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Journal articles on the topic 'Glitching'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Shew, Ashley. "Glitching Out." American Scientist 111, no. 4 (2023): 248. http://dx.doi.org/10.1511/2023.111.4.248.

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2

Hammana, Zouhair, and Victoria Louisa Klinkert. "Glitching the University Machine." Teaching Anthropology 10, no. 4 (2021): 36–46. http://dx.doi.org/10.22582/ta.v10i4.621.

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In this piece we explore how to return anthropological study to common use by way of Hilal and Petti’s (2019) use of al masha - a cultivation and reactivation of the commons. In doing so we recognise that our point of departure is one of colonial permanence, as anthropological study is tied to the discipline and its colonial disciplining, which in turn is tied to the University Machine and its infrastructure. In enacting colonial permanence and holding up its decolonial facade it is the sociality of the infrastructure that we have chosen to focus on. We argue that it is in moments of refusal t

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3

Thwaites, Denise. "Incorruptible." Axon: Creative Explorations 14, no. 1 (2024): 1–13. http://dx.doi.org/10.54375/001/nmbj91qgz1.

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Corrupted, cherry-picked, and compromised; three derogatory terms used to describe permutations in knowledge across disciplinary boundaries. Yet some of the 20th century’s most lauded ‘incorruptible’ French thinkers, Derrida, Deleuze and Foucault, were celebrated for their disobedient interlacing of concepts from biology, mathematics, linguistics, and literature. How might we approach corruption, not as a failing, but a hallmark of knowledge transformation? This hybrid essay engages with the visual and linguistic poetics of much translated French thinkers, Cixous, Derrida, Foucault, Deleuze an

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4

Melatos, A., J. A. Douglass, and T. P. Simula. "PERSISTENT GRAVITATIONAL RADIATION FROM GLITCHING PULSARS." Astrophysical Journal 807, no. 2 (2015): 132. http://dx.doi.org/10.1088/0004-637x/807/2/132.

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5

Braun, T. "Trans Glitching in Social Virtual Reality." Canadian Theatre Review 202 (May 1, 2025): 42–48. https://doi.org/10.3138/ctr.202.006.

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6

Shabanova, T. V., and J. O. Urama. "Glitch Behavior of the Pulsar B1822–09 in the Range 0.1–2.3 GHz." International Astronomical Union Colloquium 177 (2000): 107–8. http://dx.doi.org/10.1017/s0252921100059182.

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AbstractResults of timing observations of the glitching pulsar B1822–09 made practically simultaneously at widely separated frequencies of 0.1 and 1.6/2.3 GHz during seven years since 1991 to 1998 are discussed.

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7

Askeland, Amund, Svetla Nikova, and Ventzislav Nikov. "Who Watches the Watchers: Attacking Glitch Detection Circuits." IACR Transactions on Cryptographic Hardware and Embedded Systems 2024, no. 1 (2023): 157–79. http://dx.doi.org/10.46586/tches.v2024.i1.157-179.

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Over the last decades, fault injection attacks have been demonstrated to be an effective method for breaking the security of electronic devices. Some types of fault injection attacks, like clock and voltage glitching, require very few resources by the attacker and are practical and simple to execute. A cost-effective countermeasure against these attacks is the use of a detector circuit which detects timing violations - the underlying effect that glitch attacks rely on. In this paper, we take a closer look at three examples of such detectors that have been presented in the literature. We demons

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8

Epstein, R. "Gamma-ray bursts and glitching neutron stars." Physics Reports 163, no. 1-3 (1988): 155–66. http://dx.doi.org/10.1016/0370-1573(88)90042-7.

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9

Zhu, Pei-Xin, and Xiao-Ping Zheng. "Glitches and Glitching Clusters in Rotation-powered Pulsars." Astrophysical Journal 978, no. 1 (2024): 49. https://doi.org/10.3847/1538-4357/ad93c9.

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Abstract The study of pulsar glitch phenomena serves as a valuable probe into the dynamic properties of matter under extreme high-density conditions, offering insights into the physics within neutron stars. Providing theoretical explanations for the diverse manifestations observed in different pulsars has proven to be a formidable challenge. By analyzing the distribution of glitch sizes and waiting times, along with the evolution of cumulative glitch sizes over time, we have uncovered a long-term clustering phenomenon for pulsar glitches. This perspective allows us to approach the distinct gli

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10

Polzer, Thomas, Florian Huemer, and Andreas Steininger. "An Experimental Study of Metastability-Induced Glitching Behavior." Journal of Circuits, Systems and Computers 28, supp01 (2019): 1940006. http://dx.doi.org/10.1142/s0218126619400061.

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The increasing number of clock domain crossings in modern systems-on-chip makes the careful consideration of metastability paramount. However, the manifestation of metastability at a flip-flop output is often unduly reduced to late transitions only, while glitches are hardly ever accounted for. In this paper we study the occurrence of glitches resulting from metastability in detail. To this end we propose a measurement circuit whose principle substantially differs from the conventional approach, and by that allows to reliably detect glitches. By means of experimental measurements on an FPGA ta

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11

Ikechukwu Eze, Christian. "Statistical Study of Glitch Behaviours of Glitching Pulsars." International Journal of Astrophysics and Space Science 6, no. 4 (2018): 62. http://dx.doi.org/10.11648/j.ijass.20180604.11.

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12

Ferguson, Andrew. "Mirror World, Minus World: Glitching Nabokov’s Pale Fire." Textual Cultures 8, no. 1 (2014): 101–16. http://dx.doi.org/10.14434/tcv8i1.5052.

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This article considers different experiences available to the reader of Vladimir Nabokov’s Pale Fire by exploring the novel through concepts familiar from videogaming, such as the warp, the glitch, and the Let’s Play, developing particular parallels with the Nintendo game Super Mario Bros. All of these potential modes of experience are comprised in the playerly text, which serves as a conduit linking together a work’s past, present, and future readers.

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13

Kaspi, V. M., A. G. Lyne, R. N. Manchester, S. Johnston, N. D'Amico, and S. L. Shemar. "A young, glitching pulsar near the direction of W28." Astrophysical Journal 409 (June 1993): L57. http://dx.doi.org/10.1086/186859.

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14

Wang, Na, R. N. Manchester, R. Pace, et al. "Glitches in Southern Pulsars." International Astronomical Union Colloquium 177 (2000): 109–10. http://dx.doi.org/10.1017/s0252921100059194.

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AbstractParkes timing observations of 31 mostly young pulsars over nearly nine years are described. A total of 29 glitches were detected, of which 19 are previously unreported. Twelve glitches were seen in PSR J1341–6220, making this the most frequently glitching pulsar known, and the largest known glitch was detected in PSR J1614–5047. Distributions of glitch parameters were investigated.

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15

Schink, Marc, Alexander Wagner, Felix Oberhansl, et al. "Unlock the Door to my Secrets, but don’t Forget to Glitch." IACR Transactions on Cryptographic Hardware and Embedded Systems 2024, no. 2 (2024): 88–129. http://dx.doi.org/10.46586/tches.v2024.i2.88-129.

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In this work, we look into an attack vector known as flash erase suppression. Many microcontrollers have a feature that allows the debug interface protection to be deactivated after wiping the entire flash memory. The flash erase suppression attack exploits this feature by glitching the mass erase, allowing unlimited access to the data stored in flash memory. This type of attack was presented in a confined context by Schink et al. at CHES 2021. In this paper, we investigate whether this generic attack vector poses a serious threat to real-world products. For this to be true, the success rate o

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16

DeDeo, Simon. "AlephZero and mathematical experience." Bulletin of the American Mathematical Society 61, no. 3 (2024): 375–86. http://dx.doi.org/10.1090/bull/1824.

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This essay explores the impact of automated proof construction on three key areas of mathematical cognition: on how we judge the role one piece of mathematics plays in another, on how we make mistakes in reasoning about mathematical objects, and on how we understand what our theorems are truly about. It concludes by speculating on a new form of mathematical experience that these methods could make possible: “glitching”, a game-like search for uncanny consequences of our definitions.

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17

Linghede, Eva, Laura Purdy, and Natalie Barker-Ruchti. "Glitching trans* athletes: possibilities for research and practice in sports coaching." Sports Coaching Review 11, no. 1 (2021): 64–86. http://dx.doi.org/10.1080/21640629.2021.1990656.

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18

Ho, Wynn C. G. "Magnetic field growth in young glitching pulsars with a braking index." Monthly Notices of the Royal Astronomical Society 452, no. 1 (2015): 845–51. http://dx.doi.org/10.1093/mnras/stv1339.

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19

Yan, Yan. "The symmetry energy and incompressibility constrained by the observations of glitching pulsars." Research in Astronomy and Astrophysics 19, no. 5 (2019): 072. http://dx.doi.org/10.1088/1674-4527/19/5/72.

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20

Trax, Shirt. "No more mind games." Organised Sound 6, no. 3 (2001): 185–91. http://dx.doi.org/10.1017/s1355771801003041.

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The Spring sunshine makes the blind a perfect glowing square, clearly much later than the twenty-three minute duration of the live recording I set in motion, as I lay on my friend's bed alone, drunk on vodka and tonic and giddy with big city kicks after the very . . . Manhattan evening I was taken on. It was dark, I was too full of it to take the subway back to Brooklyn, I remember the cab ride over the bridge, no dog to greet me as I unlocked the heavy steel door. I was laughing at Alan Vega complaining about not being allowed to smoke, there was booing . . . ‘Frankie Teardrop’ had been glitc

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21

M.Indu*, S.HasmashruthiA.Nandhini, and N.Megala. "GLITCH-FREE NAND-BASED DIGITALLY CONTROLLED DELAY LINES." INTERNATIONAL JOURNAL OF ENGINEERING SCIENCES & RESEARCH TECHNOLOGY 5, no. 4 (2016): 117–22. https://doi.org/10.5281/zenodo.48842.

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Glitch is an undesired transition that occurs before the signal settles to its intended value. It is an electrical pulse of short duration that is usually the result of a fault or design error, particularly in a digital circuit. The existing Glitch Free NAND-based Digitally Controlled Delay Lines (DCDL) presented some glitching problem which limited their applications. To overcome this limitation new NAND-based DCDL is proposed. This will maintain the same resolution and minimum delay of existing NAND-based DCDL. The proposed DCDL will be working on the basis of two control signals which are u

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22

Espinoza, C. M., A. G. Lyne, and B. W. Stappers. "New long-term braking index measurements for glitching pulsars using a glitch-template method." Monthly Notices of the Royal Astronomical Society 466, no. 1 (2016): 147–62. http://dx.doi.org/10.1093/mnras/stw3081.

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23

Satyanarayana, J. H., and K. K. Parhi. "Theoretical analysis of word-level switching activity in the presence of glitching and correlation." IEEE Transactions on Very Large Scale Integration (VLSI) Systems 8, no. 2 (2000): 148–59. http://dx.doi.org/10.1109/92.831435.

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24

Linghede, Eva. "The promise of glitching bodies in sport: a posthumanist exploration of an intersex phenomenon." Qualitative Research in Sport, Exercise and Health 10, no. 5 (2018): 570–84. http://dx.doi.org/10.1080/2159676x.2018.1479980.

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25

Lange, Daniel. "Specters of Probability:Dr. Mabuse, der Spielerand Glitching Visions of Data." Monatshefte 117, no. 1 (2025): 1–17. https://doi.org/10.3368/m.117.1.1.

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26

Israel, G. L., D. Götz, S. Zane, S. Dall'Osso, N. Rea, and L. Stella. "Linking the X-ray timing and spectral properties of the glitching AXP 1RXS J170849-400910." Astronomy & Astrophysics 476, no. 2 (2007): L9—L12. http://dx.doi.org/10.1051/0004-6361:20078215.

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27

Gao, Chong-Yu, and Jun-Jie Wei. "A Comparative Analysis of Scale-invariant Phenomena in Repeating Fast Radio Bursts and Glitching Pulsars." Astrophysical Journal 968, no. 1 (2024): 40. http://dx.doi.org/10.3847/1538-4357/ad4a55.

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Abstract The recent discoveries of a remarkable glitch/antiglitch accompanied by fast radio burst (FRB)-like bursts from the Galactic magnetar SGR J1935+2154 have revealed the physical connection between the two. In this work, we study the statistical properties of radio bursts from the hyperactive repeating source FRB 20201124A and of glitches from the pulsar PSR B1737–30. For FRB 20201124A, we confirm that the probability density functions of fluctuations of energy, peak flux, duration, and waiting time well follow the Tsallis q-Gaussian distribution. The derived q values from q-Gaussian dis

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28

Carlin, J. B., and A. Melatos. "Autocorrelations in pulsar glitch waiting times and sizes." Monthly Notices of the Royal Astronomical Society 488, no. 4 (2019): 4890–96. http://dx.doi.org/10.1093/mnras/stz2014.

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ABSTRACT Among the five pulsars with the most recorded rotational glitches, only PSR J0534+2200 is found to have an autocorrelation between consecutive glitch sizes that differs significantly from zero (Spearman correlation coefficient ρ = −0.46, p-value = 0.046). No statistically compelling autocorrelations between consecutive waiting times are found. The autocorrelation observations are interpreted within the framework of a predictive meta-model describing stress release in terms of a state-dependent Poisson process. Specific combinations of size and waiting time autocorrelations are identif

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29

Ho, Wynn C. G., Cristóbal M. Espinoza, Danai Antonopoulou, and Nils Andersson. "Pinning down the superfluid and measuring masses using pulsar glitches." Science Advances 1, no. 9 (2015): e1500578. http://dx.doi.org/10.1126/sciadv.1500578.

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Pulsars are known for their superb timing precision, although glitches can interrupt the regular timing behavior when the stars are young. These glitches are thought to be caused by interactions between normal and superfluid matter in the crust of the star. However, glitching pulsars such as Vela have been shown to require a superfluid reservoir that greatly exceeds that available in the crust. We examine a model in which glitches tap the superfluid in the core. We test a variety of theoretical superfluid models against the most recent glitch data and find that only one model can successfully

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30

Zhou, Shiqi, Erbil Gügercinoğlu, Jianping Yuan, Mingyu Ge, and Cong Yu. "Pulsar Glitches: A Review." Universe 8, no. 12 (2022): 641. http://dx.doi.org/10.3390/universe8120641.

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∼6% of all known pulsars have been observed to exhibit sudden spin-up events, known as glitches. For more than fifty years, these phenomena have played an important role in helping to understand pulsar (astro)physics. Based on the review of pulsar glitches search method, the progress made in observations in recent years is summarized, including the achievements obtained by Chinese telescopes. Glitching pulsars demonstrate great diversity of behaviours, which can be broadly classified into four categories: normal glitches, slow glitches, glitches with delayed spin-ups, and anti-glitches. The ma

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31

Jiménez-Naharro, Raúl, Fernando Gómez-Bravo, Jonathan Medina-García, Manuel Sánchez-Raya, and Juan Gómez-Galán. "A Smart Sensor for Defending against Clock Glitching Attacks on the I2C Protocol in Robotic Applications." Sensors 17, no. 4 (2017): 677. http://dx.doi.org/10.3390/s17040677.

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32

Modafferi, Luana M., Joan Moragues, and David Keitel. "Search for long-duration transient gravitational waves from glitching pulsars during LIGO—Virgo third observing run." Journal of Physics: Conference Series 2156, no. 1 (2021): 012079. http://dx.doi.org/10.1088/1742-6596/2156/1/012079.

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Abstract Pulsars are spinning neutron stars which emit an electromagnetic beam. We expect pulsars to slowly decrease their rotational frequency. However, sudden increases of the rotational frequency have been observed from different pulsars. These events are called “glitches” and they are followed by a relaxation phase with timescales from days to months. Gravitational wave (GW) emission may follow these peculiar events. We give an overview of an analysis of GW data from the Advanced LIGO and Virgo third observing run (O3) searching for transient GW signals lasting hours to months after glitch

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33

Hujeirat, Ahmad A., and Ravi Samtaney. "Glitching Pulsars: Unraveling the Interactions of General Relativistic and Quantum Fields in the Strong Field Regimes." Journal of Modern Physics 10, no. 14 (2019): 1696–712. http://dx.doi.org/10.4236/jmp.2019.1014111.

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34

Shaw, B., M. J. Keith, A. G. Lyne, et al. "The slow rise and recovery of the 2019 Crab pulsar glitch." Monthly Notices of the Royal Astronomical Society: Letters 505, no. 1 (2021): L6—L10. http://dx.doi.org/10.1093/mnrasl/slab038.

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ABSTRACT We present updated measurements of the Crab pulsar glitch of 2019 July 23 using a data set of pulse arrival times spanning ∼5 months. On MJD 58687, the pulsar underwent its seventh largest glitch observed to date, characterized by an instantaneous spin-up of ∼1 μHz. Following the glitch, the pulsar’s rotation frequency relaxed exponentially towards pre-glitch values over a time-scale of approximately 1 week, resulting in a permanent frequency increment of ∼0.5 μHz. Due to our semicontinuous monitoring of the Crab pulsar, we were able to partially resolve a fraction of the total spin-u

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35

Clark, Colin J., Jason Wu, Holger J. Pletsch, and Lucas Guillemot. "The Einstein@Home Survey for Gamma-ray Pulsars." Proceedings of the International Astronomical Union 13, S337 (2017): 21–24. http://dx.doi.org/10.1017/s1743921317009231.

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AbstractSince the launch of the Fermi Gamma-ray Space Telescope in 2008, the onboard Large Area Telescope (LAT) has detected gamma-ray pulsations from more than 200 pulsars. A large fraction of these remain undetected in radio observations, and could only be found by directly searching the LAT data for pulsations. However, the sensitivity of such “blind” searches is limited by the sparse photon data and vast computational requirements. In this contribution we present the latest large-scale blind-search survey for gamma-ray pulsars, which ran on the distributed volunteer computing system, Einst

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36

Shiwani, Dod. "Modified Booth Dadda Multiplier using Carry Look ahead adder Design and Implementation." International Journal of Computer Science & Engineering Technology 7, no. 3 (2016): 86–93. https://doi.org/10.5281/zenodo.48793.

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This paper proposes a novel 8X8 bit Modified Booth Dadda Multiplier architecture which is an improved version of Modified Booth Wallace Multiplier. The idea involves the generation of partial products using Modified Booth Algorithm. The addition of these partial products is done using Dadda Tree which is hierarchically divided into two levels. The proposed Modified Booth Dadda Multiplier provides significant reduction in area and complexity in comparison to Modified Booth Wallace Multiplier as Dadda Tree requires less number of half adders and full adders as compared to Wallace Tree. The propo

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37

Espinoza, C. M., D. Antonopoulou, R. Dodson, M. Stepanova, and A. Scherer. "Small glitches and other rotational irregularities of the Vela pulsar." Astronomy & Astrophysics 647 (March 2021): A25. http://dx.doi.org/10.1051/0004-6361/202039044.

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Context. Glitches are sudden increases in the rotation rate ν of neutron stars, which are thought to be driven by the neutron superfluid inside the star. The Vela pulsar presents a comparatively high rate of glitches, with 21 events reported since observations began in 1968. These are amongst the largest known glitches (17 of them have sizes Δν/ν ≥ 10−6) and exhibit very similar characteristics. This similarity, combined with the regularity with which large glitches occur, has turned Vela into an archetype of this type of glitching behaviour. The properties of its smallest glitches, on the oth

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38

Stuart, Caleb. "Damaged Sound: Glitching and Skipping Compact Discs in the Audio of Yasunao Tone, Nicolas Collins and Oval." Leonardo Music Journal 13 (December 2003): 47–52. http://dx.doi.org/10.1162/096112104322750782.

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From the initial release of the CD in 1982, artists have tampered with the system to test it, compose with it and sample from it. The author examines the use of the cracked and manipulated CD in the work of Yasunao Tone, Nicolas Collins and Oval in relation to their differing approaches and the role of the CD in sound expansion. Tone and Collins are interested in indeterminacy and the benevolent catastrophe in composition, while Oval's process has more in common with pop production and studio practices.

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Singha, Jaikhomba, Avishek Basu, M. A. Krishnakumar, Bhal Chandra Joshi, and P. Arumugam. "A real-time automated glitch detection pipeline at Ooty Radio Telescope." Monthly Notices of the Royal Astronomical Society 505, no. 4 (2021): 5488–96. http://dx.doi.org/10.1093/mnras/stab1640.

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ABSTRACT Glitches are the observational manifestations of superfluidity inside neutron stars. The aim of this paper is to describe an automated glitch detection pipeline, which can alert the observers on possible real-time detection of rotational glitches in pulsars. Post alert, the pulsars can be monitored at a higher cadence to measure the post-glitch recovery phase. Two algorithms, namely median absolute deviation and polynomial regression, have been explored to detect glitches in real time. The pipeline has been optimized with the help of simulated timing residuals for both the algorithms.

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40

Edwards, Sarah. "On the Cusp of the Post-Internet Essay: Lisa Robertson’s Nilling (2012)." CounterText 9, no. 3 (2023): 339–55. http://dx.doi.org/10.3366/count.2023.0319.

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In the wake of mass digital transformations, this article turns to the question of a corresponding aesthetic transformation in literary works. Although previous studies have focussed on novels and poetry, this article turns its attention towards the essay genre by taking Lisa Robertson’s collection Nilling (2012) as its primary case-study. It contextualises Nilling within Robertson’s career to reveal her evolving towards the incorporation and depiction of technology in her writing, and reveals how the digital interrupts the collection as a flickering image or a glitching presence that is simul

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41

Zhu, Weiwei, and Victoria M. Kaspi. "SEARCHING FOR X-RAY VARIABILITY IN THE GLITCHING ANOMALOUS X-RAY PULSAR 1E 1841–045 IN KES 73." Astrophysical Journal 719, no. 1 (2010): 351–56. http://dx.doi.org/10.1088/0004-637x/719/1/351.

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42

Espinoza, Cristobal, Danai Antonopoulou, Alessandro Patruno, Ben Stappers, and Anna Watts. "Characterizing glitches and timing irregularities in pulsars and magnetars." Proceedings of the International Astronomical Union 8, S291 (2012): 381. http://dx.doi.org/10.1017/s1743921312024192.

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AbstractAs the quantity and quality of timing data improves, we have reached the point at which the difference between timing noise and small glitches is unclear. As a consequence, the number of events reported as glitches which show unusual properties, quite different to those of giant glitches, has increased. For example, there is now a substantial population of glitches that apparently involve a decrease in spin-down rate rather than an increase. Motivated by the theoretical implications of such a result, we are conducting a detailed review of how glitches are detected and characterised. We

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43

Schnabel, Marc Aurel, and Blaire Haslop. "Glitch architecture." International Journal of Architectural Computing 16, no. 3 (2018): 183–98. http://dx.doi.org/10.1177/1478077118792376.

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Architectural designs are visualised on computer screens through arrays of pixels and vectors. These representations differ from the reality of buildings, which over time will unavoidably age and decay. How, then, do digital designs age over time? Do we interpret glitching as a sudden malfunction or fault in the computation of the design’s underlying data, or as digital decay resulting not from the wear and tear of tangible materials but from the decomposition of the binary code, or from system changes that cannot appropriately interpret the data? By exploring a series of experimental design p

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44

Jacobo, Sandra, Edward Rivero, Kris Gutiérrez, and Kimiko Ryokai. "Playing with design flaws: Youth transgressive play and multimodal learning in VR ecologies." Multimodality & Society 5, no. 2 (2025): 245–67. https://doi.org/10.1177/26349795251331037.

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This paper builds on prior work Ryokai and colleagues from 2022, examining youths’ design processes, perspective-taking, and collaboration with VR SandScape—a mixed-reality system combining a spatial augmented reality (SAR) sandbox with a virtual reality (VR) head-mounted display (HMD). The current case study examines how youths’ transgressive play—a form of play challenging established rules, norms, and expectations through creative manipulation of multiple meaning-making modes—expands the boundaries of possibility for multimodal learning within VR. By attuning to youths’ ingenuity and agency

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45

Abbott, R., T. D. Abbott, S. Abraham, et al. "Constraints from LIGO O3 Data on Gravitational-wave Emission Due to R-modes in the Glitching Pulsar PSR J0537–6910." Astrophysical Journal 922, no. 1 (2021): 71. http://dx.doi.org/10.3847/1538-4357/ac0d52.

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Abstract We present a search for continuous gravitational-wave emission due to r-modes in the pulsar PSR J0537–6910 using data from the LIGO–Virgo Collaboration observing run O3. PSR J0537–6910 is a young energetic X-ray pulsar and is the most frequent glitcher known. The inter-glitch braking index of the pulsar suggests that gravitational-wave emission due to r-mode oscillations may play an important role in the spin evolution of this pulsar. Theoretical models confirm this possibility and predict emission at a level that can be probed by ground-based detectors. In order to explore this scena

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46

Zubieta, Ezequiel, Ryan Missel, Susana B. Araujo Furlan, et al. "Study of the 2024 major Vela glitch at the Argentine Institute of Radioastronomy." Astronomy & Astrophysics 698 (May 28, 2025): A72. https://doi.org/10.1051/0004-6361/202554098.

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Context. We report here on new results of the systematic monitoring of southern glitching pulsars at the Argentine Institute of Radioastronomy. In particular, we study in this work the new major glitch in the Vela pulsar (PSR J0835−4510) that occurred on 2024 April 29. Aims. We aim to thoroughly characterise the rotational behaviour of the Vela pulsar around its last major glitch and investigate the statistical properties of its individual pulses around the glitch. Methods. We characterise the rotational behaviour of the pulsar around the glitch through the pulsar timing technique. We measured

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Hujeirat, Ahmad A., and Peter Berczik. "The Origin of the Flat Rotation Curves in Spiral Galaxies: The Hidden Roles of Glitching SMDEOs and Emission of Gravitational Waves." Journal of Modern Physics 15, no. 10 (2024): 1523–42. http://dx.doi.org/10.4236/jmp.2024.1510063.

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Ho, Wynn C. G., Cristóbal M. Espinoza, Zaven Arzoumanian, et al. "Return of the Big Glitcher: NICER timing and glitches of PSR J0537−6910." Monthly Notices of the Royal Astronomical Society 498, no. 4 (2020): 4605–14. http://dx.doi.org/10.1093/mnras/staa2640.

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ABSTRACT PSR J0537−6910, also known as the Big Glitcher, is the most prolific glitching pulsar known, and its spin-induced pulsations are only detectable in X-ray. We present results from analysis of 2.7 yr of NICER timing observations, from 2017 August to 2020 April. We obtain a rotation phase-connected timing model for the entire time span, which overlaps with the third observing run of LIGO/Virgo, thus enabling the most sensitive gravitational wave searches of this potentially strong gravitational wave-emitting pulsar. We find that the short-term braking index between glitches decreases tow

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Gügercinoğlu, E., M. Y. Ge, J. P. Yuan, and S. Q. Zhou. "Glitches in four gamma-ray pulsars and inferences on the neutron star structure." Monthly Notices of the Royal Astronomical Society 511, no. 1 (2022): 425–39. http://dx.doi.org/10.1093/mnras/stac026.

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ABSTRACT We present timing solutions from the Fermi-LAT observations of gamma-ray pulsars PSR J0835 − 4510 (Vela), PSR J1023−5746, PSR J2111+4606, and PSR J2229+6114. Data ranges for each pulsar extend over a decade. From data analysis, we have identified a total of 20 glitches, 11 of which are new discoveries. Among them, 15 glitches are large ones with Δν/ν ≳ 10−6. PSR J1023−5746 is the most active pulsar with glitch activity parameter being Ag = 14.5 × 10−7 yr−1 in the considered data span and should be a target for frequently glitching Vela-like pulsars in future observations. We have done

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Pradhan, Bikram Keshari, Dhruv Pathak, and Debarati Chatterjee. "Constraining Nuclear Parameters Using Gravitational Waves from f-mode Oscillations in Neutron Stars." Astrophysical Journal 956, no. 1 (2023): 38. http://dx.doi.org/10.3847/1538-4357/acef1f.

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Abstract Gravitational waves (GWs) emanating from unstable quasi-normal modes in neutron stars (NSs) could be accessible with the improved sensitivity of the current GW detectors or with the next-generation GW detectors and, therefore, can be employed to study the NS interior. Assuming f-mode excitation in isolated pulsars with typical energy of pulsar glitches and considering potential f-mode GW candidates for A+ (upgraded LIGO detectors operating at fifth observing run design sensitivity) and Einstein Telescope (ET), we demonstrate the inverse problem of NS asteroseismology within a Bayesian

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