Archive for junio 19, 2012

Sin pruebas de texturas

Un análisis de los datos de WMAP obliga a limitar la existencia de texturas cósmicas.

Ciertas teorías predicen la existencia de “nudos” en el tejido del espacio conocidos como texturas cósmicas, y que éstas podrían ser identificadas estudiando el fondo cósmico de microondas (FCM). Investigadores del Imperial College London y del Perimeter Institute han usado datos del satélite WMPA para realizar el primer estudio global en busca de texturas cósmica. No han encontrado pruebas de existencia de esos objetos.

Según el Universo se iba expandiendo y enfriando una vez se dio el Big Bang, se tuvieron que dar distintas transiciones de fase. Estas transiciones de fase serían análogas a las que permite al vapor de agua condensarse en agua y a ésta congelarse. Estas transiciones no pueden darse de manera homogénea a lo largo de todo el espacio así que algunos teóricos propusieron que debían de producirse imperfecciones en el sistema, según éste se enfriaba, a las que llamaron texturas cósmicas. Si se generaron en el Universo temprano, esas texturas interaccionarían con la luz procedente del fondo cósmico dejando un conjunto de lugares más calientes o más fríos sobre el promedio de fondo. Si esas señales fueran detectadas entonces darían lugar a importantes pistas sobre los tipos de transiciones que podrían haber ocurrido cuando el Universo tenía una fracción de segundo de edad, lo que tendría drásticas implicaciones en la Física de partículas.

[Read More…]

Orbiter Out of Precautionary ‘Safe Mode’

NASA's Mars Odyssey spacecraft passes above Mars' south pole in this artist's concept illustration.

NASA's Mars Odyssey orbiter has been taken out of a protective status called safe mode.



Most Quasars Live on Snacks, Not Large Meals

The Homes of Quasars

Black holes in the early universe needed a few snacks rather than one giant meal to fuel their quasars and help them grow, according to observations from NASA's Spitzer and Hubble space telescopes.



CMS Status Report.

Author(s) Sirois, Yves (speaker) (Ecole Polytechnique (FR)) Corporate author(s) CERN. Geneva Series (LHCC Meetings - Open and Closed Sessions) (110 LHCC Meeting AGENDA OPEN Session) Lecture note on 2012-06-13T11:50:00 Subject category LHCC Meetings - Open and Closed Sessions Submitted by morna.robillard@cern.ch cdsweb.cern.ch
Views: 1
0 ratings
Time: 45:55 More in Science & Technology

ATLAS Status Report.

ATLAS Status Report © CERN Author(s) Monig, Klaus (speaker) (Deutsches Elektronen-Synchrotron (DE)) Corporate author(s) CERN. Geneva Series (LHCC Meetings - Open and Closed Sessions) (110 LHCC Meeting AGENDA OPEN Session) Lecture note on 2012-06-13T11:10:00 Subject category LHCC Meetings - Open and Closed Sessions Submitted by morna.robillard@cern.ch cdsweb.cern.ch LHCC Meeting, 13 June 2012
Views: 1
0 ratings
Time: 40:30 More in Science & Technology

… It’s a blooming miracle – a special LHC Report

Wrestling a 27 km superconducting collider under control is not easy. Throw in high intensity beams and it can sometimes seem a continual, frustrating battle with the vagaries of a hugely complex problem space.

 

This problem space has been thoroughly explored over the last three or four years. The myriad of potential obstacles to smooth operation ranges from unidentified falling objects (UFOs), electron clouds, beam dynamics, radiation to electronics, vacuum instabilities, “transparent” software changes, Radio Frequency (RF) trips, electrical network glitches etc. etc. The huge extended systems, such as the beam loss monitors, cryogenics, and quench protection systems, have a phenomenal number of components that inevitably have occasional failures (there is, of course, a higher probability that these occur late Friday evening and over the weekend). On the cryogenics front, cooling and keeping 36,000 tonnes of magnets at 1.9 K is a challenging prerequisite for everything else that follows.

Despite their complexity, we have very well behaved magnets and overall the machine is stable and magnetically reproducible. The magnets are well understood following a long and careful measurement campaign carried out during production. A sophisticated magnet model is even capable of dealing with the once feared dynamic effects. Together with the accuracy and stability of the power converters, our carefully optimized machine stays optimized. The injection, ramp and squeeze have been mastered and, as a general rule, injected beam makes it into collisions.

Exploitation of the LHC’s potential is helped by the presence of excellent beam instrumentation and powerful high-level software architecture. Together with some applied intelligence, these have allowed the development of tools (e.g. measurement and correction of optics, an on-line aperture model) which have opened the way to maximizing the performance of the machine. Most notably, accurate measurements of the aperture in the regions adjacent to the experiments have allowed us to reduce the beam size at the interaction points to unexpectedly low values. The better-than-expected aperture reflects good observance of tolerances during installation and very good alignment of all elements by the survey group.

The LHC has enjoyed from the start very good beam quality (both protons and ions) from the injector complex. The bunch currents have been well above, and the beam sizes well below, the nominal values quoted in the design report. The production of beam in the LINAC, Booster, PS, and SPS is distinctly non-trivial and requires continual care and attention to maintain the beam parameters, however this diligence is reflected directly in delivered luminosity.

Naturally, a cautious approach marked the re-starting in November 2009 following recovery from the 2008 incident. This was most clearly reflected in the choice to run at an initial beam energy of 3.5 TeV. Having experienced first hand the destructiveness of magnetic energy, awareness of the damage potential of the beam to the machine has underpinned the operational approach and marked the subsequent evolution in beam intensity. The full and proper functioning of the extended machine protection system (MPS) has always been an absolute priority.

The MPS consists of a federation of inputs from various systems into a beam interlock system (BIS). When the BIS is triggered it provokes a beam dump within 3 to 4 turns (that is, in a few hundred millionths of a second). The MPS has worked flawlessly, always pulling a beam abort when called upon to do so.

In addition to the MPS, the beam drives a subtle interplay of the beam dump system, the collimation system and protection devices, all of which rely on a well-defined aperture, orbit and optics for guaranteed safe operation. Assuring this throughout high intensity operation remains paramount. Numerous interlocks are in place to ensure that posted limits are always respected.

One notable feature during LHC commissioning and operation is the collective ability of CERN teams to resolve problems. There is in-depth expertise and experience on all systems, including vacuum, collimation, RF, fast kicker magnets and so on. Serious issues, such as radiation to electronics, and the lack of redundancy in protection systems, are targeted rigorously as they become apparent.  

Although precision and rigour are needed when dealing with the tightly synchronized choreography and the ever present dangers of magnetic and beam energy, an open and mostly friendly atmosphere pervades. A recent visitor to an 8:30 meeting noted the lack of defensiveness, and a willingness to directly engage a problem without needing to assign blame. There is amazing dedication from everybody involved. Problems that stop the operation of the machine happen anytime, with a slight preference for nighttime and the weekend. Despite this, there is unfailing support from all teams. Coming out of the technical stop this last weekend the Machine Protection and Electrical Integrity team worked until 5 in the morning on Saturday, and the control and timing teams were in from 2 to gone 6 on Sunday morning dealing with the effects of an innocent leap second.

Finally, trying to hold everything together across the accelerator complex is a talented, smart, moderately good-looking operations team who have necessarily developed an advanced sense of humour.

The LHC came out of a five-day technical stop on the evening of Friday 29 June. For real-time information on the operation of the machine, visit the LHC Page 1 status page.

Dancing to the beat of science

Three Strangels migrating to another dimension came to rest in the CERN Library at lunchtime on Friday 8 June: the first of choreographer-in-residence Gilles Jobin’s artistic interventions.

 

Put a choreographer in a library and strange things start to happen: feet appear from piles of books, heads disappear into bookshelves. But how did these Strangels get there? Though unintrusive, almost invisible movement, guided by gravity and  the fundamental forces that are the subjects of the books in the CERN Library.

If you weren’t able to be there, the Bulletin’s slide show shows you what you missed.

 

Smartphone lost – Privacy gone

Who doesn't own an iPhone, Android or Blackberry mobile phone today? Lucky you if you don’t! In previous issues (Issue 06/07, 2012 and Issue 32/33/34, 2011) we have pointed out their lack of security. But what happens if you lose your smartphone or it gets stolen?

 

Today, a smartphone clones your personality into the digital world. Your phone archives all your emails and messaging communications with your family, friends, peers and colleagues; contains photos and videos of the top moments of your life; holds your favourite music and movies and zillions of other bits of personal information stored in the apps of your choice (like GPS information of your jogging paths, a vault of your passwords, access to your Facebook or Twitter profiles, bank access information, flight and hotel bookings). In the future, your phone might also be used for making payments in shops.

Have you ever thought of how you would feel if you lost your smartphone or it got stolen? Naked? As I now know everything about your friends and your secrets. Ashamed? When I make your private photos public. Embarrassed? As I scoff at your weird taste in music. Helpless? Once I use your SIM card to call my friends in Australia.

There is no silver bullet for mitigation. The most easy prevention is of course disabling unused features and refraining from storing too much information on your smartphone. Back up its contents regularly and purge unnecessary data and photos. Also reduce the retention depth of your local mail box so that older mails get purged automatically. Note that there is a possibility to wipe your mobile phone remotely if it gets lost or stolen*. Finally protect your mobile phone against unauthorised access by locking it with a PIN code or swiping pattern.

And while you are at it: What about your laptop(s)?

For further information, please check our web site or contact us at Computer.Security@cern.ch.

*The CERN Mail Service provides a possibility to wipe your phone remotely. The option is available from the CERN webmail interface and you can get more information here. Note that on recent smartphone devices (iPhone, Android, etc) the “wiping process” can remove all data (pictures, music, applications etc) and restore factory settings.