Downloads & Free Reading Options - Results

Recent observations suggest that some high-velocity clouds may be confined by massive dark matter halos. In particular, the proximity and proposed dark matter content of the Smith Cloud make it a tempting target for the indirect detection of dark matter annihilation. We argue that the Smith Cloud may be a better target than some Milky Way dwarf spheroidal satellite galaxies and use gamma-ray observations from the Fermi Large Area Telescope to search for a dark matter annihilation signal. No significant gamma-ray excess is found coincident with the Smith Cloud, and we set strong limits on the dark matter annihilation cross section assuming a spatially-extended dark matter profile consistent with dynamical modeling of the Smith Cloud. Notably, these limits exclude the canonical thermal relic cross section ($\sim 3\times10^{-26}{\rm cm}^{3}{\rm s}^{-1}$) for dark matter masses $\lesssim 30$ GeV annihilating via the $b \bar b$ or $\tau^{+}\tau^{-}$ channels for certain assumptions of the dark matter density profile; however, uncertainties in the dark matter content of the Smith Cloud may significantly weaken these constraints.

We report the first result of weak gravitational lensing survey on a 2.1 sq deg Rc-band image taken with a wide field camera (Suprime-Cam) on the prime focus of 8.2 m Subaru Telescope. The weak lensing mass reconstruction is applied to the data to search for dark matter halos of cluster scale; M >= 10^14 solar mass. The reconstructed convergence field is divided by 1-sigma noise to obtain the signal-to-noise ratio map (S/N-map) of the detection. Local maxima and minima are searched on the S/N-map and the probability distribution function (PDF) of the peaks are created to compare with model predictions. We found excess over noise PDF created from the randomized realization on both positive and negative sides. Negative peaks imply the presence of voids in the dark matter distribution and this is the first report of the detection. Positive peaks, on the other hand, represent the dark matter halos and the number count of the halos on the 2.1 sq deg image is 4.9 +- 2.3 for S/N > 5 where the Gaussian smoothing radius of the convergence map is 1'. The result is consistent with the prediction assuming the Press-Schechter mass function and the NFW halo profile under the cluster normalized CDM cosmology. Although the present statistics is not enough due to the limited field of view, this work demonstrates that dark matter halo count via weak lensing is a promising way to test the paradigm of structure formation and cosmological model.

In a recent preprint entitled "Searching for dark matter in X-rays: how to check the dark matter origin of a spectral feature" [arXiv:1001.0644v1], the authors have claimed that some archival X-ray data could be used to rule out dark matter in the form of 5-keV sterile neutrinos at the level of 20 sigma. Unfortunately, the limit was derived incorrectly. We point out the shortcomings of this analysis and show that the tentative detection of a spectral feature consistent with a 5-keV sterile neutrino is not in contradiction with existing limits. Future observations of dwarf spheroidal galaxies will test this hypothesis.

We present here the prospects for the GLAST Large Area Telescope (LAT) detection of the signature of the lightest Kaluza-Klein particle (LKP). It decays by direct annihilation into electron-positron pairs that may be detectable in the high energy electron flux. We discuss the LAT capability for detecting the high energy (20 GeV - ~1 TeV) cosmic ray electron flux and we analyze the LAT sensitivity to detect LKP-produced electrons for various particle masses. We include an analysis of the diffusive propagation of the electrons in the galaxy.

Recent observations suggest that some high-velocity clouds may be confined by massive dark matter halos. In particular, the proximity and proposed dark matter content of the Smith Cloud make it a tempting target for the indirect detection of dark matter annihilation. We argue that the Smith Cloud may be a better target than some Milky Way dwarf spheroidal satellite galaxies and use gamma-ray observations from the Fermi Large Area Telescope to search for a dark matter annihilation signal. No significant gamma-ray excess is found coincident with the Smith Cloud, and we set strong limits on the dark matter annihilation cross section assuming a spatially extended dark matter profile consistent with dynamical modeling of the Smith Cloud. Notably, these limits exclude the canonical thermal relic cross section (approximately 3 x 10 (sup -26) cubic centimeters per second) for dark matter masses less than or approximately 30 gigaelectronvolts annihilating via the B/B- bar oscillation or tau/antitau channels for certain assumptions of the dark matter density profile; however, uncertainties in the dark matter content of the Smith Cloud may significantly weaken these constraints.

We apply the linear filter for the weak-lensing signal of dark-matter halos developed in Maturi et al. (2005) to the cosmic-shear data extracted from the Garching-Bonn-Deep-Survey (GaBoDS). We wish to search for dark-matter halos through weak-lensing signatures which are significantly above the random and systematic noise level caused by intervening large-scale structures. We employ a linear matched filter which maximises the signal-to-noise ratio by minimising the number of spurious detections caused by the superposition of large-scale structures (LSS). This is achieved by suppressing those spatial frequencies dominated by the LSS contamination. We confirm the improved stability and reliability of the detections achieved with our new filter compared to the commonly-used aperture mass (Schneider, 1996; Schneider et al., 1998) and to the aperture mass based on the shear profile expected for NFW haloes (see e.g. Schirmer et al., 2004; Hennawi & Spergel, 2005). Schirmer et al.~(2006) achieved results comparable to our filter, but probably only because of the low average redshift of the background sources in GaBoDS, which keeps the LSS contamination low. For deeper data, the difference will be more important, as shown by Maturi et al. (2005). We detect fourteen halos on about eighteen square degrees selected from the survey. Five are known clusters, two are associated with over-densities of galaxies visible in the GaBoDS image, and seven have no known optical or X-ray counterparts.

We present an observational estimate of the fraction and distribution of dark mass in the innermost region of the two Galactic globular clusters NGC 6218 (M12) and NGC 288. Such an assessment has been made by comparing the dynamical and luminous mass profiles derived from an accurate analysis of the most extensive spectroscopic and photometric surveys performed on these stellar systems. We find that non-luminous matter constitutes more than 60% of the total mass in the region probed by our data (R

We investigate singlet scalar dark matter (DM) candidate in a left-right symmetric gauge model with two Higgs bidoublets (2HBDM) in which the stabilization of the DM particle is induced by the discrete symmetries P and CP. According to the observed DM abundance, we predict the DM direct and indirect detection cross sections for the DM mass range from 10 GeV to 500 GeV. We show that the DM indirect detection cross section is not sensitive to the light Higgs mixing and Yukawa couplings except the resonance regions. The predicted spin-independent DM-nucleon elastic scattering cross section is found to be significantly dependent on the above two factors. Our results show that the future DM direct search experiments can cover the most parts of the allowed parameter space. The PAMELA antiproton data can only exclude two very narrow regions in the 2HBDM. It is very difficult to detect the DM direct or indirect signals in the resonance regions due to the Breit-Wigner resonance effect.

[Abridged] Though the exact role of infrared dark clouds in the formation process is still somewhat unclear, they seem to provide useful laboratories to study the very early stages of clustered star formation. Infrared dark clouds have been identified predominantly toward the bright inner parts of the galactic plane. The low background emission makes it more difficult to identify similar objects in mid-infrared absorption in the outer parts. This is unfortunate, because the outer Galaxy represents the only nearby region where we can study effects of different (external) conditions on the star formation process. The aim of this paper is to identify extended red regions in the outer galactic plane based on reddening of stars in the near-infrared. We argue that these regions appear reddened mainly due to extinction caused by molecular clouds and young stellar objects. The work presented here is used as a basis for identifying star forming regions and in particular the very early stages. We use the Mann-Whitney U-test, in combination with a friends-of-friends algorithm, to identify extended reddened regions in the 2MASS all-sky JHK survey. We process the data on a regular grid using two different resolutions, 60" and 90". The two resolutions have been chosen because the stellar surface density varies between the crowded spiral arm regions and the sparsely populated galactic anti-center region. We identify 1320 extended red regions at the higher resolution and 1589 at the lower resolution run. The majority of regions are associated with major molecular cloud complexes, supporting our hypothesis that the reddening is mostly due to foreground clouds and embedded objects.

We present results of a search for the 3.5 keV emission line in our recent very long (~ 1.4 Ms) XMM-Newton observation of the Draco dwarf spheroidal galaxy. The astrophysical X-ray emission from such dark matter-dominated galaxies is faint, thus they provide a test for the dark matter origin of the 3.5 keV line previously detected in other massive, but X-ray bright objects, such as galaxies and galaxy clusters. We do not detect a statistically significant emission line from Draco; this constrains the lifetime of a decaying dark matter particle to tau > (7-9) x 10^27 s at 95% CL (combining all three XMM-Newton cameras; the interval corresponds to the uncertainty of the dark matter column density in the direction of Draco). The PN camera, which has the highest sensitivity of the three, does show a positive spectral residual (above the carefully modeled continuum) at E = 3.54 +/- 0.06 keV with a 2.3 sigma significance. The two MOS cameras show less-significant or no positive deviations, consistently within 1 sigma with PN. Our Draco limit on tau is consistent with previous detections in the stacked galaxy clusters, M31 and the Galactic Center within their 1-2 sigma uncertainties, but is inconsistent with the high signal from the core of the Perseus cluster (which has itself been inconsistent with the rest of the detections). We conclude that this Draco observation does not exclude the dark matter interpretation of the 3.5 keV line in those objects.

We explored several viable scenarios of how LAT might observe DM, when the spectral feature is predicted to be observed in the HE electron flux It has been demonstrated elsewhere that LAT will be capable to detect HE electrons flux in energy range from 20 GeV to - 1 TeV with 520% energy resolution and good statistics If there is a DM-caused feature in the HE electron flux (in the range 20 GeV - 1 TeV), LAT will be the best current instrument to observe it!

A signal from decaying dark matter (DM) can be unambiguously distinguished from spectral features of astrophysical or instrumental origin by studying its spatial distribution. We demonstrate this approach by examining the recent claim of 0912.0552 regarding the possible DM origin of the 2.5 keV line in Chandra observations of the Milky Way satellite known as Willman 1. Our conservative strategy is to adopt a relatively large dark mass for Willman 1 and relatively small dark masses for the comparison objects. We analyze archival observations by XMM-Newton of M31 and Fornax dwarf spheroidal galaxy (dSph) and Chandra observations of Sculptor dSph. By performing a conservative analysis of X-ray spectra, we show the absence of a DM decay line with parameters consistent with those of 0912.0552. For M31, the observations of the regions between 10 and 20 kpc from the center, where the uncertainties in the DM distribution are minimal, make a strong exclusion at the level above 10sigma. The minimal estimate for the amount of DM in the central 40 kpc of M31 is provided by the model of 0912.4133, assuming the stellar disk's mass to light ratio ~8 and almost constant DM density within a core of 28 kpc. Even in this case one gets an exclusion at 5.7sigma from central region of M31 whereas modeling all processed data from M31 and Fornax produces more than 14sigma exclusion. Therefore, despite possible systematic uncertainties, we exclude the possibility that the spectral feature at ~2.5 keV found in 0912.0552 is a DM decay line. We conclude, however, that the search for DM decay line, although demanding prolonged observations of well-studied dSphs, M31 outskirts and other similar objects, is rather promising, as the nature of a possible signal can be checked. An (expected) non-observation of a DM decay signal in the planned observations of Willman 1 should not discourage further dedicated observations.

Light From Darkness? Searching For Dark Matter. Dr. Tracy Slatyer explains how dark matter –the mysterious 85 percent of the matter in the universe—continues to elude scientific understanding. She describes how dark matter collisions might create observable signals, and how we can attempt to pick out those signals from telescope observations.

High-precision measurements of the temperature and polarization anisotropies of the cosmic microwave background radiation have been previously employed to set robust constraints on dark matter annihilation during recombination. In this work we improve and generalize these constraints to apply to energy deposition during the recombination era with arbitrary redshift dependence. Our approach also provides more rigorous and model-independent bounds on dark matter annihilation and decay scenarios. We employ principal component analysis to identify a basis of weighting functions for the energy deposition. The coefficients of these weighting functions parameterize any energy deposition model and can be constrained directly by experiment. For generic energy deposition histories that are currently allowed by WMAP7 data, up to 3 principal component coefficients are measurable by Planck and up to 5 coefficients are measurable by an ideal cosmic variance limited experiment. For WIMP dark matter, our analysis demonstrates that the effect on the CMB is described well by a single (normalization) parameter and a "universal" redshift dependence for the energy deposition history. We give WMAP 7 constraints on both generic energy deposition histories and the universal WIMP case.

Performer: THE WESTWAY STUDIO ORCHESTRA Writer: Roger Roger; J. Scott Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 2.0mil truncated conical, 2.3mil truncated conical, 2.8mil truncated conical, 3.3mil truncated conical. These were recorded flat and then also equalized with Turnover: 482.0, Rolloff: -13.75. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: SMP 1471 IU Catalog number: MQ731 Other IDs from the record include: SMP 1471

We present spectral data cubes of the [CI] 809GHz, 12CO 115GHz, 13CO 110GHz and HI 1.4GHz line emission from an 1 square degree region along the l = 328{\deg} (G328) sightline in the Galactic Plane. Emission arises principally from gas in three spiral arm crossings along the sight line. The distribution of the emission in the CO and [CI] lines is found to be similar, with the [CI] slightly more extended, and both are enveloped in extensive HI. Spectral line ratios per voxel in the data cubes are found to be similar across the entire extent of the Galaxy. However, towards the edges of the molecular clouds the [CI]/13CO and 12CO/13CO line ratios rise by ~50%, and the [CI]/HI ratio falls by ~10$%. We attribute this to these sightlines passing predominantly through the surfaces of photodissociation regions (PDRs), where the carbon is found mainly as C or C+, while the H2 is mostly molecular, and the proportion of atomic gas also increases. We undertake modelling of the PDR emission from low density molecular clouds excited by average interstellar radiation fields and cosmic-ray ionization to quantify this comparison, finding that depletion of sulfur and reduced PAH abundance is needed to match line fluxes and ratios. Roughly one-third of the molecular gas along the sightline is found to be associated with this surface region, where the carbon is largely not to be found in CO. ~10% of the atomic hydrogen along the sightline is cold gas within PDRs.

We present spectral data cubes of the [CI] 809GHz, 12CO 115GHz, 13CO 110GHz and HI 1.4GHz line emission from an 1 square degree region along the l = 328{\deg} (G328) sightline in the Galactic Plane. Emission arises principally from gas in three spiral arm crossings along the sight line. The distribution of the emission in the CO and [CI] lines is found to be similar, with the [CI] slightly more extended, and both are enveloped in extensive HI. Spectral line ratios per voxel in the data cubes are found to be similar across the entire extent of the Galaxy. However, towards the edges of the molecular clouds the [CI]/13CO and 12CO/13CO line ratios rise by ~50%, and the [CI]/HI ratio falls by ~10$%. We attribute this to these sightlines passing predominantly through the surfaces of photodissociation regions (PDRs), where the carbon is found mainly as C or C+, while the H2 is mostly molecular, and the proportion of atomic gas also increases. We undertake modelling of the PDR emission from low density molecular clouds excited by average interstellar radiation fields and cosmic-ray ionization to quantify this comparison, finding that depletion of sulfur and reduced PAH abundance is needed to match line fluxes and ratios. Roughly one-third of the molecular gas along the sightline is found to be associated with this surface region, where the carbon is largely not to be found in CO. ~10% of the atomic hydrogen along the sightline is cold gas within PDRs.

The dark matter halo of the Milky Way is expected to contain an abundance of smaller subhalos. These subhalos can be dense and produce potentially observable fluxes of gamma rays. In this paper, we search for dark matter subhalo candidates among the sources in the Fermi-LAT Second Source Catalog which are not currently identified or associated with counterparts at other wavelengths. Of the nine high-significance, high-latitude (|b|>60 degrees), non-variable, unidentified sources contained in this catalog, only one or two are compatible with the spectrum of a dark matter particle heavier than approximately 50-100 GeV. The majority of these nine sources, however, feature a spectrum that is compatible with that predicted from a lighter (~5-40 GeV) dark matter particle. This population is consistent with the number of observable subhalos predicted for a dark matter candidate in this mass range and with an annihilation cross section of a simple thermal relic (sigma v~3x10^{-26} cm^3/s). Observations in the direction of these sources at other wavelengths will be necessary to either reveal their astrophysical nature (as blazars or other active galactic nuclei, for example), or to further support the possibility that they are dark matter subhalos by failing to detect any non-gamma ray counterpart.

Theoretical challenges to understand Dark Matter and Dark Energy suggest the existence of low-mass and weakly coupling fields in the universe. The quasi-parallel photon-photon collision system (QPS) can provide chances to probe the resonant production of these light dark fields and the induced decay by the coherent nature of laser fields simultaneously. By focusing high-intensity lasers with different colors in the vacuum, new colors emerge as the signature of the interaction. Because four photons in the initial and final states interplay via the dark field exchange, this process is analogous to four-wave mixing in quantum optics, where the frequency sum and difference among the incident three waves generate the fourth wave with a new frequency via the nonlinear property of crystals. The interaction rate of the four-wave mixing process has the cubic dependence on the intensity of each wave. Therefore, if high-intensity laser fields are given, the sensitivity to the weakly coupling of dark fields to photons rapidly increases over the wide mass range below sub-eV. Based on the experimentally measurable photon energies and the linear polarization states, we formulate the relation between the accessible mass-coupling domains and the high-intensity laser parameters, where the effects of the finite spectrum width of pulse lasers are taken into account. The expected sensitivity suggests that we have a potential to explore interactions at the Super-Planckian coupling strength in the sub-eV mass range, if the cutting-edge laser technologies are properly combined.

We study a simplified scenario in the next-to-minimal supersymmetric standard model with a split electroweak spectrum, in which only the singlino and higgsinos are light and other superpartners are decoupled. Serving as a dark matter candidate, a singlino-dominated neutralino $\tilde{\chi}_1^0$ should have either resonant annihilation effects or sizable higgsino components to satisfy the observed relic abundance. The sensitivities of LHC searches and dark matter detection experiments are investigated. With an integrated luminosity of $30 (300) \mathrm{fb}^{-1}$, $3l + E_\mathrm{T} \!\!\!\!\!\!\!/ \;\;\;$and $2l + E_\mathrm{T} \!\!\!\!\!\!\!/ \;\;\;$ searches at the 13 (14) TeV LHC are expected to reach up to $m_{\tilde{\chi}_1^0}\sim 150 (230) \mathrm{GeV}$ and $m_{\tilde{\chi}_2^0,\tilde{\chi}_1^{\pm}}\sim 320 (480) \mathrm{GeV}$. Near future dark matter direct and indirect detection experiments can cover some parameter regions where collider searches lose their sensitivities.

We study a simplified scenario in the next-to-minimal supersymmetric standard model with a split electroweak spectrum, in which only the singlino and higgsinos are light and other superpartners are decoupled. Serving as a dark matter candidate, a singlino-dominated neutralino $\tilde{\chi}_1^0$ should have either resonant annihilation effects or sizable higgsino components to satisfy the observed relic abundance. The sensitivities of LHC searches and dark matter detection experiments are investigated. With an integrated luminosity of $30 (300) \mathrm{fb}^{-1}$, $3l + E_\mathrm{T} \!\!\!\!\!\!\!/ \;\;\;$and $2l + E_\mathrm{T} \!\!\!\!\!\!\!/ \;\;\;$ searches at the 13 (14) TeV LHC are expected to reach up to $m_{\tilde{\chi}_1^0}\sim 150 (230) \mathrm{GeV}$ and $m_{\tilde{\chi}_2^0,\tilde{\chi}_1^{\pm}}\sim 320 (480) \mathrm{GeV}$. Near future dark matter direct and indirect detection experiments can cover some parameter regions where collider searches lose their sensitivities.

We study current constraints and search prospects for a GeV scale vector boson at a range of low energy experiments. It couples to the Standard Model charged particles with a strength

208 pages : 22 cm

Williams spent his life as a doctor practicing pediatric medicine in northern New Jersey, a few miles west of New York City. During the work day, between seeing patients, he often dashed off poems on the backs of blank prescription pads that he kept in his pocket. This particular poem was written in just such a spontaneous way, after seeing the Russian Ballet perform in Manhattan. Each of the 16 readers in this collection took the challenge to make the same kind of leap - reading it spontaneously.<br />(Summary by Alan Davis-Drake)

2Velveteen Rabbit

By Margery Williams

<em>"What is REAL?"</em> asked the Rabbit one day... <br /><br />Written in 1922, <em>The Velveteen Rabbit</em>, or, <em>How Toys Become Real</em> is the tale of a sweet unassuming toy rabbit who questions what it is to live and to love. It was the first children's title written by Margery Williams (1881 - 1944), who had previously created only for adults. This story eclipsed all others, to become her most famous work, and an ever adored classic for all ages. (Summary written by Marlo Dianne)<br /><br /><em>"It was by a sort of accident that The Velveteen Rabbit became the beginning of all the stories I have written since…By thinking about toys and remembering toys, they suddenly become very much alive. Toys I had loved as a little girl--my almost forgotten Tubby, who was the rabbit, and Old Dobbin, the Skin Horse, and the toys my children had loved."</em> -- Margery Williams

3Velveteen Rabbit (version 2)

By Margery Williams

This classic story by Margery Williams, published in 1922, imparts the timeless message that toys need not be expensive or modern to be appreciated. Through giving and receiving love, even a commonplace stuffed animal can become real in the eyes of a child. This recording, read by a mother and daughter, is dedicated to Barbara Bear, who is real.<br /><br />Read by Barbara Bear and Mama Bear

Williams was born in Rutherford, New Jersey, a community near the city of Paterson. His father was an English immigrant, and his mother was born in Puerto Rico. He attended public school in Rutherford until 1897, then was sent to study at Château de Lancy near Geneva, Switzerland, the Lycée Condorcet in Paris, France, for two years and Horace Mann School in New York City. Then, in 1902, he entered the University of Pennsylvania Medical School. During his time at Penn, Williams befriended Ezra Pound, Hilda Doolittle (best known as H.D.) and the painter Charles Demuth. These friendships supported his growing passion for poetry. He received his M.D. in 1906 and spent the next four years in internships in New York City and in travel and postgraduate studies abroad (e.g., at the University of Leipzig where he studied pediatrics). He returned to Rutherford in 1910 and began his medical practice, which lasted until 1951. Ironically, most of his patients knew little if anything of his writings; instead they viewed him as a doctor who helped deliver over 2,000 of their children into the world. <br/>(From Wikipedia)

5Lincoln Story Book

By Henry L. Williams

Subtitle: A Judicious Collection of the Best Stories and Anecdotes of the Great President, Many Appearing Here for the First Time in Book Form - compiled by Henry L. Williams<BR><BR>The Abraham Lincoln Statue at Chicago is accepted as the typical Westerner of the forum, the rostrum, and the tribune, as he stood to be inaugurated under the war-cloud in 1861. But there is another Lincoln as dear to the common people--the Lincoln of happy quotations, the speaker of household words. Instead of the erect, impressive, penetrative platform orator we see a long, gaunt figure, divided between two chairs for comfort, the head bent forward, smiling broadly, the lips curved in laughter, the deep eyes irradiating their caves of wisdom; the story-telling Lincoln, enjoying the enjoyment he gave to others. (from the preface of the book) This is so big it took two pages on Internet Archive to store it all (Part 1 has 01 - 255 and part 2 has 256-391).<p>

6Harbor of Doubt

By Frank Williams

Young Code Schofield had lost his schooner May Schofield in an Atlantic gale a few months ago, and now the townspeople on the small island of Grande Mignon off the coast of New Brunswick were beginning to talk suspiciously of the events surrounding that loss. Insurance investigators have been summoned to investigate, friends are alienating themselves from Code, and he finds himsef challenged by even those he's known and trusted his whole life. Does Code Schofield have anything to prove, and if so, to whom, and why? (Summary by Roger Melin)

7All the Brothers Were Valiant

By Ben Ames Williams

Joel Shore, newly appointed captain of the whaling ship Nathan Ross following his brother's apparent demise as captain of the same ship, elects to make his first cruise as captain to the very location where his brother had last been seen - the Gilbert Islands, in order to try to learn more about what happened to his brother. The focus of this tale is of that voyage halfway around the globe and the adventures which he and his crew encounter. (Summary by Roger Melin)

8Why Marry?

By Jesse Lynch Williams

Why Marry? is a comedy, which "tells the truth about marriage". We find a family in the throes of proving the morality of marriage to a New Age Woman. Can the family defend marriage to this self-supporting girl? Will she be convinced that marriage is the ultimate sacredness of a relationship or will she hold to her perception that marriage is the basis of separating two lovers.<br><br>"Why Marry?" won the first Pulitzer Prize for Drama. (Summary by Linette Geisel) <br><br> <b>Cast:</b><br> Narrator- <a href="http://librivox.org/reader/1259">Elizabeth Klett</a></br> Jesse Lynch Williams - <a href="http://librivox.org/reader/1259">Elizabeth Klett</a></br> A most estimable lady - <a href="http://librivox.org/reader/123">Ezwa</a></br> Bachelor's niece - <a href="http://librivox.org/reader/4009">Diana Majlinger</a></br> JEAN, the host's younger sister, who has been brought up to be married and nothing else - <a href="http://librivox.org/reader/3536">Arielle Lipshaw</a></br> REX, an unmarried neighbor, who has not been brought up to be anything but rich - <a href="http://librivox.org/reader/5719">John Fricker</a></br> LUCY, the hostess, who is trying her best to be "just an old-fashioned wife" in a new-fashioned home - <a href="http://librivox.org/reader/5139">Katine</a></br> UNCLE EVERETT, a Judge, who belongs to the older generation and yet understands the new—and believes in divorce - <a href="http://librivox.org/reader/4705">Algy Pug</a></br> COUSIN THEODORE, a clergyman and yet a human being, who believes in everything—except divorce - <a href="http://librivox.org/reader/5189">Samanem</a></br> JOHN, who owns the house and almost every one in it—and does not believe in divorce - <a href="http://librivox.org/reader/6035">Marty Kris</a></br> HELEN, the host's other sister, whom every one wants to marry, but who doesn't want to marry any one - <a href="http://librivox.org/reader/4174">Availle</a></br> ERNEST, a scientist, who believes in neither divorce nor marriage but makes a great discovery - <a href="http://librivox.org/reader/5635">Matthew Reece</a></br> THE BUTLER - <a href="http://librivox.org/reader/2911">David Lawrence</a></br><br> <b>Audio edited by Linette Geisel</b>

9American Big-Game Hunting

By George S. Anderson, Winthrop Chanler, Oscar F. C. Crocker, Walter Bourchier Devereux, George Bird Grinnell, Arnold Hague, W. D. Pickett, Archibald Rogers, Theodore Roosevelt, Bronson Rumsey, Dean Sage, Roger D. Williams and Owen Wister

The first book published by The Boone and Crockett Club founded by Theodore Roosevelt and George Grinnell, who declared in their Editors Note: "Hunting big game in the wilderness is, above all things, a sport for a vigorous and masterful people. The rifle-bearing hunter, whether he goes on foot or on horseback, whether he voyages in a canoe or travels with a dog-sled, must be sound of body and firm of mind, and must possess energy, resolution, manliness, self-reliance, and capacity for hardy self-help. In short, the big-game hunter must possess qualities without which no race can do its life-work well; and these are the very qualities which it is the purpose of this Club, so far as may be, to develop and foster."<br /><br /> A bit outdated as to the equipment they used, this book is nevertheless an intense look at the west in early days, and at the beginnings of the conservationist movement in America. Each chapter focuses on a different animal, from buffalo, mountain goat, elk, pronghorn sheep, grizzlies, etc., indigenous peoples, different areas like the Rockies and Yellowstone, and it still captures the essence of the spirit of the hunt.<br /><br /> The book ends with a list of the club's original 100 members, a veritable Who's Who of Generals, Colonels, Doctors, Senators and Representatives, amongst them that most illustrious Gen'l William T. Sherman. ( ~ Michele Fry, read by LibriVox Volunteers)

10Indians Of Carlsbad Caverns National Park

By Jack R. Williams

A short review of the history and presence of Native Americans in the area of the Carlsbad Caverns in New Mexico, USA. - Summary by david wales

11Planet of the Gods

By Robert Moore Williams

Far, far in the future Earth has achieved real peace and is sending out interstellar expeditions, not to conquer, but to explore. The third such expedition, has made it to the Vega system and discovered to everyone's amazement, not only a solar system but two worlds circling the Vega sun that seem to have atmosphere and water. And apparently intelligent life is there as well because something tries, and almost succeeds, in blasting the expedition ship out of space before it can even get close to either one. Damaged, with 3 dead men aboard, the expedition ship semi-crashes and seeks to hide from this obviously hostile civilization. The three dead members of the crew are buried and four of the local inhabitants pay a friendly call. Then during the second night on this planet, one of the dead bodies knocks on the door and wants to come in. Something very strange is going on here.

12Hunting In Many Lands

By Henry T. Allen, George S. Anderson, Daniel Moreau Barringer, Winthrop Chanler, George H. Gould, Madison Grant, William Woodville Rockhill, Elliott Bulloch Roosevelt, Theodore Roosevelt, Alden Sampson, Henry L. Stimson, Charles E. Whitehead, Caspar W. Whitney and Roger D. Williams

The first volume published by the Boone and Crockett Club, entitled "American Big Game Hunting," confined itself to sport on the American continent. This second volume presents a number of interesting sketches written by club members who have hunted big game in other lands. Essays include: Hunting in East Africa, To the Gulf of Cortez, A Canadian Moose Hunt, A Hunting Trip in India, Dog Sledging in the North, Wolf-Hunting in Russia, A Bear-Hunt in the Sierras, The Ascent of Chief Mountain, The Cougar, Big Game of Mongolia and Tibet, Hunting in the Cattle Country, Wolf-Coursing, Game Laws, and Protection of the Yellowstone National Park. - Summary by Michele Fry

13The Chemistry of Cookery

By W. Mattieu Williams

This book, written in the late 1800s, is a book of chemistry that explains the whys and hows of cooking to trained chefs and laymen alike. The book deals with some compounds of common foodstuffs, like albumen or gluten, and illustrates what happens from a chemist's point of view during certain types of food preparation like roasting, frying, or stewing. A part of the chapters also details adulterations of food - thankfully since outlawed - and how to detect them in the finished product.

14Romance of Modern Invention

By Archibald Williams

This is a volume of exploration into the newest inventions of the turn of the previous century. Journalist Archibald Williams walks the reader through diverse inventions which were changing the world at just that point in time. - Summary by Carolin

15Hive of Busy Bees

By Effie Mae Hency Williams

In the summer, Don and Joyce stay on their Grandma and Grandpa's farm. They have great fun, and every night Grandma tells them a story about a different kind of bee such as Bee Kind, Bee Polite, and Bee Honest that stings people who aren't honest.

16Romance of Modern Mechanism

By Archibald Williams

In 1910, when this book was published, the advancement of modern mechanism was still moving at a rapid pace. It must have seemed like very day, new inventions were made to make life easier. Most of these are still very much in use today, such as the lawn-mower, automatic milking machines in the dairy industry, fire engines, and escalators. Learn about how these worked in this volume. - Summary by Carolin

Summer is around the corner, time to make ice cream! This volume contains tried and true recipes for all kinds of cold drinks and desserts to cool off on a hot summer day. Though published in 1891, these recipes can still sweeten this year's season. - Summary by Carolin

Ever wondered how football has changed over the years? Look no further! This selection of rules, positions, and explanations of how football was played in the late 1800s is sure to leave you with a greater knowledge of the evolution of the sport. (Summary by Campbell Schelp)

A book of William Carlos Williams's early poetry. Included in this recording are 18 poems published by Williams in Volume 13 of 'Poetry' literary journal in 1919. - Summary by KevinS

20Science in Short Chapters

By W. Mattieu Williams

This is a collection of articles written by W. Mattieu Williams on different subjects, that in his opinion "are likely to be interesting to all readers who are sufficiently intelligent to prefer sober fact to sensational fiction, but who, at the same time, do not profess to be scientific specialists." This book offers and intriguing glimpse into the scientific ideas of late 19th century. Though nowadays these essays should not be seen as wholly scientifically accurate, they are still entertaining and in many basic aspects remain truthful. - Summary by Kikisaulite

21Doomsday Eve

By Robert Moore Williams

In the midst of the war—that terrible conflict that threatened humanity's total destruction—the "new people" suddenly appeared. Quietly performing incredible deeds, vanishing at will, they were an enigma to both sides. Kurt Zen was an American intelligence officer among the many sent to root them out. He found them. Taken captive in their hidden lair, he waited as the enemy prepared to launch the super missile, the bomb to end all bombs—and all life. If only he could find the source of the new people's power, Kurt alone might be able to prevent obliteration of the Earth.... - Summary by Original text

A very brief introduction to postal stamps used and issued during times of war. The principal focus might be said to be placed upon the Great War which just erupted in Europe and across much of the globe. - Summary by KevinS

23Black Pawl

By Ben Ames Williams

This riveting novel takes place on a whaling ship, where its captain, Black Pawl, has a troubled relationship with the first mate, his son. A minister is permitted aboard for the homeward-bound journey along with a young woman who is accompanying him. Before long, unforeseen complications and electrifying events ensue. <br> Williams, an American author, wrote hundreds of short stories, many appearing in popular magazines, and over 30 novels, several of which were made into motion pictures. ( Lee Smalley)

24New Lamps

By Robert Moore Williams

Ronson came to the Red Planet on the strangest mission of all ... he only knew he wanted to see Les Ro, but he didn't know exactly why. It was because he knew that Les Ro had the answer to something that had never been answered before, if indeed, it had ever been asked! For Les Ro traded new lamps for old—and they were the lamps of life itself! A story of what life holds for all of us. - Summary by Author

25Man with the Clubfoot

By Valentine Williams

"The Man with the Clubfoot" is one of the most ingenious and sinister secret agents in Europe. It is to him that the task is assigned of regaining possession of an indiscreet letter written by the Kaiser.<br><br> Desmond Okewood, a young British officer with a genius for secret service work, sets out to thwart this man and, incidentally, discover the whereabouts of his brother.<br><br> He penetrates into Germany disguised, and meets with many thrilling adventures before he finally achieves his mission.<br><br> In "The Man with the Clubfoot," Valentine Williams has written a thrilling romance of mystery, love and intrigue, that in every sense of the word may be described as "breathless." - Summary by from original text

Joaquin Murrieta was a famous Californio bandit, known as the "Robin Hood of El Dorado".<br><br> <i>Joaquin Murrieta was the son of worthy parents, and nothing in his early youth betokened any traits of the monster which he afterwards became. . . . In the following pages every trace of his blood-stained footsteps is closely followed. Some of the facts are furnished by contemporary witnesses; most of them by official documents. He proceeded from step to step, wading deeper and deeper into crime, until quiet citizens were almost afraid to breathe his name aloud.<br><br> In addition to this being a faithful narration of the fearful deeds of Joaquin, incidentally the work gives a faithful delineation of "life in the diggings" in the early days of California, when almost every nugget of gold was blood-spotted ere rude Justice bared her death-dealing arm.</i><br><br> Murrieta is believed to have inspired the fictional character of Zorro by Johnston McCulley. You may judge for yourself how much of the account here is truthful and how much is sensationalized. - Summary by TriciaG & from the Synopsis

27Return of Clubfoot

By Valentine Williams

Whilst spending a holiday in a small Central American Republic, Desmond Okewood, of the Secret Service, learns from a dying beachcomber of a hidden treasure.<br><br> With the assistance of a millionaire, he sets out for Cock Island, in the Pacific. To his astonishment he discovers that the Man with the Clubfoot, whom he had regarded as dead, has anticipated him. It is obvious to Okewood that his old enemy is also in search of the hidden gold, and there ensues a thrilling sequence of adventures, in which the millionaire's pretty daughter takes a prominent part.<br><br> Okewood has the cipher, and the Man with the Clubfoot determines to secure it, for without that cipher it is impossible to discover the hiding-place of the treasure; but there is something that the Man with the Clubfoot does not know, whereas Okewood does. - Summary by Original Gutenberg text

A complete survey of the Independent Boise School District, Boise, Idaho was conducted over two weeks, with the purpose to study and observe the schools in operation, including the systems of financing and filing educational records. Facts are presented alongside conclusions and recommendations to be understood the general public as to the importance of educational enterprise. - Summary by Leon Harvey

Dr. Haverill is asked to fill in as local physician for the skittish Dr. Lennox in a small Pennsylvania town. The locals seem to be a superstitious bunch, prone to fearing traveling in the woods at night and with good reason. It seems a series of vicious attacks have occurred by what appears to be some kind of large animal. As the bodies begin to pile up, Dr. Haverill starts to question whether the responsible party could be something beyond humanity.<br><br> Writer Margery Williams Bianco (writing here under the pseudonym Harper Williams) is perhaps better known for writing the children's classic "The Velveteen Rabbit", but this dark slice of mystery horror fiction was found to be admired by none other than H. P. Lovecraft. Lovecraft scholars have noted in particular a distinct influence that this book had on his famous story "The Dunwich Horror".<br><br> Also please note that this book is of its time and features racially insensitive language in the early chapters. Those who are concerned with such language should be advised.

30Clubfoot the Avenger

By Valentine Williams

At the conclusion of The Return of Clubfoot, Dr. Grundt has been left for dead on a south sea island by former secret agent Desmond Oakwood. Oakwood and his brother Francis are now retired from the Secret Service and are living comfortably retired in England. But the body of an apparent suicide is discovered in a car park in London, and the possibility that Grundt is alive and seeking revenge in England pulls the Oakwoods out of retirement to once again face the sinister and deadly CLUBFOOT. - Summary by sjmarky

As it would be impossible to treat, in the compass of a few hundred pages, all the great engineering feats of modern times without reducing individual accounts to uninteresting brevity, the author has preferred, where selection is possible, to take typical instances of engineering practice, and, by the aid of comparatively detailed descriptions, to place the reader in a position to appreciate them and similar undertakings. - Summary by Adapted from the Preface

In the following pages we shall peep into the history of typical companies in Great Britain, the United States, and elsewhere; consider the various forms of traction, signals, and other mechanical appliances connected with the working of a railway; notice the effects of railway communication on a country for its peaceful development, or its conquest in war; and make the tour of a typical locomotive factory. These and other matters have been treated as simply as may be, but with sufficient fullness to give the reader a fair idea of what the railway really is, how it has been made, and what the future may have in store for it. - Summary by from the preface.

Any writer on mining in its general aspect is, when casting about for a starting-point, driven to express what others have said before him-that the history of mining is the history of civilization. The following pages, while touching on the chief branches of the mining industry, must necessarily omit reference to many of the great treasure-houses of the world. Special prominence has been given to the precious metals, because their discovery and working has witnessed the most stirring scenes in mining life. We have the whole world to roam over; so excursions are made into those spots where typical or prominent instances of mining of various minerals are to be found.

The Author has been encouraged by the reception given to <i>The Romance of Modern Exploration</i> to write a companion volume on the adventures of early travelers and explorers. For conveniences' sake the period covered ends at A.D. 1600, a date sufficiently advanced to permit mention of the first polar expeditions in which English navigators played so important a part.

It may be thought, perhaps, that exploration must be comparatively easy today. Less laborious no doubt it is in some details when Mandeville and Magellan travelled. But there are difficulties enough remaining to leave the romance of exploration untouched. Every explorer carries his life in his hand, however fine may be his outfit. Within the limits of this volume it is impossible even to notice all the modern explorers who have a claim on our admiration. - Summary adapted from the introduction

36Sour Grapes

By William Carlos Williams

A collection of poems largely collected from previous magazine and journal publications. (Summary by KevinS)

LibriVox volunteers bring you 9 recordings of Troy by Charles Williams.<br> This was the Fortnightly Poetry project for June 11, 2023. <br> ------<br> A poem about the women caught up in the Trojan War by Charles Williams, a member of the Inklings, an Oxford based group of writers that included J.R.R. Tolkien and C.S.Lewis. (Summary by Alan Mapstone)

A collection of short stories by Pansy, Rev. C.M. Livingston, and other authors. The first eleven stories are about Mary Burton, who, although she is unable to go to Europe like her cousin, decides to visit Britain through books and write letters to her friend of her "travels". - Summary by TriciaG

Charles Williams was one of The Inklings, an Oxford based group of writers which included J.R.R. Tolkien and C.S. Lewis. Although Williams' poetry was mainly influenced by his deeply held Christian faith, he also had a great knowledge of and respect for the ideas and values of the classical world. (Summary by Alan Mapstone)

Charles Williams was one of The Inklings, an Oxford based group of writers which included J.R.R. Tolkien and C.S. Lewis. <br><br> Although Williams' poetry was mainly influenced by his deeply held Christian faith, he also studied mysticism and had a great knowledge of and respect for the ideas and values of the classical world. <br><br> Divorce (1920) is Williams' third book of poetry following Poems of Conformity which is also available on Librivox. <br><br> (Summary by Alan Mapstone)

It is hardly needful to observe, that it is the incumbent duty of every faithful abridger, as well as a faithful translator, to adhere scrupulously to the sense of his author, except the reason to the contrary be universally obvious, nor even then without apprizing the reader of it. This is what I have endeavored throughout to pay the strictest regard to. The reader of the ensuing pages will find in them the genuine thoughts and sentiments of Dr. Owen, to the best of my knowledge, and no other. Sometimes, indeed, the abridger thought it absolutely necessary, in discharging his duty to his readers, to exchange an expression, or to alter a phraseology, for others that appear now more expressive, or better understood. And now and then he has taken the liberty, for a similar reason,of inserting an expressive or animating epithet, justified by the connexion; or turned a sentence merely declarative into an awakening interogation. Some may think that these liberties are after all ioo seldom used, while others are ready to entertain a jealousy, when they apprehend that any freedom is taken with an author whom they so much revere. To please all is impossible, while men's ideas of propriety and utility are so various; and, therefore, to attempt it would be a fruitless toil, the offspring of folly, and the parent of disappointment. Suffice it to say, that in the present undertaking the Editor has proposed as the end, the greatest and most general good, and with dependance on the head of all gifts and graces, the blessed and adorable Person, whose glory in the salvation of his people is the sublime and delightful subject of these volumes, he has pursued that end according to the best of his judgment. And he cannot help indulging a pleasing hope, that the cause of truth, the profitable knowledge of God our Savior, the edification of believers, and the increase of fervent love among brethren, will be promoted by the present attempt. - Summary by Editor's Preface

42Lost Warship

By Robert Moore Williams

A boat of survivors cast adrift in the South Seas is picked up by the US Naval battleship The Idaho. They think their prayers have been answered, but when Japanese bombers blast them into the prehistoric era via a rift in the space-time continuum, their troubles are only beginning! - Summary by Ben Tucker

This children's book, written by the author of "The Velveteen Rabbit", tells the story of Cecco, an adventurous and spirited wooden dog, who gets out of the toy cupboard and experiences many adventures with Bulka, the rag puppy, and other toy characters from the toy storage. - Summary by Mark Harrington