Friday, December 26, 2014

The IPA Rahul Basu Memorial Award

The IPA Rahul Basu Memorial Award  (2014) for the best thesis in High Energy Physics was presented on 12th December, 2014, at the DAE Symposium held at IIT Guwahati. As mentioned in one of the earlier posts, the two awardees for the 2012-2014 period were Dr. Pratishruti Saha (Univ. of Delhi) for her thesis entitled `Addressing some issues beyond the standard model at Hadron Colliders', and Dr.  Nikhil Karthik (TIFR, Mumbai) for his thesis entitled `Studies on gauge link smearing and their applications to lattice QCD at finite temperature', and two  honourable mentions, Dr.  Ritu Aggarwal (Panjab University) for her thesis entitled `Measurement of High x neutral current ep cross sections and extraction of xF3 structure function using Zeus detector at Hera', and Dr.  Amaresh Jaiswal (TIFR, Mumbai) for his thesis entitled `Formulation of relativistic dissipative fluid dynamics and its applications in heavy-ion collisions'.  The two awardees gave talks on their work during the award ceremony, Dr. Saha, in person, and Dr. Karthik via a Skype connection.

Dr. Saha explained how her work on  direct and indirect searches at various accelerators could be used to identify new physics.  A very well cited paper of her's identifies  how measurements at the Tevatron and the LHC could be used to distinguish between various scenarios which go beyond the Standard Model. Dr. Saha and co-workers had  considered how top polarisation could be used to distinguish between various scenarios, which had been used to explain asymmetries in the top quark production process. The work also had relevance to observations at the Large Hadron Collider.  Her thesis focused on the fact that the top quark occupies a special place in the standard model, and hence, the analysis of its behaviour can have important implications in scenarios which attempt to go beyond the Standard model, in various sectors like the Higgs sector.  She had also analysed the behaviour of the bottom quark and its contribution to resonances.

Dr. Nikhil Karthik spoke about the work in his thesis, which contributes to important technical advances in  lattice QCD, and also studies its deconfined phase. Although the coupling constant in this  phase is not too large, perturbative estimates of quantities like the viscosity and the screening mass do not agree with expectations due to discretization effects. Specifically, existing lattice studies based on the staggered discretization of quarks, found a screening mass which, contrary to expectations is smaller than that of the free field theory. Smoothed gauge configurations are the prescription to ameliorate such unwanted discretization effects. Dr. Karthik's thesis investigated the effects of different types of smoothing, and devised an optimum smoothing strategy which succeeded in   identifying the reasons why the screening mass shows the observed behaviour.  Dr. Karthik's talk was also notable due to the clarity with which technical issues were conveyed to the audience.

The award ceremony was well attended, with many students and many well known physicists in the audience. It was heartwarming that three of these were  Rahul's friends in graduate school,  Prof. Rohini Godbole, Prof. Ashoke Sen, and Prof. Sunil Mukhi, distinguished physicists, and in the case of Profs. Mukhi and Godbole, members of the award committee. We congratulate the winners, and wish them all success in their future endeavours.

This blog post is by Neelima  Gupte and Sumathi Rao. 

Wednesday, December 17, 2014

For the children

For the children of Peshawar

Rest in Peace.

This blog post by Neelima Gupte and Sumathi Rao.

Wednesday, November 26, 2014


But what about the unsung one?
The companion to the great hero,
does he not deserve praise?
Destiny may not have chosen him,
Fate must have overlooked him,
but he still fought the great evil,
slayed the vile demon.

Nothing can be done alone,
too often is this forgotten.
The focus is put on one,
who did not choose,
but was chosen.
What about the other,
the one that did choose?

He chose to risk everything.
There was nothing great at work,
forcing him to choose.
It was a simple,
yet immense, decision.

Sometimes the greater heros are not the destined ones,
they are the ones that stood by the heros,
by the choice they made,
never regretting it,
only pushing forward to the goal.
Never  overlook  the companions,
for something important will be missed,
that may be lost forever.

-James Anderson ,   'To the unsung hero'.

For  Tukaram Ombale and the other ordinary citizens of Mumbai who did far more than their duty on 26/11.

This blog post is by Neelima Gupte and Sumathi Rao.

Thursday, November 20, 2014

The IPA Rahul Basu Memorial Award (2014)

The winners of the Rahul Basu Memorial Award (2014) for the best thesis  in high energy physics have been announced.

The winners are

1. Pratishruti Saha (Univ. of Delhi) for her thesis entitled

Addressing some issues beyond the standard model at Hadron Colliders

2. Nikhil Karthik (TIFR Mumbai) for his thesis entitled.

Studies on gauge link smearing and their applications to lattice QCD at finite temperature.

The following theses have received Honourable Mention

1. Ritu Aggarwal (Panjab University) for her thesis entitled

Measurement of High x neutral current ep cross sections and extraction of xF3 structure function using Zeus detector at Hera

2. Amaresh Jaiswal (TIFR, Mumbai) for his thesis entitled

Formulation of relativistic dissipative fluid dynamics and its applications in heavy-ion collisions

Congratulations to all winners. The awards will be presented at the next DAE Symposium on High-Energy Physics, being held in Guwahati from December 8-12, 2014. The award ceremony has been scheduled on December 12th from 4-5:30 PM. Dr. Saha and Dr. Karthik will present talks on their theses and receive a cash award, and Drs. Aggarwal and Jaiswal will be presented with citations.

The  Award committee members were Sunanda Bannerjee, Rohini Godbole, Sourendu Gupta, Neelima Gupte, Bedanga Mohanty, and Sunil Mukhi. The award is administered by the Indian Physics Association.

This blog post is by Neelima Gupte and Sumathi Rao.

A short report of the award ceremony can be found in the post on 26/12/2014.

Saturday, November 8, 2014

Who owns India?

After the idea of India has been debated endlessly for years, here comes a new debate: Who owns India? This provocative question was posed by Gopalkrishna Gandhi in his public lecture under the Indian Academy of Sciences auspices  at IIT Madras yesterday.

It appeared that the real question posed was not who owns India, but who thinks they own India. This question can have many answers, some of which were proposed by the speaker in his talk, using the north/south paradigm. These started with the geographic north of India  which has always imposed it's political hegemony on the south. While the presidentship of India has rested many times with those from the south, although C. Rajagopalachari, one the speaker's two distinguished grandfathers,  had to yield his claim to the first presidentship to Dr. Rajendra Prasad, the north's claims to the prime ministership, the executive headship of the nation,  have been consistent, with P. V. Narasimha Rao and K. Deve Gowda having been the two exceptions.  The other exception to the rule, has been Kamaraj's astute stewardship of the country during the crucial transitions after the sad demises of Nehru and Shastri, one after the other. The north has also always  been vocal about it's cultural presumptions and lack of knowledge about the south, especially that of the quite major distinctions between southern states. The south has been philosophical about these assumptions, which arise from the more basic assumption of ownership.

However, the geographic north and south are not the only north south divide! There's the techno-economic north and south divide as well. This north south divide exists both between nations and within nations, with the north's paternalistic assumption that the protection of it's own interests also contributes to the 'development' of  the south, being remarkable for its convenience, and for the justification of its actions. A similar divide also exists between genders. It is not even necessary to state which is north here!

The speaker ended with a specific request to the academies. It's necessary to know who owns India (the people of India, it is clear). It is also necessary to know what India owns. The huge resources of India are well documented, especially by the Surveys of India, starting from the Survey of India from 1757, to the Geological Survey of India  also started circa 1857, the Botanical and Zoological Surveys of India, and others.  It would be well if the scientific academies took advantage of this knowledge, to opine on how this wealth could be used to maximally benefit its owners, the people.  This  request was an eye-opener, and we hope it will chart a direction for our scientific bodies.

This blog post is by Neelima Gupte and Sumathi Rao.

Wednesday, September 24, 2014

MoM's made it to Mars

(A view from the ground. Curiosity Rover picture  (NASA via Scientific American))

First map of Mars,  Giovanni Schiaparelli,  (1888)
The Mangalyaan has safely made it to the Mars orbit, dead on time and with no glitches. We join the nation and PM Modi, (natty in a red Nehru jacket),  in congratulating the ISRO scientists on  success in a difficult mission. We take particular pride in the number of women we saw in the mission control room (on our TV screens, of course!). It was a good start to Wednesday morning, which has now become the Mangalvaar.

More soon, it is a working day after all. In any case ISRO has said it all on it's twitter page  here, an admirable job by their PR team, in publicising the sterling work done by their scientists.

This blog post by Neelima Gupte and Sumathi Rao.

First pic here.

One more.

Dust storm!

A 3-d picture.



Mountains and valleys.

The photo top left shows Elysium, the largest volcanic region of Mars, the bottom right shows the mountains and canyons, Mount Olympus, no less.

MoM's quite the chatterbox, and has lots of friends up there (Five orbiters, two rovers  and a flyby, hope we counted everyone).
They are not all as talkative!

06/03/2015. Crater of Arsia Mons (L) Valles Marineris Canyon (R)

Sunday, September 14, 2014

Mind Games

The technique of optogenetic generation of memories has already been
demonstrated for `incepting' false memories in mice by neuroscientists in the MIT lab of neuroscience. See here for details.  It has now been demonstrated that this technique can be used to erase traumatic memories, in mice again, of course!

In the optogenetic technique, neurons are labelled with a light sensitive protein, and pulses of light are used to switch the neurons on and off.The patterns of neurons activated with negative memories, e.g. when the lab mice received an electric shock (mild, the researchers take care to aver) were identified and tagged with the light sensitive protein, and so were the patterns when positive memories were formed (the mice were allowed to play with lady mice).

Later, the mice were put in an enclosure, and the natural preference of the mice for any preferred area of the enclosure was observed. Next, if the negative memories of the mice were activated when they went to the preferred area, they avoided the preferred area, and if the positive memories were excited when they went to the less preferred area, they started spending more time in the less preferred area.

When mice that had been shocked were put with females and the negative memory was activated, the pattern or em-gram of the negative memory became less strong. Conversely, electric shocks were given to mice with positive memories excited, the positive memories also became weaker. Now, if the mice were put in the enclosure again, the fear conditioned mice started spending more time in the area they had avoided earlier, and the reward conditioned mice did the opposite, indicating that both kinds of memories had been reversed.

Memory erasure via association of location, has been long used in psychiatry. Similar effects can be induced by drugs, and fear and reward conditioning of behaviour has been known since Pavlovian times. However, here the memory erasure was achieved by optic simulation of a pattern (an em-gram) stored in a specific area of the brain. As in the `inception' of memories, this also identifies  the neural circuits and the physical location of the area in the brain where specific memories are formed. An important finding in the present case was that when the negative memories were labelled and activated in the dentate gyrus, an area of the hippocampus, which forms new memories, and records
factual details of experiences,  the memories could be erased, or made less negative. On the other hand, the strength of negative memories labelled and activated  in the basolateral complex of the amygdala (which links emotion to memories)  could not be reduced.

While transferring the technique to humans is a long way off, the method also holds promise for the post-traumatic treatment of stress disorders. As in the case of the inception of false memories, similar results can be invoked by chemical means. This may constitute a more practical method of treatment. However the identification of the hard wired circuitry of the brain and the identification of the specific neuronal patterns (em-grams) associated with specific memories constitute the real strength of the optogenetic methods.

This blog post by Neelima Gupte and Sumathi Rao.

Friday, August 22, 2014

Nāḷ nalvāḻttukkaḷ

நாள் நல்வாழ்த்துக்கள்

Everybody is saying it, so why not us? Many happy returns of the day, Madras. Today, August 22nd marks the 375th return of the day in 1679 when Francis Day and Andrew Cogan leased the villages of Chennaipattinam and Madraspattinam from the Nayakar representatives of the Vijaynagar empire (notwithstanding disputes about the date).  Many festivities are in progress, spearheaded by the Hindu, the Mahavishnu of Mount Road, no less. They have a lovely and historic set of Chennai photographs here. Less lovely is the Madras song (fluff isn't the strong point of the Hindu!). However, do have a look. Maybe you will like it. 

More on the topic, by and by.

This blog post is by Neelima Gupte and Sumathi Rao.

Tuesday, August 12, 2014

By the blue sea

Last month came a trip out of the blue and into the blue.  The location was the place where the blue of the sky mixes seamlessly into the blue of the sea, viz. the Greek island of Rhodes. The blue of the sea has to be seen to believed.  Turquoise and azure mix within 20 feet of the shore and darken into indigo. Beyond the horizon looms a grey blue shadow, the shore of Turkey.

For all Turkey is so near, the Turks and the Greeks share a complicated relationship, from medieval times to modern times. Rhodes was home to the Knights Hospitaller, who left behind a fortified enclave, and a harbour. The island boasts several places of worship, which have maintained their function, but alternated denominations during its chequered past. The  hostility lurks underneath the surface, even to this day! The Knights Hospitaller left behind the medieval portion of the town, which is a World Heritage site, with fortifications, the Palace of the Grand Master,  mosaics of the nine Muses, medieval streets (with markets selling modern bric-a-brac) and a quaint harbour.

Antiquity is a little far away. The famed Colossus succumbed to an earthquake in 226 BC, and its fragments lay around for nearly 800 years, until they were sold as scrap. The remnants of antiquity on the island   can be found in the broken pillars of the Acropolis at Rhodes, to which we could not make it, alas! As for modern times, they are embodied by cheerful teenagers enjoying the pristine beaches. They do seem to get a tad drunk and noisy at night, but they are on holiday, after all! The Aegean idyll was sandwiched between, the new international airport at Mumbai, (the White Peacock is indeed beautiful, may it last) , and Air India preening itself at Frankfurt, on having finally made it to the Star Alliance (long may that last too!). Altogether, it was a wonderful week, out of the hot summer in India, and the conference was pretty good too. Here's to the next time!

This blog post by Neelima Gupte and Sumathi Rao.

Wednesday, June 25, 2014

Bicep flexing 2 : After the dust up

This week saw the actual publication of the BICEP2 result on the detection and analysis of the polarisation signature of inflationary behaviour on the cosmic wave background in the final arbiter of all physics research, Physical Review Letters. The paper does an admirable job of explaining  the problem, its background, the data, the analysis, the results and the limitations, if not to the lay reader (not the purpose of PRL, anyway), at least to physicists in other fields. Here is a short summary of what it says.

First, the background. The central paradigm for the origin and evolution of the universe, is the Big Bang Theory, first proposed by Alpher, Bethe and Gamow. The validity of the Big Bang theory was established by the discovery of the cosmic microwave background by Penzias and Wilson. One of the most fruitful areas of research in recent times has been the observation of the anisotropies in the cosmic microwave background, and the consequent refinement of the cosmological models. The `standard model' of cosmology is known as `Lambda-CDM' model, where the Lambda refers to the cosmological constant and CDM stands for `cold, dark, matter'.  This model can account for observed properties like the existence and structure of the cosmic microwave background, the large scale structure in the distribution of galaxies, the abundances of gases like hydrogen, helium and lithium, and the accelerating expansion of the universe. It is particularly important to point out that cosmic microwave background measurements now have precision over angular scales ranging from the whole sky to arcminutes. As a result, the parameters of the Lambda-CBM model are constrained to a precision of less than 1 %.

Inflationary scenarios, including the first one proposed by Alan Guth,  extend the model above by adding an early period wherein a metastable state corresponding to a local minimum of the potential energy undergoes  nearly exponential expansion, which leads to the subsequent big bang.
The addition of inflation to the early scenario explains features like the flatness and isotropy, which cannot be explained within the standard framework above. Inflation also explains that the Universe's primordial perturbations  originate in quantum fluctuations stretched by this exponential expansion, which invokes quantum effects in curved space time at energy and time scales of the order of 10^16 GeV and 10^(-32) seconds, which are completely inaccessible in the real world, both in nature and the laboratory. It is therefore important to have a direct and clear test of this theory. The BICEP2 experiment provides such a test, and therein lies its importance.

 The signature is as follows. While a number of inflationary scenarios exist, they all have a common prediction. Inflation would have produced gravitational waves that would cause characteristic distortions in the cosmic microwave background, with a unique  signature in the radiation field.  The quadrupole nature of the  gravitational waves lead to a polarisation in the radiation field with the `B-mode' pattern characteristic of a curl on angular scales of the order of a degree. Such a pattern cannot be produced by density fluctuations which produce a  `E-mode' pattern characteristic of a gradient on smaller angular scales. It is the `B-mode' pattern seen at exactly the expected angular scales in the BICEP2 experiment that provides the unique signature of inflation. The ratio of the amplitude of the tensor perturbations  characteristic of gravitational waves, to the scalar modes associated with density perturbations, is used to identify the strength of the B-mode, and also to predict the energy density during the inflationary phase.

Since the `B-mode' pattern provides the signature of inflation, it is important to eliminate the effect of foreground sources  which can produce such a pattern. One of these is the effect of gravitational lensing. However, this is much weaker than the effect seen in the BICEP2 experiment. Hence this effect has been ruled out. One serious objection raised since the results were announced, is that such a pattern could be due to the impact of the galaxy's dust. Unfortunately, there is no convincing data on the distribution of dust. Hence the BICEP2 analysis has estimated the effects of cosmic dust based on theoretical models, and concluded that dust could not reproduce the magnitude of the observed signal. However,the validity of this conclusion depends on the accuracy of  hitherto experimentally unvalidated theoretical models. Critics of the BICEP2 result claim that the new data released by the PLANCK satellite is not incompatible with dust levels that lead to polarisation signatures  which are of the order of the BICEP2 signal. A number of measurements that are scheduled within the coming year are expected to resolve this ambiguity.

The BICEP2 experiment also leads to a variety of exciting theoretical implications. More on these can be read here. For the present, there is no doubt that the BICEP2 experiment constitutes an important landmark in understanding the mechanisms that lead to the formation of the universe and its subsequent evolution. We look forward to its further validation.

This blog post is by Neelima Gupte and Sumathi Rao.
Here is the outlook    after the latest analysis of the Planck data. The BICEP2 result begins to look dusty. More later.

Monday, April 28, 2014

The sacred and the secular

Last week was a combination of the sacred and the secular. First, the sacred. The sacred was multidenominational: viz. the dargah of Shaikh Moinuddin Chisti at Ajmer, and the Bramha temple at Pushkar. The dargah was complete with marble jalis and floors, chadars made of roses, threads to ask for wishes, and qawwals singing Sufi qawwalis. The mood was cheerful, and the atmosphere about half way between a  fair ground and Friday prayers. Pushkar was even more cheerful, the only sour note being Savitri Devi, Brahma's wife, sulking away in a temple on the hill side thanks to having been displaced at Brahma's side by a milkmaid named Gayatri Devi (to say nothing of an eponymous Maharani ruling the roost for many years in nearby Jaipur).

Speaking of sulking, the secular provided solid reasons for sulking,  the secular being the current Lok Sabha elections, and the reasons for sulking being bounced off the voter list for the sixth time despite filling Form Six, those self same six times! The cheerful polling officers at the polling booth pored over the list three times (six by two, get it?) and said sorry madam, name missing, thereby putting paid to hopes of recurrence of  the miracle that had happened six years ago (that of name being found on the supplementary list).    There was another six by two piece of numerology for those who made it to the polling booth. There were three electronic voting machines in the booth, thanks to forty two (six into seven, what else?) candidates being in the fray in Chennai South parliamentary constituency.  Hopefully, the elected candidate, whoever it be, will fulfil the fervent mannat made at the dargah and the tirth (oh, please, please, please, finally fix Taramani Link Road), and another trip to Ajmer and Pushkar can be made, this time complete with chadar and coconut. The next wish will be to be put back
on the voter list (at least for the duration of the municipal elections)!

This blog post by Neelima Gupte and Sumathi Rao.

Monday, March 24, 2014

Inflation flexes its biceps

Last week saw the announcement of a major discovery in Physics. Researchers at the Harvard Smithsonian Center for Astrophysics announced the discovery of the signature of gravitational waves in studies of the polarisation of the cosmic wave background data registered at the  Background Imaging of Cosmic Extragalactic Polarization 2 (Bicep2) experiment at the South Pole. The observations are also consist with scenarios called `inflation', which postulate that the universe underwent rapid expansion shortly after its creation in the big bang. The scenario goes as follows: gravitational waves are created due to quantum fluctuations in the structure of space time, right after the big bang. These were magnified to observable levels due to the rapid expansion that occurred during the inflationary epoch and imposed their signature on the cosmic microwave background in the form of a characteristic polarisation pattern. The BICEP2 experiment observed a distinctive twisting pattern called a curl or B-mode in the polarisation of the cosmic microwave background. Such a pattern had been observed before due to the effect of gravitational lensing (a warping of light due to the presence of nearby massive objects) but  this effect has been ruled out here. Measurements also indicate that the contribution of the gravitational waves to the signal is quite large compared to the contributions of the density fluctuations, increasing confidence in the reliability of the discovery. However, the cautious look forward to support of this discovery from other experiments, such as those carried out by the Planck satellite.

The excitement generated by the discovery is comparable to the excitement generated by the discovery of the cosmic microwave background by Penzias and Wilson, even though indirect evidence of gravitational waves has been obtained before in measurements from pulsars, and even resulted in the 1993 Nobel prize. This discovery supports the inflationary models of cosmology first proposed in the 1980-s by Alan Guth, Linde and others, and further analysis of the data may be able to support some inflationary models, and rule out others, and will keep astronomers and cosmologists busy and happy for several years!

This blog post is by Neelima Gupte and Sumathi Rao.

Wednesday, March 5, 2014

Rahul Basu (04/03/1956-05/03/2011)

Each day since we first lost you
Life is not the same,
Each day we search for reasons
Each day we call your name.

But each day we're reminded
Of the joy that you would bring,
Each day we still remember
How you brightened everything.

So each day we live on
We will never be apart,
For in each day that passes
You're forever in our hearts.

Graham Allaway

This blog post is by Neelima Gupte and Sumathi Rao.


Wednesday, February 19, 2014

No hanging, this time!

The Supreme Court, in a landmark judgement yesterday, commuted the death sentences of Rajiv Gandhi's assassins, Murugan, Santhan and Periavelan to life imprisonment. The reason cited was the inordinate delay of 11 years, in giving a decision on their mercy petitions.  The Chief Justice said "...delay violates the requirement of a fair, just and reasonable procedure. Regardless and independent of the suffering it causes, delay makes the process of execution of death sentence unfair, unreasonable, arbitrary and capricious and thereby, violates procedural due process guaranteed under Article 21 of the Constitution and the dehumanizing effect is presumed in such cases." This decision was expected after the earlier Supreme Court decision on, January 21st, commuting the death penalty of 15 prisoners, citing the same reason, viz., the inordinate delay in a decision on their mercy petitions. Both these decisions have been hailed as a victory by the opponents of the death penalty. However,unlike the beneficiaries of the January 21st decision, the nature of the crime, i.e. the political assassination of a popular leader, and a former prime minister, as well as the fact that the assasination was a plot by the LTTE,  have led to polarised and highly charged opinions on both sides in the present case. In Tamil Nadu, longstanding sympathy for Srilankan Tamils, as well as the age of the assassins at the time of the crime, (two were 19 and one 24),  and their model conduct in prison, have led to jubilation at the verdict. Others find this a little mystifying.

A further layer has been added by  today's decision by the Tamil Nadu government of Jayalalitha, a known foe of the LTTE, to let the death row convicts as well as others who have been awarded life imprisonment  in the same case, walk free. A plus point in this, could be the reunion of families, some of whom have never accepted that their kin were involved in the conspiracy, and others who argued that they were bit players, the principal culprits being already dead. (The actual assassin, Dhanu, died in the suicide attack,  and her handler, the  One eyed Jack, Sivarasan, committed suicide by consuming the famed LTTE cyanide tablets when the police closed in on the conspirators in a rented house in Bangalore 22 years ago.) A particularly sad case is that of Harithra, the daughter of Nalini and Murugan, who has never seen her parents outside jail. However, even if the central government accepts the freeing of the convicts, life outside jail may still turn out to be rough for the releasees. Whatever the rights and wrongs of this case, it will be good if the right lessons are extended to other cases, like that of Afzhal Guru, where political considerations justified a hanging, that was  not warranted by the facts of the case.

This blog post is by Neelima Gupte and Sumathi Rao.