster Abell 115 (z=0.1971). The X-ray surface brightness distribution shows a merger of 2 sub-clusters with substantial off-axis motion. The northern sub-cluster moves toward the southwest and exhibits a strong X-ray surface brightness gradient toward this direction as well as a "fan" of X-ray bright Intra-Cluster Medium (ICM) toward the northeast. The southern sub-cluster shows a pronounced northeast-southwest elongation, probably as a consequence of the ongoing merger. The temperature of the ICM is highly non-uniform across the cluster. Although the merger is well underway and has had a substantial influence on the morphology of the 2 sub-clusters, it has apparently not disturbed the cool sub-cluster cores. The ICM in between the sub-clusters has a significantly elevated temperature of ~8 keV. However, owing to the low surface brightness, we do not find direct evidence for shocks in this region. The X-ray surface brightness distribution of the northern sub-cluster is highly non-uniform. The data show a bright central core region of about 10" (30 kpc) diameter. A highly significant surface brightness discontinuity separates the core from the ambient ICM. We discuss several possibilities to explain the compact core, and its relation to the central radio galaxy 3C 28.0 and the sub-cluster's cooling flow. Further outwards, at about 24.6" (80 kpc) to the southwest of the sub-cluster core, the surface brightness distribution shows a jump associated with a contact discontinuity. The Chandra imaging spectroscopy data do not show evidence for a shock associated with the surface brightness jump. We conclude that it is associated with denser plasma moving sub-sonically through the ambient plasma.

astro-ph