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Izquierda en crisis
La reciente derrota electoral del SPD alemán y el anunciado triunfo
de los conservadores británicos, según indican todas las
encuestas cuando se convoquen elecciones en aquél país, vienen
a subrayar la crisis de la izquierda socialdemócrata en Europa.
La izquierda se muestra perpleja de que los ciuadadanos no pasen factura a
los partidos que inspiraron las políticas económicas causantes
de la crisis. Se olvidan, así, de que mientras gobernó no
trató de corregirlas ni de cuestionarlas. Más bien les
ofreció un aval en la línea de la Tercera Vía de Tony
Blair y se limitó a marcar sus diferencias con los conservadores en
terrenos como los valores y las costumbres. Como consecuencia, la izquierda
no sólo no se ha legitimado como alternativa cuando tenía que
hacerlo, sino que, en muchos casos, la crisis le sorprendió en el
Gobierno, gestionando la economía desde los presupuestos que han
fracasado y que los electores castigan en su cabeza. Cuando ahora los
conservadores adoptan para salir de la crisis las políticas que
tradicionalmente se asociaban a la socialdemocracia, no hacen más
que ocupar un territorio que ésta dejó vacío durante
los años de bonanza.
La reacción de la izquierda ante esta situación no puede
resultar más equivocada. Por una parte, se ha dedicado a buscar los
problemas en su interior, desencadenando luchas de liderazgo que, hasta el
momento, se han saldado con una victoria de los aparatos y, por
consiguiente, de los dirigentes que mejor los controlan, no de los más
capaces y experimentados. Por otra, ha reforzado el discurso de los valores
y las costumbres, que la crisis ha convertido en una lengua de madera de
acentos beatíficos y compleja traducción práctica.
Mientras los partidos a la izquierda no dispongan de un análisis de
lo que está pasando, y no tanto de lo que les ocurre a ellos, es
difícil que puedan revertir una tendencia electoral que los está
alejando del poder en los países más importantes de Europa.
Why is space black?
Why is
space black?, NASA's Science Question of the Week, Goddard
Space Flight Center, 28 Marzo 2003.
Simple, isn't it? Why is space black?
Many different explanations have been put forward to resolve Olbers' Paradox.
The best solution at present is that the Universe is not infinitely old; it is
somewhere around 15 billion years old. That means we can only see objects as
far away as the distance light can travel in 15 billion years. The light from
stars farther away than that has not yet had time to reach us and so can't
contribute to making the sky bright.
Another reason that the sky may not be bright with the visible light of all the
stars is because when a source of light is moving away from you, the wavelength
of that light is made longer (which for light means more red.) This means that
the light from stars that are moving away from us will become shifted towards
red, and may shift so far that it is no longer visible at all. (Note: You hear
the same effect when an ambulance passes you, and the pitch of the siren gets
lower as the ambulance travels away from you; this effect is called the Doppler
Effect).
Supermassive Black Holes Bringing Universe Closer to Death
In spite of all the erupting stars, colliding galaxies and collapsing black
holes, the cosmos is quite orderly. So far, all theoretical calculations
have proven that the entropy of the universe is just a tiny fraction of the
maximum allowable amount. But why?
An analysis by Chas Egan of the Australian National University in Canberra and
Charles Lineweaver of the University of New South Wales in Sydney indicates
that the collective entropy of all the supermassive black holes at the centers
of galaxies is about 100 times higher than previously calculated. Because
supermassive black holes are the largest contributor to cosmic entropy, the
finding suggests that the entropy of the universe is also about 100 times
larger than previous estimates, the researchers reported online September 23 at
arXiv.org.
Entropy quantifies the number of different microscopic states that a physical
system can have while looking the same on a large scale. For instance, an
omelet has higher entropy than an egg because there are more ways for the
molecules of an omelet to rearrange themselves and still remain an omelet than
for an egg, notes cosmologist Sean Carroll of the California Institute of
Technology in Pasadena.
A black hole is the entropy champ because there are myriad ways for all the
material that has fallen into it to be arranged microscopically while the black
hole retains the same numerical values for its observable properties — charge,
mass and spin.
(...)
Having a more reliable entropy estimate is important, says Egan, because for
life or other complex phenomena to exist, the entropy of the universe must be
less than the maximum possible value. Consider, he notes, when hot water is
poured into a cold bath. Initially the hot and cold water are separate and the
system is orderly — it has low entropy. But once the hot and cold water are
thoroughly mixed, the entropy is maximized and no further heat flow is
possible.
In the case of the universe, Egan says, “we’d like to know [when and] if the
entropy will eventually reach a maximum value, marking the end of all
dissipative processes, including life.” Physicists have dubbed that maximum
entropy “heat death.”
(...)
Not everyone agrees that the higher entropy contributed by supermassive black
holes puts the universe closer to heat death. Theorist Ned Wright of the
University of California, Los Angeles says that because the extra entropy is
locked inside the black holes, the rest of the universe should have lower
entropy and be further away from heat death.
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