Lecturas “dirigidas" de la poesía estadounidense : The new american poetry (1960) y Legitimate dangers (2006)

Este artículo estudia dos antologías de poesía estadounidense publicadas en su país de origen en 1960 y en 2006, respectivamente: The New American Poetry, compilada por Donald Allen, y Legitimate Dangers: American Poets of the New Century, por Michael Dumanis y Cate Marvin. A cincuenta años de la aparición de la primera, la crítica reconoce la función rupturista, renovadora y, a la vez, seminal de la selección de Allen, quien presentaba su texto como una colección de poetas y poemas opuestos al “verso académico". Del mismo modo, Dumanis y Marvin presentan una antología que busca difundir autores jóvenes cuya poesía propone el riesgo como valor fundamental. Nuestro enfoque compara y contrasta ambas antologías, para señalar los aspectos comunes, las declaraciones de principios y las poéticas subyacentes a ambas, y los procesos de canonización que llevan a cabo.

Poetry for export : Contemporary Argentine Poetry (1969), de William Shand, una antología poética argentina en inglés

La traducción se planta como el medio para que un público ajeno a la lengua de origen de un texto pueda acceder a él. En el caso de la poesía, debido a su difícil traducción y a su escasa publicación, la problemática de la traducción se torna doble. A partir de entonces, la presentación de una antología poética argentina en inglés como carta de presentación de la literatura nacional en el mundo resulta una obra interesante en cuanto a sus contenidos y repercusiones en el canon internacional

Charles Segal. Aglaia. The Poetry of Alcman, Sappho, Pindar, Bacchylides and Corinna, Maryland, Rowman y Littlefield Publishers, Ine., 1998, 339 pp.

Fil: Errecalde, Alejandro Martín. Universidad Nacional de La Plata. Facultad de Humanidades y Ciencias de la Educación; Argentina.

Charles Segal. Aglaia. The Poetry of Alcman, Sappho, Pindar, Bacchylides and Corinna, Maryland, Rowman y Littlefield Publishers, Ine., 1998, 339 pp.

Fil: Errecalde, Alejandro Martín. Universidad Nacional de La Plata. Facultad de Humanidades y Ciencias de la Educación; Argentina.

Gregory Nagy. Poetry as Performance, Homer and Beyond. Cambrige-New York-Melbourne, Cambridge University Press, 1996, ix + 254 pp. ; Gregory Nagy. Homeric Questions, Austin, University of Texas Press, 1996, ix + 180 pp.

Fil: Zecchin de Fasano, Graciela Cristina. Universidad Nacional de La Plata. Facultad de Humanidades y Ciencias de la Educación; Argentina.

Poetry for export : Contemporary Argentine Poetry (1969), de William Shand, una antología poética argentina en inglés

La traducción se planta como el medio para que un público ajeno a la lengua de origen de un texto pueda acceder a él. En el caso de la poesía, debido a su difícil traducción y a su escasa publicación, la problemática de la traducción se torna doble. A partir de entonces, la presentación de una antología poética argentina en inglés como carta de presentación de la literatura nacional en el mundo resulta una obra interesante en cuanto a sus contenidos y repercusiones en el canon internacional

Poetry for export : Contemporary Argentine Poetry (1969), de William Shand, una antología poética argentina en inglés

La traducción se planta como el medio para que un público ajeno a la lengua de origen de un texto pueda acceder a él. En el caso de la poesía, debido a su difícil traducción y a su escasa publicación, la problemática de la traducción se torna doble. A partir de entonces, la presentación de una antología poética argentina en inglés como carta de presentación de la literatura nacional en el mundo resulta una obra interesante en cuanto a sus contenidos y repercusiones en el canon internacional

Charles Segal. Aglaia. The Poetry of Alcman, Sappho, Pindar, Bacchylides and Corinna, Maryland, Rowman y Littlefield Publishers, Ine., 1998, 339 pp.

Fil: Errecalde, Alejandro Martín. Universidad Nacional de La Plata. Facultad de Humanidades y Ciencias de la Educación; Argentina.

A non-perturbative Kolmogorov turbulence approach to the cosmic web structure

The Kolmogorov approach to turbulence is applied to the Burgers turbulence in the stochastic adhesion model of large-scale structure formation. As the perturbative approach to this model is unreliable, here a new, non-perturbative approach, based on a suitable formulation of Kolmogorov's scaling laws, is proposed. This approach suggests that the power-law exponent of the matter density two-point correlation function is in the range 1–1.33, but it also suggests that the adhesion model neglects important aspects of the gravitational dynamics.

Say The Word! Celebrate National Poetry Month with Inman E. Page Library

National Poetry Month is in full effect at Inman E. Page Library (April 2016)! Get ready to write, perform, and dialogue about the written word. We look forward to hearing your voice on the microphone.

Implications of a possible clustering of highest-energy cosmic rays

Recently, a possible clustering of a subset of observed ultra-high energy cosmic rays above ≃40 EeV (4 × 1019 eV) in pairs near the supergalactic plane was reported. We show that a confirmation of this effect would provide information on the origin and nature of these events and, in case of charged primaries, imply interesting constraints on the extragalactic magnetic field. Possible implications for the most common models of ultra-high energy cosmic ray production in the literature are discussed.

Cosmic microwave background theory

A long-standing goal of theorists has been to constrain cosmological parameters that define the structure formation theory from cosmic microwave background (CMB) anisotropy experiments and large-scale structure (LSS) observations. The status and future promise of this enterprise is described. Current band-powers in ℓ-space are consistent with a ΔT flat in frequency and broadly follow inflation-based expectations. That the levels are ∼(10−5)2 provides strong support for the gravitational instability theory, while the Far Infrared Absolute Spectrophotometer (FIRAS) constraints on energy injection rule out cosmic explosions as a dominant source of LSS. Band-powers at ℓ ≳ 100 suggest that the universe could not have re-ionized too early. To get the LSS of Cosmic Background Explorer (COBE)-normalized fluctuations right provides encouraging support that the initial fluctuation spectrum was not far off the scale invariant form that inflation models prefer: e.g., for tilted Λ cold dark matter sequences of fixed 13-Gyr age (with the Hubble constant H0 marginalized), ns = 1.17 ± 0.3 for Differential Microwave Radiometer (DMR) only; 1.15 ± 0.08 for DMR plus the SK95 experiment; 1.00 ± 0.04 for DMR plus all smaller angle experiments; 1.00 ± 0.05 when LSS constraints are included as well. The CMB alone currently gives weak constraints on Λ and moderate constraints on Ωtot, but theoretical forecasts of future long duration balloon and satellite experiments are shown which predict percent-level accuracy among a large fraction of the 10+ parameters characterizing the cosmic structure formation theory, at least if it is an inflation variant.

Cosmic velocity fields and their interpretation

We review the current status of our knowledge of cosmic velocity fields, on both small and large scales. A new statistic is described that characterizes the incoherent, thermal component of the velocity field on scales less than 2h−1 Mpc (h is H0/100 km·s−1·Mpc−1, where H0 is the Hubble constant and 1 Mpc = 3.09 × 1022 m) and smaller. The derived velocity is found to be quite stable across different catalogs and is of remarkably low amplitude, consistent with an effective Ω ∼ 0.15 on this scale. We advocate the use of this statistic as a standard diagnostic of the small-scale kinetic energy of the galaxy distribution. The analysis of large-scale flows probes the velocity field on scales of 10–60 h−1 Mpc and should be adequately described by linear perturbation theory. Recent work has focused on the comparison of gravity or density fields derived from whole-sky redshift surveys of galaxies [e.g., the Infrared Astronomical Satellite (IRAS)] with velocity fields derived from a variety of sources. All the algorithms that directly compare the gravity and velocity fields suggest low values of the density parameter, while the POTENT analysis, using the same data but comparing the derived IRAS galaxy density field with the Mark-III derived matter density field, leads to much higher estimates of the inferred density. Since the IRAS and Mark-III fields are not fully consistent with each other, the present discrepancies might result from the very different weighting applied to the data in the competing methods.