Friday, 27 March 2015

Have alien civilizations built cosmic accelerators from black holes?

Have alien civilizations built cosmic accelerators from black holes?

Has an advanced alien civilization built a black-hole-powered particle accelerator to study physics at "Planck-scale" energies? And if such a cosmic collider is lurking in a corner of the universe, could we detect it here on Earth?
Brian Lacki of the Institute for Advanced Studies in Princeton, New Jersey, has done calculations that suggest that if such an accelerator exists, it would produce yotta electron-volt (YeV or 1024 eV) neutrinos that could be detected here on Earth. As a result, Lacki is calling on astronomers involved in the search for extraterrestrial intelligence (SETI) to look for these ultra-high-energy particles. This is supported by SETI expert Paul Davies of Arizona State University, who believes that the search should be expanded beyond the traditional telescope searches.
The nightmare of particle physics is the dream of astronomers searching for extraterrestrials
Brian Lacki, Institute for Advanced Studies
Like humanity, it seems reasonable to assume that an advanced alien civilization would have a keen interest in physics, and would build particle accelerators that reach increasingly higher energies. This energy escalation could be the result of the "nightmare scenario" of particle physics in which there is no new physics at energies between the TeV energies of the Standard Model and the 1028 eV Planck energy (10 XeV) – where the quantum effects of gravity become strong. "The nightmare of particle physics is the dream of astronomers searching for extraterrestrials," says Lacki.
An important problem facing alien physicists would be that the density of electromagnetic energy needed to reach the Planck scale is so great that the device would be in danger of collapsing into a black hole of its own making. However, Lacki points out that a clever designer could, in principle, get round this problem and "reaching [the] Planck energy is technically allowed, if extremely difficult".
Not surprisingly, such an accelerator would have to be rather large. Lacki believes that if electric fields are used for acceleration, the device would have to be at least 10 times the radius of the Sun. However, a magnetic synchrotron-type accelerator could be somewhat smaller. As for what materials could be used to make the accelerator, Lacki says that normal materials could not withstand the strong electromagnetic fields. Indeed, one of the few places where such a high energy density could exist is in the vicinity of a black hole, which he argues could be harnessed to create a Planck-scale accelerator.

"Vast amounts of pollution"

Colliding particles at tens of XeVs is only half the battle, however. Lacki calculates that the vast majority of collisions in such a cosmic collider would be of no interest to alien researchers. To get useful information about Planck-scale physics, he reckons that the total collision rate in the accelerator would have to be about 1024 times that of the Large Hadron Collider. "As such, accelerators built to detect Planck events are extremely wasteful and produce vast amounts of 'pollution'," explains Lacki.
While much of this pollution would be extremely high-energy particles, that in principle could reach Earth, it is unclear whether they could escape the intense electromagnetic fields within the collider. Furthermore, like colliders here on Earth, the builders of a cosmic machine would probably try to shield the surrounding region from damaging radiation. Indeed, Lacki's analysis suggests that neutrinos are the only particles that are likely to reach Earth.
These neutrinos would have energies that are a billion or more times greater than the highest energy neutrinos ever detected here on Earth. However, unlike their lower-energy counterparts, these accelerator neutrinos would be much easier to detect because they interact much more strongly with matter. Lacki calculates that the majority of such neutrinos passing through the Earth's oceans will deposit their energy in the form of a shower of secondary particles. While the oceans are far too murky for physicists to detect the light given off by the showers, Lacki reckons that the sound of a shower could be detected by a network of hydrophones in the water. However, because these neutrinos are expected to be extremely rare, he calculates that about 100,000 hydrophones would be needed to have a chance of detecting the neutrinos.

Whole of the Moon

Another possibility, albeit less sensitive, is to use the Moon as a neutrino detector. Indeed, the NuMoon experiment is currently using a ground-based radio telescope to try to detect showers created when 1020 eV neutrinos smash into the lunar surface.
While the detection of YeV neutrinos would not be proof that an alien accelerator exists – some theories suggest that they could be produced naturally by the decay of a cosmic strings – Lacki says that spotting such high-energy particles would be an important breakthrough in physics.
While Davies is keen to expand SETI, he does identify one important drawback of looking for cosmic colliders. "My main problem is that once the [alien] experiments are done, there would be no need to keep the thing running, so unless there are mega-machines like this popping up all over the place, there would be only transient pulses," he told physicsworld.com.
Davies believes that it is very difficult for humans today to understand why an advanced civilization would want to build a Planck-scale collider. "Why do it? Perhaps to create a baby universe or some other exotic space–time sculpture," he speculates. "Why do that? Perhaps because this hypothetical civilization feels it faces a threat of cosmic dimensions. What might that threat be? I have no idea! However, a civilization that knows a million times more than humanity might perceive all sorts of threats of which we are blissfully unaware."
Lacki's calculations are described in a preprint on arXiv.
  • Paul Davies has written a feature article for Physics World about SETI called "The Eerie Silence"

New US philanthropy group picks physicist as boss

New US philanthropy group picks physicist as boss

Marc Kastner, a physicist at the Massachusetts Institute of Technology (MIT), has become the first president of the Science Philanthropy Alliance (SPA) – a new grouping of six organizations aiming to increase private funding for fundamental research in the US. Kastner began the appointment earlier this week, having taken a leave of absence from MIT.
The alliance – composed of the Howard Hughes Medical Institute, the Kavli Foundation, the Gordon and Betty Moore Foundation, theResearch Corporation for Science Advancement, the Alfred P Sloan Foundation and the Simons Foundation – formed two years ago. The alliance's goal is to increase the value of philanthropic funding to fundamental research – currently estimated at about $2bn – by another $1bn within five years.
The SPA was created following concern that funding for basic research has dwindled in the US, with R&D funding at its lowest level – as a percentage of the federal budget – since the 1960s Apollo era. In addition, funding has shifted towards applied research, which Kastner feels neglects the importance of basic science. "We know historically that some of the greatest breakthroughs in technology have come about in that kind of discovery-driven research," he says, pointing out that the creation of the Global Positioning System in 1995 evolved from fundamental research carried out several decades earlier.

Funding research

Kastner says that although private funding cannot make up the losses suffered from decreased government support, philanthropists are still in a position to make a big difference. To do this, he says that the alliance needs to show potential donors why fundamental research is important, as well as the technologies that can result from such research. "I think people forget about this," says Kastner. "They see that you can write software and do wonderful things with computers, and they forget that this came out of decades of fundamental research."
Kastner adds that the alliance will also "put in front of potential philanthropists ideas of how they could really make a difference and the satisfaction they could get out of it". The alliance supports around 16 universities – and will soon add non-profit research laboratories and more universities – that share the same goals of increasing levels of fundamental research and have created funds to do so.

Key experience

Kastner has experience of securing philanthropic funding, having done so in his role as head of MIT's physics department, a position he held for nine years. In November 2013 US president Barack Obama nominated him to head the Department of Energy's Office of Science, which manages much of the nation's basic-science research, but his appointment stalled in Congress last year with the position yet to be filled.

UK unveils national strategy for stimulating growth in quantum technologies

UK unveils national strategy for stimulating growth in quantum technologies

The UK has released a national strategy to stimulate growth in quantum technologies. Announced last month by the Quantum Technologies Strategic Advisory Board (QTSAB), the plan outlines five actions that, if implemented, would allow the UK to capitalize on the country's R&D in quantum technology. The QTSAB is chaired byDavid Delpy, a former head of the UK's Engineering and Physical Sciences Research Council (EPSRC), and has 12 members from UK industry and academia.
The first action, which was already announced late last year, is the establishment of a national network of technology hubs that involve 17 universities and more than 50 industry partners. So far, £120m has been promised to the hubs from the UK government with an additional £60m from industrial partners. The hubs are part of the £270m National Quantum Technology Programme, which is overseen by the QTSAB, that was established in 2013 to encourage the growth of industries based on technologies such as quantum encryption and quantum metrology.

Demonstrating commercial products

The second action involves stimulating the development of commercial applications and markets for quantum technologies. This will be done by providing public funds to build "demonstrators" of potential commercial products, and through the creation of a roadmap for the future development of quantum technologies. "Quantum technologies stand to offer industry truly revolutionary capabilities in key areas," says Trevor Cross, chief technology officer at e2v, a UK firm that develops RF power, imaging and semiconductor technologies, and is involved with the National Quantum Technology Programme. According to Delpy, a related goal is the development of quantum components that can be integrated into new products by a "competent engineer", rather than a highly specialized quantum physicist.
Another action identified by the board is the need to grow a workforce that is skilled in the development of quantum technologies. To achieve this goal, £15m of the £270m will be devoted to training the next generation of quantum engineers through the funding of PhD students by ESPRC. "Quantum skills will allow us to bring game-changing advantages to future timing, sensing and navigation capabilities, in a sector that could be worth more than £1bn to the UK economy," says Greg Clark, who is the UK's universities, science and cities minister.
The QTSAB also says that the UK quantum-technology community should undertake an "early and broad engagement with UK society" to ensure that the industry grows in a responsible manner with the creation of effective regulatory and standard regimes.

Balancing international collaboration

The fifth and final action is to maximize the benefit to the UK through international collaboration. The QTSAB warns that several other countries have already established centres of excellence for quantum technologies, and that UK researchers and businesses need to strike a balance between international collaboration and supporting the development of home-grown research and development efforts.
Cross told physicsworld.com that e2v is particularly interested in the commercial development of quantum-metrology technologies that fit in with the firm's expertise in vacuum technology. He says that sensors based on ultracold atoms, for example, could be used in a range of applications from navigation systems that do not rely on GPS satellites to gravimeters used by civil engineers for detecting underground features such a potential sinkholes along a stretch of road. He believes that demonstrators of these products will be available in two to three years, and that specialized products could be on the market in five years.

ndia-based Neutrino Observatory faces a new hurdle

ndia-based Neutrino Observatory faces a new hurdle

Just months after receiving the green light from the Indian government, the India-based Neutrino Observatory (INO) has been dealt a blow after a court writ was filed against the facility's new site by local environmentalists and politicians. The writ, filed in a state court and the National Green Tribunal, alleges that the site is in a seismic and highly biodiverse area, and that tunnelling required for the project could affect nearby aquifers.
Originally scheduled to be complete in 2012, the INO finally received the go-ahead in January this year when it received Rs 15bn ($236m) towards construction inside a mountain near Pottipuram – 110 km from the temple town of Madurai in the southern state of Tamil Nadu. Pottipuram was selected after environmentalists protested in 2010 that the original choice – Singara village in Tamil Nadu – was near an elephant corridor. The INO is to be built some 1.3 km beneath the mountain peak, accessible via a 2 km-long tunnel. The lab will comprise three caverns – the largest, being 132 m long, 26 m wide and 30 m high, will house the 50,000 tonne Iron Calorimeter neutrino detector.
Physicists in India say that the absence of such a facility deprives them of hands-on experience in experimental particle physics – a continuing weak point for the community. Scientists are now dismayed by the new writ, which is being heard at the Madurai bench of the High Court. "The site is a wasteland, a barren land," says INO project director Naba Mondal of the Tata Institute of Fundamental Research in Mumbai. "We were not going to occupy a forest land or one with good vegetation." That view is backed by a 2011 report from the ministry of environment and forests, which states that the forest clearance would be "notional" as "no forest land is expected to be occupied, since both the tunnels and laboratories are underground".

"Unnecessary panic"

Mondal adds that the writ is taking valuable energy and time away from getting the project going. "Such petitions create a kind of question mark in the minds of people who do not understand physics, an unnecessary panic that is not warranted," he says.
Thiagarajan Jayaraman of the Tata Institute of Social Sciences Mumbai disputes the claims in the petition, saying that the tunnelling zone for the observatory is a "charnockite" zone – one that contains feldspar and quartz rocks – with no groundwater. Indeed, a study carried out by the Geological Survey of India (GSI) last year concluded that there was no abnormal threat of groundwater getting into the access tunnel as well as the cavern area. This, combined with the fact that no habitation or water wells exist in the proposed site, suggests, according to the GSI, that there is little danger of the groundwater regime being disturbed by the proposed tunnelling.
However, V T Padmanabhan, chairman of the Society of Science Environment and Ethics – a non-governmental organization – based in Thrissur, Kerala, told physicsworld.com that the project is close to the border with Kerala, which is rich in biodiversity and groundwater sources.