Shame for IEEE, Springer Verlag, ACM, AIP, WorldScientific, Taylor and Francis, Elsevier

For more than 8 years our blog has identified that IEEE, Springer Verlag, ACM, AIP (American Institute of Physics), WorldScientific (Singapore), Taylor and Francis, Elsevier conferences are fake, bogus, scam, sham, mock and predatory. Now we have additional Proofs:


or google: IEEE 120 SCIgen Papers

The IEEE SCIgen Papers were 85 two years ago:
Several Blogs (included reported this. In 2014, these SCIgen papers in IEEE were 120.

Let''s start with the IEEE SCIGen Fake Papers of 2009. What's happened in 2009:
In 2009, we had received the following email from a girl that was working in IARIA's secretariat.

IEEE Computer Society Press sent it in January 17 (2009) to all the IEEE Sponsored, Co-Sponsored Conferences as well as to conferences
that publish their Proceedings with IEEE CS Press. It is impressive how many IEEE conferences are based on a review on the Abstract!.

John Walz: , Reisman, Sorel" ,,,
date Sat, Jan 17, 2009 at 4:03 AMsubject Confidential: Important CPS Message Regarding Fraudulent Machine-Generated Paper Submissions

TO: CPS Clients FROM: Evan Butterfield, Director of Products and Services RE: Fraudulent Machine-Generated Paper Submissions (CONFIDENTIAL) DATE: 16 January 2009

The IEEE Computer Society (CS) has evidence that multiple (IEEE) conferences are receiving machine-generated papers. In two cases, conferences have actually accepted an obviously fraudulent submission. This is a serious issue that threatens the credibility of your conference, the quality of the digital library, and the reputation of both the IEEE and CS. It requires your immediate attention. Please take this opportunity to ensure that your peer review processes are being followed, and adapt to any new requirements that may be communicated by the IEEE or the Computer Society. No conference published by CPS should rely on an abstract review. It is very important that you review carefully the full text of all papers submitted to your conference. If you have already accepted papers, your program committee should review the full text again. While CPS staff will be conducting random spot-checks of conference papers in the publishing queue, we are relying on you to authenticate the content of your proceedings. Any papers that were not actually presented at your conference need to be brought to our attention, and should receive close review. In known cases, the machine-generated origin is obvious from a reading of the first few paragraphs of the paper; the abstracts are human-generated and do not indicate the quality of the paper itself. In the past, papers have been submitted by “Herbert Schlangemann,” but be mindful that the perpetrator of this fraud will change the approach over time. In the event you discover any evidence of questionable content or behavior, please communicate that to us immediately along with an action plan for addressing the problem. Thank you for your help in maintaining the quality of our products.




A team of scientists compared leading theories of jets produced by rotating supermassive black holes with Chandra data. A sampling of nine giant galaxies that exhibit large disturbances in their gaseous atmospheres showed that the central black holes in these galaxies must be spinning at near their maximum rates.
"We think these monster black holes are spinning close to the limit set by Einstein's theory of relativity, which means that they can drag material around them at close to the speed of light," said Rodrigo Nemmen, a visiting graduate student at Penn State University, and lead author of a paper on the new results presented at American Astronomical Society in Austin, Texas.

The research reinforces other, less direct methods previously used which have indicated that some stellar and supermassive black holes are spinning rapidly.

According to Einstein's theory, a rapidly spinning black hole makes space itself rotate. This effect, coupled with gas spiraling toward the black hole, can produce a rotating, tightly wound vertical tower of magnetic field that flings a large fraction of the inflowing gas away from the vicinity of the black hole in an energetic, high-speed jet.

Computer simulations by other authors have suggested that black holes may acquire their rapid spins when galaxies merge, and through the accretion of gas from their surroundings.

"Extremely fast spin might be very common for large black holes," said co-investigator Richard Bower of Durham University. "This might help us explain the source of these incredible jets that we see stretching for enormous distances across space."

One significant connection consequence of powerful, black-hole jets in galaxies in the centers of galaxy clusters is that they can pump enormous amounts of energy into their environments, and heat the gas around them.

This heating prevents the gas from cooling, and affects the rate at which new stars form, thereby limiting the size of the central galaxy. Understanding the details of this fundamental feedback loop between supermassive black holes and the formation of the most massive galaxies remains an important goal in astrophysics.

Adapted from materials provided by Chandra X-ray Center, via EurekAlert!, a service of AAAS.

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